SR XMon Mar 21 17:13:56 2016xrt_webfacula.cfa.harvard.edu x86_64darwin7.1.1R ***************************************************************** NOTICE: IDL Save/Restore files embody unpublished proprietary information about the IDL program. Reverse engineering of this file is therefore forbidden under the terms of the IDL End User License Agreement (IDL EULA). All IDL users are required to read and agree to the terms of the IDL EULA at the time that they install IDL. Software that reads or writes files in the IDL Save/Restore format must have a license from ITT Visual Information Solutions explicitly granting the right to do so. In this case, the license will be included with the software for your inspection. Please report software that does not have such a license to ITT Visual Information Solutions (info@ittvis.com). *****************************************************************  'D CATALOG_TABLE4נ  0@P`p 0@P`pIDSTART_ENDXYRATINGTYPEERUPTIONSYMMETRY DIRECTIONTWISTWRITHETHREADSCAVITYFLARE FLARE_LINKCMECME_LINKBOXAIA_FOV HEK_TITLE HEK_OBSERVER HEK_COMMENTSHEK_LINK CAT_OBSERVER CAT_COMMENTSCAT_LINK00002010-04-24T05:48:232010-04-24T07:14:482871110.50--------N---[-203,777,-160,382][1567,3486,1694,2773]Promimnence eruptionKarel SchrijverhhErupting prominence slightly within limb, showing two disjoint arms, and significant downfalling plasma.@@ivo://helio-informatics.org/FE304_KarelSchrijver_20100426_144313McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=000000012010-04-30T19:33:542010-05-01T02:56:08-5541790.0-------- C2.2|C5.7http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2010/04/30/gev_20100430_1928/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2010/05/01/gev_20100501_0134/index.html--[-975,-132,522,-164][166,2085,1807,2886]None Neal HurlburtGGNice filament eruption on disk that appears to trigger C flare on limb.>>ivo://helio-informatics.org/FE304_NealHurlburt_20100504_190608McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=000100022010-04-30T22:00:062010-05-01T01:20:10-4552400.0--------N---[-179,-730,477,3][651,1930,2089,2808]Filament eruptionKarel SchrijverFilament eruption@@ivo://helio-informatics.org/FE171_KarelSchrijver_20100501_175540McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=000200032010-05-04T05:00:062010-05-04T07:40:23-95-4100.0--------N---[-864,673,-835,15][608,3169,645,2084]''Filament Eruption Near Central Meridian Ralph Seguin11Nice filament eruption near the central meridian.==ivo://helio-informatics.org/FE304_RalphSeguin_20100518_210611Reeves-::http://aia.cfa.harvard.edu/filament/index.html?search=000300042010-05-05T15:16:002010-05-06T02:13:51501-4210.0--------N---[-246,1248,87,-929][1606,4095,647,2046]Filament Eruption CascadeRtimmonsbbOne on-disk filament eruption with associated wave seems to trigger an on-limb eruption. Very nice>>ivo://helio-informatics.org/FE171_NealHurlburt_20100507_224704Schanche-::http://aia.cfa.harvard.edu/filament/index.html?search=000400052010-05-05T16:00:022010-05-05T17:56:02221-3540.0--------N---[88,354,-243,-464][1777,3056,1099,1818]Filament eruption and wave Ralph Seguin[[Nice filament eruption with a good associated wave that seems to trigger the M class flare.>>ivo://helio-informatics.org/FE193_NealHurlburt_20100505_224054McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=000500062010-05-05T16:00:022010-05-05T17:58:37199-3780.0--------N---[-197,595,11,-768][1420,3339,878,1957]Nice filament eruption and wave Ralph SeguinA nice filament eruption in the south with an associated wave. There is an M-class flare in the northern hemisphere that follows shortly after.in AR11069...>>ivo://helio-informatics.org/FE193_NealHurlburt_20100506_221856McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=000600072010-05-06T05:50:052010-05-06T07:29:41347-3930.0--------N---[194,499,-288,-498][1986,3265,1034,1753]Small filament eruption Ralph SeguinSmall filament eruption.@@ivo://helio-informatics.org/FE171_KarelSchrijver_20100507_002900McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=000700082010-05-08T01:58:252010-05-08T08:13:311806590.0-------- B4.3|C9.3http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2010/05/08/gev_20100508_0318/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2010/05/08/gev_20100508_0451/index.html--[-877,1237,75,1244][572,4095,2114,4095] Nice filament eruption with wave Ralph SeguinA nice filament eruption with a fast moving wave traveling across the disk. This eruption is followed by several more very nice eruptions from the save active region, also with associated waves.==ivo://helio-informatics.org/FE171_RalphSeguin_20100510_233043McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=000800092010-05-10T09:25:042010-05-10T11:59:328047120.0--------1?---[633,975,885,539][2749,4028,2875,3594]Compact eruption on limbRtimmons\\Nice compact filament eruption on the limb. Shows good field line movement and oscillation.>>ivo://helio-informatics.org/FE304_NealHurlburt_20100510_185546McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=000900102010-05-11T04:13:012010-05-11T08:16:196058270.0--------N---[408,801,1013,641][2416,3695,3067,3786]%%Limb Eruption with Absorption Feature Ralph SeguinSmall interesting eruption the limb with a dark absorption blob/feature. Very shortly after the limb eruption, you can see another (the same?) eruption a bit farther in.==ivo://helio-informatics.org/FE171_RalphSeguin_20100511_200122McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=001000112010-05-12T00:00:052010-05-12T05:36:358494970.0--------1?---[623,1076,674,320][2816,4095,2517,3236]Small Eruption Ralph SeguinQQSmall eruption near limb that precedes a much larger eruption in the same region.==ivo://helio-informatics.org/FE211_RalphSeguin_20100512_165304McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=001100122010-05-12T12:58:492010-05-12T15:59:059144390.0--------1?---[648,1179,761,117][2176,4095,2240,3319]Nice fillament eruption on limb Ralph Seguin((Very nice filament eruption on the limb.==ivo://helio-informatics.org/FE171_RalphSeguin_20100512_164405McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=001200132010-05-18T14:00:052010-05-18T16:00:053339611.0PC?C?A?RNNNNN-N-[237,429,1031,891][1964,3243,3290,4009]Small Eruption Near Pole Ralph Seguin66A small filament eruption near the north polar region.==ivo://helio-informatics.org/FE211_RalphSeguin_20100518_200730McCauleyMcCauley: Jet-like eruption.::http://aia.cfa.harvard.edu/filament/index.html?search=001300142010-05-25T02:18:402010-05-25T04:45:23-9594503.7QS?FANRYNY?D?N-0744FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/05/CME0025/CME.html[-1125,-793,524,376][0,1279,2439,3158]''Filament erupting off northeastern limb Mark Cheung55Filament (blue, 304) erupting off the northeastern limb. The southern end of the filament is seen to detach and rise while the northern end remains anchored and temporarily brighten in 304 (ribbon-like structures). The coronal structures seen in 171 (red) and 211 (green) are disrupted by the rising filament.<>ivo://helio-informatics.org/FE171_NariakiNitta_20100712_201445McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=002900302010-06-13T01:00:052010-06-13T12:24:436108851.5PCPARNNYYN-0351FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/06/CME0020/CME.html[178,1042,1127,644][2105,4024,2984,4063]33Filament eruption and coronal cavity lift-off (CME) Thomas BergerModerate-sized filament eruption on NW limb. Lower boundary of coronal cavity is very sharply defined. Coronal cavity outline is seen to rise and escape to the NW (obvious CME). Backflow mass is seen to impact the disk about 300 arcsec to the East.;;ivo://helio-informatics.org/FE304_TomBerger_20100614_174154McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=003000312010-06-15T00:00:002010-06-15T23:59:36-7377671.5QSPARYNYYN-0432FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/06/CME0025/CME.html[-435,-1039,568,965][180,1459,2966,3685]((Filament eruption off the northeast limb Thomas BergerThe erupting filament can be easily seen in 304. In 171, large-scale configuration of the loops around the filament can be seen.;;ivo://helio-informatics.org/FE304_TomBerger_20100618_162726McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=003100322010-06-16T13:45:002010-06-16T23:52:32-10394181.5QSFARYNYNN-0141FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/06/CME0027/CME.html[-733,-1345,221,615][0,1279,2385,3104]Filament eruption Mark Cheung((Filament erupting off the northeast limb<>A larger filament erupts with reconnection at both footpoints.==ivo://helio-informatics.org/FE193_RalphSeguin_20100706_182921McCauleyffMcCauley: Untwisting apparent at the eastern footpoint. No CME entry due to missing CACTus/LASCO data.::http://aia.cfa.harvard.edu/filament/index.html?search=005400552010-07-06T08:18:592010-07-06T12:00:187562742.0ARPASYY?NNB1.0OOhttp://www.lmsal.com/solarsoft/last_events_20100709_1002/gev_20100706_1002.htmlY?-[647,864,379,169][2668,3947,2145,2864]Small Eruption with Dimming Ralph Seguin55A small filament erupts with compact, strong dimming.==ivo://helio-informatics.org/FE171_RalphSeguin_20100706_182117McCauleyGGMcCauley: Nice EUV wave. No CME entry due to missing CACTus/LASCO data.::http://aia.cfa.harvard.edu/filament/index.html?search=005500562010-07-08T05:55:172010-07-08T18:59:26990162.0QSPANR?YNYNN-Y?-[721,1259,435,-403][1615,4095,1378,2771]Small Eruption with Rain Ralph Seguin{{Small filament eruption near the limb with the material flowing southward and falling back in and coronal rain at the end.==ivo://helio-informatics.org/FE304_RalphSeguin_20100708_231506McCauley88McCauley: No CME entry due to missing CACTus/LASCO data.::http://aia.cfa.harvard.edu/filament/index.html?search=005600572010-07-17T18:17:422010-07-18T15:36:13-2833881.0--------N---[-737,172,655,121][618,2537,2155,3234]((Large filament eruption/two ribbon flareWei LiuLarge filament eruption toward observer (slightly off to the east), followed by a two ribbon flare, clearly shows an arcade of post-flare loops, giant sigmoid (1/2 solar radiis), decreasing shear angle of flare loops with time.88ivo://helio-informatics.org/FE304_WeiLiu_20100720_005007McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=005700582010-07-19T01:40:232010-07-19T17:13:362285041.0--------N---[16,439,764,244][1468,3387,2349,3428]$$Filament Eruption Near Emerging Flux Ralph SeguinA filament erupts to the west of an emerging flux region. Nice dimming. The strong red and green dots are the underlying magnetogram.==ivo://helio-informatics.org/FE211_RalphSeguin_20100719_220850McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=005800592010-07-20T00:00:282010-07-20T10:52:363546801.0--------3?---[181,527,435,925][1679,3598,2642,3721]Ephemeral region jet/eruptionKarel SchrijverEruption from a small emerging ephemeral region, observed also in 211/193/171, but clearly of much greater extent when seen in the 304 channel.@@ivo://helio-informatics.org/FE304_KarelSchrijver_20100720_150329McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=005900602010-07-20T01:34:122010-07-20T10:14:47-758-4952.0--------3?---[-623,-892,-325,-664][146,1425,864,1583]Filament eruption and flareKarel Schrijver##Repeated activation of a filament in what looks like a decayed, dispersed small active region. One of the activations is associated with a flare, with post-eruption arcade. The corona SE of the region appears to dim and/or change thermal structure for a considerable time after the eruption.@@ivo://helio-informatics.org/FE193_KarelSchrijver_20100720_145357McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=006000612010-07-20T07:04:072010-07-20T08:34:54-5343692.0--------N---[-457,-610,330,408][519,1798,2304,3023]Filament eruption in ERKarel Schrijver..Fimalent eruption in small QS ephemeral region@@ivo://helio-informatics.org/FE171_KarelSchrijver_20100720_144228McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=006100622010-07-21T00:00:292010-07-21T10:52:12-7541002.0--------N---[-634,-874,231,-31][152,1431,1855,2574]FIlament eruptionWei Liu==FIlarment eruption seen as absorption features at 193 and 21188ivo://helio-informatics.org/FE193_WeiLiu_20100729_202902McKillop-::http://aia.cfa.harvard.edu/filament/index.html?search=006200632010-07-26T06:46:292010-07-26T09:03:116118282.0QSCSRNNNDN-N?-[477,744,1048,607][2106,4025,2888,3967] loop eruptionJuan Martinezsykora((thin filament eruption, behind the limb?DDivo://helio-informatics.org/FE211_JuanMartinezSykora_20100727_230901McCauleyMcCauley: LASCO data gap may have precluded a CME entry. The obvious cavity is associated with the neighboring filament in the foreground, but the erupting one shows signs of a cavity during the eruption in the 171 channel.::http://aia.cfa.harvard.edu/filament/index.html?search=00630064-----1---------------Juan MartinezsykoraMMslow mass eruption with a lot of dynamics of a very large filament structure.DDivo://helio-informatics.org/FE304_JuanMartinezSykora_20100729_202319---00652010-07-27T15:30:252010-07-27T20:24:05-8935423.0IP?C?ANRYNN?D?N-N?-[-1044,-743,793,292][0,1919,2413,3492]filament erutionJuan Martinezsykora""filament eruption with kink motionDDivo://helio-informatics.org/FE304_JuanMartinezSykora_20100729_205720McCauley88McCauley: LASCO data gap may have precluded a CME entry.::http://aia.cfa.harvard.edu/filament/index.html?search=006500662010-07-28T00:00:312010-07-28T17:57:10-776-5984.0QSFARYNYYN-0227JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2010/07/CME0018/CME.html[-340,-1212,-251,-945][0,1919,512,1591]Prominence eruptionKarel SchrijverProminence eruption@@ivo://helio-informatics.org/FE304_KarelSchrijver_20100729_174021McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=006600672010-07-29T00:00:292010-07-29T04:00:08-9615694.0IPP?RY?NYDN-Y-[-1189,-733,786,353][0,1279,2638,3357]Filament eruptionKarel SchrijverFilament eruption@@ivo://helio-informatics.org/FE171_KarelSchrijver_20100729_174617McCauleyaaMcCauley: There was a minor CME observed by LASCO, but it didn't make it into the CACTus catalog.::http://aia.cfa.harvard.edu/filament/index.html?search=00670068-----1---------------Karel SchrijverFilament eruption@@ivo://helio-informatics.org/FE304_KarelSchrijver_20100729_175020---0069-----1--------------- Thomas Berger<>ivo://helio-informatics.org/FE304_NealHurlburt_20100827_175146---00792010-08-27T01:59:182010-08-27T13:59:22636-7124.7QSPAR?Y?YDB4.7OOhttp://www.lmsal.com/solarsoft/last_events_20100830_1505/gev_20100827_0436.html0353JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2010/08/CME0025/CME.html[254,1018,-387,-1036][2469,3748,503,1222]Filament Eruption Neal HurlburtAAA nice filament eruption which may well be associated with a CME.>>ivo://helio-informatics.org/FE171_NealHurlburt_20100827_174000McCauleyNNMcCauley: An eruption to the north appears to tigger the fast rise of this one::http://aia.cfa.harvard.edu/filament/index.html?search=007900802010-09-04T12:46:182010-09-04T21:26:279251002.0IPPASN?NY?NB2.5OOhttp://www.lmsal.com/solarsoft/last_events_20100908_0919/gev_20100904_1714.html0422FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/09/CME0012/CME.html[662,1188,368,-168][2176,4095,1675,2754]Filament eruption Thomas BergerKKFilament eruption from AR 11101. Coronal arcade and flare ribbon formation.;;ivo://helio-informatics.org/FE171_TomBerger_20100920_221217McCauleyNNMcCauley: An eruption to the north appears to tigger the fast rise of this one::http://aia.cfa.harvard.edu/filament/index.html?search=008000812010-09-06T03:49:072010-09-06T13:32:448957043.0AR?P?A?RYYNDN-0416FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/09/CME0017/CME.html[414,1375,378,1030][2176,4095,2682,3761]Off-limb filament eruption Marc DerosaEEOff-limb filament eruption that blows a hole in the overlying corona.<>ivo://helio-informatics.org/FE171_NariakiNitta_20101117_235339SuMcCauley: CACTus didn't register an event that is obviously associated, but possibly associated material can be seen in this entry: http://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/11/CME0029/CME.html Su: A small low-lying filament eruption was disturbed by the one overlying on it::http://aia.cfa.harvard.edu/filament/index.html?search=011301142010-11-17T00:00:102010-11-17T03:09:197408442.5QSPSRY?NYYN-N-[627,854,1028,660][2643,3922,3095,3814]''Filament eruption off northwestern limb Mark CheungThe gravitational draining of filament material (304, red) does not seem cause footpoint brightening. This suggests the filament was located beyond the limb.< minor CME Nariaki NittaFilament eruption due possibly to kink instability. This type of eruption is often not successful. But there was at least a CME, althugh a minor one - in the height range of 2-6 Rsun, the CME got accelerated from 180 km/s to 420 km/s. Surprisingly this interesting event has not been in the knowledgebase, although it was used in presentations by Nitta (AGU 2010 Fall) and Wei Liu (SPD 2011) and possibly more.99ivo://helio-informatics.org/FEMET_halocme_20111122_212606Su==Su: A beautiful standard kink appears during a quick eruption::http://aia.cfa.harvard.edu/filament/index.html?search=012601272010-12-11T05:12:202010-12-11T13:30:46654471.5IPP?SRNNNNN-N-[-283,413,700,194][1517,2796,2434,3153]Filament eruptionAnna MalanushenkoA filament eruption near AR 11133, immediatly following a smaller scale eruption nearby and immediately preceding a filament eruption near AR 11131.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20101217_011004SuggSu: Mass is seen to lift up from one leg and fall back on another leg of the filament, partial eruption::http://aia.cfa.harvard.edu/filament/index.html?search=012701282010-12-12T00:00:092010-12-12T11:18:42-149023.5PCFS?R?NYNN-0349FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/12/CME0025/CME.html[-741,713,1169,634][813,3236,2734,4095]Filament eruption on the N limbAnna Malanushenko Filament eruption on the N limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20101217_022741SuMcCauley: CME entry also includes a separate (but related?) event to the south. Su: A rolling prominence erupts on the polar-crown, vertical threads flowing along horizontal bright loops at 171::http://aia.cfa.harvard.edu/filament/index.html?search=012801292010-12-14T00:00:102010-12-14T20:44:417915324.5IPFARY?NYN C2.3|C2.3http://www.lmsal.com/solarsoft/last_events_20101217_1041/gev_20101214_1445.html|http://www.lmsal.com/solarsoft/last_events_20101217_1041/gev_20101214_1503.html1059FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/12/CME0034/CME.html[72,1510,128,936][1700,4095,2262,3607]Lifted Filament Eruption Thomas BergerFilament eruption associated with C2.3 flare. Apparent flux rope from flare "lifts" the filament up and then the pair of them erupt with very high velocity. The filament's northern leg "collides" with the "surface" to create a small after-flare>>ivo://helio-informatics.org/FE171_ThomasBerger_20101215_002708SuSu: One leg of this filament lifts up slowly due to the disturbance of the nearby AR filament activation, then ends up with a quick eruption::http://aia.cfa.harvard.edu/filament/index.html?search=01290130-----1---------------Karel SchrijverLarge filament eruption@@ivo://helio-informatics.org/FE171_KarelSchrijver_20101217_010421---01312010-12-14T13:00:052010-12-14T23:59:00-5369344.0QSP?RYNYYN-1059FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/12/CME0034/CME.html[-848,-224,589,1279][133,2176,2948,4095]Filament eruption over NE limbKarel SchrijverFilament eruption over NE limb@@ivo://helio-informatics.org/FE193_KarelSchrijver_20101217_010621Su99McCauley: The CME entry is dominated by a larger event on the other limb (catalog ID #130), but it also captures this event. Su: A NE prominence with a clear cavity in 171 A image arises and then erupts with most material falling back on the surface excellent U shape prominene with tornado-like vertical threads::http://aia.cfa.harvard.edu/filament/index.html?search=013101322010-12-16T04:43:352010-12-16T12:05:401295942.0QSFARNNYN1?-0425FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/12/CME0039/CME.html[491,-234,303,885][1623,2902,2679,3398]44Quiet-Sun filament eruption and post-eruption arcadeKarel Schrijver55Quiet-Sun filament eruption adnd post-eruption arcade@@ivo://helio-informatics.org/FE193_KarelSchrijver_20101217_012725SuffSu: One leg of a filament rises quietly and most material falls back on the surface in the 304 A image::http://aia.cfa.harvard.edu/filament/index.html?search=013201332010-12-17T00:00:092010-12-17T15:00:488184842.5IPP?SRNNYNN-N-[1261,375,741,227][2176,4095,2315,3394]Small filament eruption Marc Derosa%%Small filament eruption on west limb.< CME Nariaki Nitta33No GOES X-ray flare associaterd with this eruption.99ivo://helio-informatics.org/FE304_halocme_20110113_165714SuggSu: A clear beautiful filament erupts with most of its stuff falling back on the surface in 304 A image::http://aia.cfa.harvard.edu/filament/index.html?search=013501362010-12-23T00:00:092010-12-23T04:55:21621-9283.0PCPAS?Y?NNN-0243JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2010/12/CME0059/CME.html[169,1073,-674,-1183][2124,4043,0,1079]Filament EruptionAnna Malanushenko))Eruption of filament seen on the SE limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110110_215344SuMMSu: A sideway(possible) prominence eruption with a possible kink in the final::http://aia.cfa.harvard.edu/filament/index.html?search=013601372010-12-23T08:09:452010-12-23T10:26:33-499-8772.0PCC?ARYNNNN-N-[-629,-368,-962,-793][578,1857,226,945]Small eruptionAnna MalanushenkommSmall eruption of a clearly helical structure on the SE limb. At least a turn and a half seems to be visible.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110110_220115SuvvSu: A weak filament motion with most mass falling back on the surface in 304 A image may not belong to a real eruption::http://aia.cfa.harvard.edu/filament/index.html?search=013701382010-12-24T00:28:572010-12-24T06:50:331010-2972.5QSFARNNYNN-0142JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2010/12/CME0060/CME.html[1337,683,-623,29][2816,4095,1194,1913]Filament eruptionAnna Malanushenko33A clear eruption of a large filament on the W limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110110_215655Su]]Su: This prominence eruption with most material leaving in 304 A image is probably with a CME::http://aia.cfa.harvard.edu/filament/index.html?search=013801392010-12-24T20:05:582010-12-25T16:23:58705-5394.0QSP?SRYYYNN-0139FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/12/CME0056/CME.html[200,1210,-281,-797][2176,4095,610,1689]Triple filament eruptionAnna MalanushenkoqqThree nearb filaments take off one after another, the first on the SW disk and the other two cliser to t he limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110110_231748SuMcKillop: Possible rolling motion in the first eruption. Su: Three filament eruption occurred in a row, the middle quiescent one displays a clear kink in 304 A and 171 A images, and the last small AR filament appears to show a kink structure too::http://aia.cfa.harvard.edu/filament/index.html?search=013901402010-12-24T22:28:462010-12-25T15:33:34-9572494.0QSFS?RYNYNN-0271FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2010/12/CME0058/CME.html[-1207,-706,457,40][0,1279,2103,2822]Filament eruptionAnna Malanushenko Filament eruption on the W limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110110_230238Su[[Su: A huge prominence lifts off slowly and mass is seen leaving the disk, beautiful tornado::http://aia.cfa.harvard.edu/filament/index.html?search=014001412010-12-30T00:00:032010-12-30T09:00:036076811.5QSF?ARYNYNN-0136JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2010/12/CME0074/CME.html[354,860,836,527][2420,3699,2824,3543]''Filament eruption - limb and disk views Nariaki NittaSlow prominence eruption on the limb, which seems to be on a larger scale -- for example, the area in the box seems to be part of the eruption so does the eastern part of the active region (a small eruption around 2:30 UT).99ivo://helio-informatics.org/FE304_halocme_20110114_195858Su[[Su: A rolling filament erupts with most material falling back on the surface in 304 A image::http://aia.cfa.harvard.edu/filament/index.html?search=014101422011-01-01T18:01:442011-01-02T23:54:14598-7083.0PCFARYNYNN-0264JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/01/CME0004/CME.html[-326,1523,-1228,-188][1014,4095,3,1734]Triple filament eruptioinsWei LiuThree filament eruptions near the southwest limb. The first two eruptions went off almost in concert, although they were more than 1/2 solar radius away.88ivo://helio-informatics.org/FE304_WeiLiu_20110118_235128SuMcCauley: Entries refer to southernmost eruption. Su: Two filament eruptions on the polar-crown, tornado, sympathetic eruptions::http://aia.cfa.harvard.edu/filament/index.html?search=014201432011-01-01T22:54:142011-01-02T19:24:14994-3293.0QSF??RNNYNN-0136JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/01/CME0003/CME.html[616,1372,-541,-116][2816,4095,1141,1860]filament eruptionWei LiuaaDetailed view of one of the triple filament eruptions. Note the funnel shaped erupting structure.88ivo://helio-informatics.org/FE304_WeiLiu_20110119_000347SujjSu: A prominence eruption on the western limb with most stuff falling back, tornado, U shape, sympathetic?::http://aia.cfa.harvard.edu/filament/index.html?search=014301442011-01-02T00:00:432011-01-02T08:30:43522-7362.5QSPAS??NYNN-0210GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/01/Flow0001/CME.html[217,826,-524,-948][2278,3557,462,1181]Filament eruptionWei Liu,,A filament eruption near the southwest limb.88ivo://helio-informatics.org/FE304_WeiLiu_20110106_191656Su11Su: A QS filament eruption, tornado, sympathetic?::http://aia.cfa.harvard.edu/filament/index.html?search=014401452011-01-08T00:00:032011-01-08T02:27:39-70-6231.0QSP?RNNNNN-N-[-744,604,-444,-802][809,3054,379,1640]Filament eruption Thomas BergerLarge trailing segment of major E-W filament lifts off slowly. This section of the filament is not very prominent in 304 but the lift-off is clearly visible nonetheless.;;ivo://helio-informatics.org/FE304_TomBerger_20110110_223651SuMcCauley: See HEK movie for improved visibility in 304. Su: It's a weak motion, and we can get a little message about it in 304 A image::http://aia.cfa.harvard.edu/filament/index.html?search=014501462011-01-10T00:00:092011-01-10T02:53:33-7426071.5QSCA?R?NNYNN-N-[-1202,-282,349,866][0,1919,2521,3600]small filament eruptionWei Liu11A small filament erupted near the northeast limb.88ivo://helio-informatics.org/FE304_WeiLiu_20110110_185408SuMMSu: One leg of the filament lifts off from the surface and falling to another::http://aia.cfa.harvard.edu/filament/index.html?search=014601472011-01-10T00:30:452011-01-10T06:27:45-836-6471.0QSC?A?R???YN-N-[-1084,-587,-412,-882][16,1295,610,1329]minor filament eruptioniWei LiuiiA filament eruption. Note the gradually rising horizontal "pieces" of material seen in the 171 A channel.88ivo://helio-informatics.org/FE171_WeiLiu_20110110_183129SuQQSu: A weak motion doesn't change the shape and structure of upper field obviously::http://aia.cfa.harvard.edu/filament/index.html?search=014701482011-01-14T00:00:122011-01-14T12:00:12-1048571.0PCP?S?RNNY?NN-N-[-368,160,649,1065][1235,2514,3117,3836]Filament eruptionWei Liu&&Filament eruption near the north pole.88ivo://helio-informatics.org/FE304_WeiLiu_20110118_225504McCauleyUUMcCauley: See HEK movie for 304 channel. Su: Little message can we get from the image::http://aia.cfa.harvard.edu/filament/index.html?search=014801492011-01-16T16:06:092011-01-17T00:00:09-5185811.5QSC??NNNNB1.6kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/01/16/gev_20110116_1841/index.htmlN-[-821,-215,757,405][545,1824,2657,3376]Filament EruptionAnna MalanushenkobbFilament eruption on the NE limb. Note the footpoint brightening in 171A when the eruption starts.BBivo://helio-informatics.org/FE171_AnnaMalanushenko_20110117_221858SuaaMcCauley: See HEK movie for 304 channel. Su: The filament breaks up and falls back on the surface::http://aia.cfa.harvard.edu/filament/index.html?search=014901502011-01-18T13:54:102011-01-18T18:12:109695114.0QSPSRYY?N?N-N-[794,1144,685,337][2816,4095,2540,3259]Filament eruptionAnna MalanushenkoA filament eruption.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110119_025519SuMcCauley: No significant CME, but some associated material can be seen in this movie: http://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/01/Flow0036/CME.html Su: A rolling and twisting prominence eruption::http://aia.cfa.harvard.edu/filament/index.html?search=015001512011-01-24T22:30:092011-01-25T07:00:09703-6263.5QSFARYNYYN-N-[346,1060,-362,-889][2580,3859,646,1365]Triple filament eruptionsWei LiuuuThree filaments erupted across the disk almost simultaneously. The one on the southwest limb is the most impressive, while the other two (one on southeast and the other on the west limb near the equator) are probably failed eruptions as most of the material was seen to fall back to the Sun. It is not clear about the causal relationship between these concurrent eruptions.88ivo://helio-informatics.org/FE304_WeiLiu_20110125_233413Su))McCauley: There was a CME large enough to register in the CACTus catalog, but some associated material can be seen in this event: http://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/01/Flow0053/CME.html Su: It's a SW prominence eruption, and mass is seen leaving the disk in 304 A disk, U shape::http://aia.cfa.harvard.edu/filament/index.html?search=015101522011-01-26T07:23:512011-01-26T12:45:09-832052.0QSC?A?RNNNNN-N-[-278,111,403,7][1269,2548,2030,2749]Minor filament eruptionWei LiuhhA small filament erupted near the disk center. Note simultaneous flaring on the disk below the filament.88ivo://helio-informatics.org/FE304_WeiLiu_20110127_015905SuUUSu: A weak signal displays an asymmetric filament eruption in 304 A movie in the disk::http://aia.cfa.harvard.edu/filament/index.html?search=015201532011-01-28T00:00:092011-01-28T03:59:3311233084.0ARFSRNNNNM1.4kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/01/28/gev_20110128_0044/index.html0459JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/01/CME0072/CME.html[705,1542,522,94][2176,4095,2022,3101]>>First large eruption in the sequence followed an M-class flareAnna MalanushenkoA spectacular eruption on the NW limb immediately following the M-class flare associated with AR 11149. This was the first large eruption in a sequence of several.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110201_000453SuSu: A powerful flare with clear flare arcs and a CME(11149), rotating, rolling motion? Sideways ejections before and after the eruption::http://aia.cfa.harvard.edu/filament/index.html?search=015301542011-01-28T00:00:092011-01-28T08:49:21-889-6084.0QSP?S?RYY?YY? B5.2|B3.4http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/01/28/gev_20110128_0331/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/01/28/gev_20110128_0402/index.html0311JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/01/CME0073/CME.html[-1320,-459,-303,-913][0,1919,495,1574]Filament eruptionAnna Malanushenko66A spectacular eruption of a large filament on SE limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110131_235606SuooSu: This prominence with rolling and twisting structure rises and then falls back on the surface in 304 A image::http://aia.cfa.harvard.edu/filament/index.html?search=015401552011-01-28T03:30:452011-01-28T06:55:57765-7391.5QSP?SRNNNYN-0221GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/01/Flow0069/CME.html[415,1114,-495,-983][2683,3962,457,1176]Flux rope eruptionAnna Malanushenko((Fainf flux rope eruption on the SW limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110201_012702Su@@Su: It's a SW prominence eruption and it happens behind the limb::http://aia.cfa.harvard.edu/filament/index.html?search=015501562011-01-28T03:38:332011-01-28T06:09:451040773.5ARFASNNNNN-0459FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/01/CME0054/CME.html[724,1355,328,-174][2816,4095,1817,2536]HHLarge eruption in the sequence of several that followed an M-class flareAnna MalanushenkobbA large eruption, second of the sequence, that followed an M-class flare associated with AR 11149.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110201_000706SuMcCauley: The CME entry is complicated by an event that occurs a few hours earlier. Su: The eruption with a CME(11149) jets lots of mass and some falling back on the surface::http://aia.cfa.harvard.edu/filament/index.html?search=015601572011-01-28T11:42:092011-01-28T19:26:33-416-5892.0QSC?SNRNNNNN-N-[-652,-179,-381,-796][716,1995,708,1427]AAFolament eruption on the limb with coronal darkening disappearingAnna MalanushenkoKKA filament and a dark blobon its side on the SE limbtake off and disappear.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110201_011951SuWWSu: An arc rises slowly and then erupts with some of material falls back on the SW disk::http://aia.cfa.harvard.edu/filament/index.html?search=015701582011-01-29T07:19:392011-01-29T10:03:2710053172.0QSF?ANR?YNNNN-0238FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/01/CME0059/CME.html[714,1295,614,19][2176,4095,2036,3115]--Flux rope eruption, next in the long sequenceAnna MalanushenkoAn eruption of long, faint and clearly twisted flux rope, another one in the long sequence initiated by an M-class flare in AR11149 a day ago.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110201_005702Su@@Su: Weak signal in 171 A and 193 A images and clear arc in 304 A::http://aia.cfa.harvard.edu/filament/index.html?search=015801592011-01-30T08:18:102011-01-31T00:00:106554413.0QSFSRNNYNB1.3kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/01/30/gev_20110130_1201/index.html0416FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/01/CME0066/CME.html[224,1086,801,82][2176,4095,2244,3323]Large filament eruptionAnna Malanushenko++Eruption of a large filament on the SW diskBBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110202_011619SuwwSu: A large-scale arc lifts off and erupts on the eastern disk, oscillations and horizontal motions before the eruption::http://aia.cfa.harvard.edu/filament/index.html?search=015901602011-02-02T00:00:042011-02-03T17:08:28-256-1453.0ARF?SRNNNNB4.1|B1.1|B4.1|B2.0|B2.6http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/02/02/gev_20110202_0027/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/02/02/gev_20110202_0244/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/02/02/gev_20110202_0614/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/02/02/gev_20110202_1020/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/02/03/gev_20110203_0551/index.htmlN-[-592,80,-293,4][982,2261,1448,2167]00Flux Emergence with Wave and Triggered Eruptions Ralph SeguinNice emerging flux region trailing an active region. A small eruption in/around the emerging flux triggers a sigmoid shaped filament to erupt in the active region just to its west.==ivo://helio-informatics.org/FE193_RalphSeguin_20110204_002748SuSu: Clear field lines are seen in 171 A image and some field lines are opened and bright arcs are formed, Very cleaer null-point reconnection leads to the eruption in the small emerging AR as shown in 171, several eruptions::http://aia.cfa.harvard.edu/filament/index.html?search=016001612011-02-02T00:00:122011-02-02T17:00:124077963.5PCFSRYNNNN-1224FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/02/CME0005/CME.html[159,655,1067,525][1767,3686,2835,3914]!!Small Filament Eruption with Rain Ralph SeguinqqSmall filament eruption near the northwest limb, visible in 304, 211 and 171. Not very strong, with coronal rain.==ivo://helio-informatics.org/FE171_RalphSeguin_20110202_215021SuSu: An arcade-like prominence eruption with lots of rolling motion and twist, another filament eruption before it behind the limb::http://aia.cfa.harvard.edu/filament/index.html?search=01610162-----1--------------- Ralph SeguinA small eruption (reported earlier) from an emerging flux region triggers a coronal wave and and two other filament eruptions: a sigmoid filament in the active region just to the west of the emerging flux erupts (already reported) The coronal wave appears to trigger an eruption in the large filament complex much farther north. The eruption of the large filament complex has some coronal rain./brightening associated to its west.==ivo://helio-informatics.org/FE171_RalphSeguin_20110204_003609---01632011-02-03T10:33:102011-02-03T23:39:10-5704402.5QSFARYNYNN-Y?-[-1101,-38,861,18][139,2058,2241,3320]Filament EruptionAlberto SainzdaldaLarge filament eruption.CCivo://helio-informatics.org/FE304_AlbertoSainzDalda_20110205_030439SuMcCauley: LASCO data gap precluded a CME entry. Su: A clear asymmetric filament eruption in 304 A image displaying lots of twisting/rolling motion, the same as last one::http://aia.cfa.harvard.edu/filament/index.html?search=016301642011-02-10T11:00:102011-02-10T14:34:22-903-6503.5QSPARYNYNN-0139GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/02/Flow0006/CME.html[-994,-812,-566,-734][0,1279,605,1324]Prominence eruptionAnna Malanushenko!!A prominence eruption on SE limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110211_194043SuVVSu: A prominence is seen rising and falling back on the surface finally in 304 A image::http://aia.cfa.harvard.edu/filament/index.html?search=016401652011-02-10T14:14:342011-02-11T03:57:46-640-4843.5QSPARYNYNN-0139GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/02/Flow0005/CME.html[-212,-1068,-649,-318][22,1941,703,1782]Filament eruptionAnna Malanushenko88Filament eruption seen both on the disk and on the limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110214_185741SuFFSu: A large filament erupts in SE disk with most material falling back::http://aia.cfa.harvard.edu/filament/index.html?search=01650166-----1---------------Anna Malanushenko[[Filament eruption on the SE limb, immediately after a prominence eruption in the same area.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110211_194717---01672011-02-10T20:24:102011-02-11T00:36:10-8414732.0ARCSRYYNNN-N-[-921,-762,539,407][6,1285,2477,3196]&&Filament activity and possibly a flareAnna MalanushenkovvFilament activity and possibly a flare on the limb. There was a flare associated with this region a few hours earlier.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110214_191136SuooSu: A bright channels is seen and clear field structures appear in 171 A image, a failed kink filament eruption::http://aia.cfa.harvard.edu/filament/index.html?search=016701682011-02-11T03:40:582011-02-11T17:32:341569053.5PCPSRY?Y?YNN-N-[-107,419,672,1138][1669,2948,3197,3916]**Eruption of a compact filament on the diskAnna MalanushenkoA seemingly compact filament on the disk erupts and expands a lot. During the eruption the top part of it could be seen on the limb as a cusp-like structure.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110214_184716SuWWSu: A slowly filament eruption in (near) polar-crown with a kink structure (?), tornado::http://aia.cfa.harvard.edu/filament/index.html?search=016801692011-02-11T06:03:462011-02-11T11:31:2210103393.0ARFSRYNNNB9.0kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/02/11/gev_20110211_0758/index.html0405FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/02/CME0016/CME.html[864,1155,467,211][2816,4095,2254,2973]Filament eruptionAnna MalanushenkoRapid eruption of thin filament on the limb. The filament develops a strong bend and raises up to a few times the projected distance between the footpoints before its apparent disconnection.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110214_183647SuLLSu: A beautiful arc with rolling and twisting structure appears in AR(11154)::http://aia.cfa.harvard.edu/filament/index.html?search=016901702011-02-11T08:35:342011-02-11T14:32:34-1073112.5ARPASY?NNN1?-0209FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/02/CME0017/CME.html[-1247,-899,228,-207][0,1919,1526,2605]Prominence eruptionAnna MalanushenkoLarge eruption that seems to go in wo stages. The first stage looks like an extremely rapid expansion of a coronal cavity seen in 211A with no apparent 304A "filling" and three hours later a large filament erupts, which is observed in 304A.BBivo://helio-informatics.org/FE211_AnnaMalanushenko_20110211_202403SuggSu: This quick sideway eruption changes the structure of field clearly in 171A image, jet-like eruption::http://aia.cfa.harvard.edu/filament/index.html?search=017001712011-02-12T17:37:222011-02-12T21:57:46-3925312.0IP?P?SRNNYN B4.7|B5.8http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/02/12/gev_20110212_1821/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/02/12/gev_20110212_1913/index.htmlN-[-695,-90,699,363][754,2033,2574,3293]##Faint filament eruption on the diskAnna Malanushenko^^Faint filament eruption on the disk that followed brightening of coronal loops of a nearby AR.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110214_193940SuZZSu: Rising filament is seen in 304 A image, but we can't confirm more information about it::http://aia.cfa.harvard.edu/filament/index.html?search=017101722011-02-14T00:00:042011-02-14T05:00:40-602-1421.5QSCSRYNNN2?-N-[-638,-566,-101,-183][405,1684,1452,2171]Small flux rope eruptionAnna MalanushenkoddEruption of small filament in a small nameless active region (that later probably becomes AR 11161).BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110216_203302Su<>ivo://helio-informatics.org/FE304_ThomasBerger_20110307_182844SullSu: Filament is seen lifting and material is seen leaving from the surface, no clear evidence in 171 and 193::http://aia.cfa.harvard.edu/filament/index.html?search=018401852011-03-03T00:00:042011-03-04T00:00:04-11562534.0IP?FASYNYY3?-0359JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/03/CME0004/CME.html[-837,-1475,-178,683][0,2551,1752,3185]Prominence eruption Thomas BergerwwLarge prominence lift-off on the equatorial East limb behind AR 11166. Coronal rain in loop footpoint far to the North.>>ivo://helio-informatics.org/FE304_ThomasBerger_20110308_022634SuSu: The prominence moves sideway on the western limb and the lifts and erupts and most mass falls back on the surface in 304 A image, vertical threads U shape::http://aia.cfa.harvard.edu/filament/index.html?search=018501862011-03-04T02:42:102011-03-04T07:36:10-996-2473.0IP?FSRYNNNN-0506JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/03/CME0006/CME.html[-741,-1250,-561,67][0,1919,1097,2176]Prominence eruption Thomas Berger``Quiescent prominence eruption on SE limb. Southern footpoint blows off; northern stays attached.>>ivo://helio-informatics.org/FE304_ThomasBerger_20110308_023547SuYYSu: A standard symmetric arcade eruption and twisting structure is obvious in 171 A image::http://aia.cfa.harvard.edu/filament/index.html?search=018601872011-03-05T14:05:042011-03-06T00:00:04-9644544.0IPFSRYYYN2?-Y?-[-1219,-708,310,597][0,1279,2444,3163]Small filament eruptionAnna Malanushenko..Fiament etupiton and the post-eruption arcade.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110308_193613SuMcCauley: LASCO data gap precluded a CME entry,. LASCO data gap precluded CME entry. Su: It happens in a decaying AR and a quick eruption leaves a beautiful kink::http://aia.cfa.harvard.edu/filament/index.html?search=018701882011-03-06T13:50:102011-03-06T17:50:10-3593981.0AROAS?NNNNC3.9kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/03/06/gev_20110306_1521/index.htmlN-[-462,-256,296,500][810,2089,2352,3071]Faint filament eruptionAnna Malanushenko00Spray surge or possibly small filament eruption.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110309_212654SuMcCauley: Not sure if this is actually a filament eruption, so putting "Other" for the eruption column. Su: A couple of jets at the border of the AR (11166)::http://aia.cfa.harvard.edu/filament/index.html?search=018801892011-03-07T19:00:012011-03-07T20:53:218127014.5ARFARYNNNM3.7kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/03/07/gev_20110307_1943/index.html0702JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/03/CME0017/CME.html[463,1161,1001,400][2762,4041,2856,3575]Lightbulb filament eruptionAnna Malanushenko  Sun clearly came up with a brilliant idea. This spectacular eruption of a massive filament seem to happen before the M-class flare (which took place at 19:43-20:01UT and peaked at 20:12 according to GOES).The flare kernels seem very small and could barely be seen at the footpoints of the filament, but the change in exposure suggests they were very bright. The boundary of the cavity is seen as a bright circle, nearly complete, and later turns into a ligthbulb-shaped structure with the twisted filament in the middle, completing the analogy.BBivo://helio-informatics.org/FE211_AnnaMalanushenko_20110307_223300SussSu: Clear arcs are seen at the footpoints of the flare in 304 A image and a strong eruption results in a CME(11164)::http://aia.cfa.harvard.edu/filament/index.html?search=018901902011-03-08T16:38:102011-03-09T00:00:101059-4265.0ARP?SRYYNNM4.4|M1.5|C8.8CChttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/03/08/gev_20110308_1808/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/03/08/gev_20110308_1935/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/03/08/gev_20110308_2332/index.html0584JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/03/CME0023/CME.html[912,1206,-282,-570][2816,4095,979,1698]Post-flare eruptionAnna MalanushenkobbAn M-class flare apparently triggered a filament eruption. The erupting flux tube is seen kinking.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110312_011853SuMcCauley: Listed as a partial eruption (?) because it's not clear that filament material was expelled with the magnetic structure. Su: A clear kink is seen in 171 A and 193 A images and a quick eruption leaves two bright arcs which are rising slowly::http://aia.cfa.harvard.edu/filament/index.html?search=019001912011-03-09T20:29:502011-03-09T23:59:501802615.0ARPASNNNN C9.4|X1.5http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/03/09/gev_20110309_2203/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/03/09/gev_20110309_2313/index.htmlN-[84,276,326,197][1709,2988,2124,2843]((Close-up of the site of an X-class flareAnna MalanushenkoJJA close-up of the site of an X-class flare. It followed a fews pray surges on the E and W of the region, a filament activation in the N part of the region amd a ,assive filament eruption in the E part of the region. The event happened to take place on birthray of someone who wrote a dissertation on flares. Hapy Birthday, SabrinaBBivo://helio-informatics.org/FE171_AnnaMalanushenko_20110312_024726SuSu: It brightens in AR(11166) in all three images and jets mass out sideway, and a CME is followed. Failed eruption of a twisted structure at the core of the AR, jet-like eruption at the border.::http://aia.cfa.harvard.edu/filament/index.html?search=01910192-----1---------------Anna MalanushenkoA filament eruption immediately following a C-class flare and preceding an X-class flare. The filament seems to travel eastwards and then northwestwards and probably towards the observed. On the end of the movie an interesting ripples could be seen on the NE limb in 304A.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110312_023344---01932011-03-17T08:45:112011-03-17T16:00:113079552.0PCP?SRYNNNN-N-[-112,726,1312,598][1600,3519,3016,4095]Polar filament eruption Thomas BergerSlow rise and untwist of North polar filament. Appears to be on the back side of the Sun prior to eruption - no filament visible on the front side disk.>>ivo://helio-informatics.org/FE304_ThomasBerger_20110406_172630SuKKSu: A clear rolling motion of the arcade prominence with horizontal threads::http://aia.cfa.harvard.edu/filament/index.html?search=01930194-----1--------------- Thomas Berger22Large kink-loop eruption from AR 11171 on SW limb.>>ivo://helio-informatics.org/FE304_ThomasBerger_20110406_182612---01952011-03-19T11:24:112011-03-19T14:51:111019-4905.0QSFSRYNYNN-0976JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/03/CME0060/CME.html[738,1299,-78,-903][1650,4095,544,1917]AR 11171 Filament Eruption Thomas BergerJJLarge twisting/kinking loop eruption from filament in AR 11171 on SW limb.>>ivo://helio-informatics.org/FE304_ThomasBerger_20110406_195322Su\\Su: Clear twisting structure is seen in 304 A and 171 A images and it's located on AR(11171)::http://aia.cfa.harvard.edu/filament/index.html?search=019501962011-03-27T12:45:122011-03-28T02:07:429410563.0PCPSRY?Y?YNN-0141JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/03/CME0096/CME.html[-74,262,928,1183][1565,2844,3376,4095]Polar crown filament eruptionWei LiuA filament eruption near the north pole. Note the various trajectories of the ejected material: some falls back and some joins the nearby filament on the west limb.88ivo://helio-informatics.org/FE304_WeiLiu_20110408_212349SuGGSu: Weak twisting structure is seen in 171 A image and it moves sideway::http://aia.cfa.harvard.edu/filament/index.html?search=019601972011-03-29T18:40:112011-03-30T00:00:11-1910673.0PCFARYNYNN-0879JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/03/CME0104/CME.html[-186,147,930,1204][1376,2655,3376,4095]Polar crown filament eruptionWei LiuBBA filament eruption near the north pole. Some material falls back.88ivo://helio-informatics.org/FE304_WeiLiu_20110412_001257SuMcCauley: The coronagraph signature is mixed with a larger, backside eruption. Su: A polar-crown asymmetric prominence eruption::http://aia.cfa.harvard.edu/filament/index.html?search=019701982011-03-31T21:00:292011-03-31T23:59:17333-1714.0ARFSRNNNN B7.0|C1.6http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/03/31/gev_20110331_2135/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/03/31/gev_20110331_2207/index.html0229JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/03/CME0117/CME.html[2,665,-502,161][1964,3243,1404,2123]00Mild eruption, but associated with a sizable CME Nariaki Nitta33This eruption seems to explain the CME observed by LASCO C2 at PA~180, first seen at 23:06. It reached C3, but did not survive a long distance. The eruption itself is not spectacular, and people could have thought the CME was a back-side event, but now STEREO data do show that it was from the front side.99ivo://helio-informatics.org/FE304_halocme_20110408_191734SussSu: Clear change of the field structure is seen in 171 A image, the eruption results a jet nearby, complex topology::http://aia.cfa.harvard.edu/filament/index.html?search=019801992011-04-02T09:00:112011-04-02T21:10:11401-2984.0IPPSRYYYNN-N?-[140,661,-124,-473][2076,3355,1191,1910]Filament eruption in AR 11178 Thomas Berger@@Filament eruption and two-ribbon flare in AR 11178/11176 region.99ivo://helio-informatics.org/FE304_TBerger_20110425_183146SuMcCauley: LASCO data gap may have precluded a CME entry. Su: Although it happens in disk in AR(11181), It displays a clear kink in 171 A and 304 A images::http://aia.cfa.harvard.edu/filament/index.html?search=019902002011-04-02T19:50:112011-04-04T00:00:11852-3692.0ARP?ASY?NNNB7.4kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/04/02/gev_20110402_2234/index.htmlY?-[548,1157,-151,-587][2816,4095,1074,1793]$$Filament eruption Flare in AR 11176 Thomas BergernnFilament eruption and C3 flare in AR 11176 on SW limb. Nice arcade of post-flare loops visible in 171 and 211.99ivo://helio-informatics.org/FE211_TBerger_20110425_184341SuMcCauley: LASCO data gap precluded a CME entry. Su: Many bright arcs are seen in 171 A and 193 A images and mass is seen moving sideway in 304 A image::http://aia.cfa.harvard.edu/filament/index.html?search=020002012011-04-08T21:00:302011-04-09T01:59:54-3754742.0IP?FSRNNNNB8.0kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/04/09/gev_20110409_0040/index.html0139FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/04/CME0019/CME.html[-922,172,-73,1021][464,2383,2299,3378] Low-energy (?) filament eruption Nariaki Nitta22Seem only in 304 A. Flaring not obvious. No CME?99ivo://helio-informatics.org/FE304_halocme_20110416_210631Su//Su: Rising arcs are only obvious in 304 A image::http://aia.cfa.harvard.edu/filament/index.html?search=020102022011-04-09T05:00:002011-04-09T22:20:00664-7404.0QSCA?RNNYNN-N-[358,970,-514,-966][2515,3794,455,1174]99Small filament eruption converged into coronal structures Nariaki NittabbSlow process, perhaps related to the larger eruption in the northeastern active region (AR 11188).99ivo://helio-informatics.org/FE304_halocme_20110416_221328Su||Su: It's a quiet and slowly process and it looks like a collapse rather than a eruption, failed eruption of vertical threads::http://aia.cfa.harvard.edu/filament/index.html?search=020202032011-04-24T00:00:012011-04-24T02:04:01-3314802.0QSF?SRNNNNN-N-[-430,-231,643,316][858,2137,2488,3207]Faint filament eruptionAnna MalanushenkoA faint filament eruptionBBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110426_004032SuMcCauley: Appears to be a full eruption, but it's position/direction probably precluded it from generating a CME in LASCO. Su: It's not clear what happens in 171 A and 193 A images, while a rising arc is seen in 304 A image::http://aia.cfa.harvard.edu/filament/index.html?search=020302042011-04-24T07:34:012011-04-24T09:26:01-9284314.0IP?FASN?YNN-0424FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/04/CME0104/CME.html[-1051,-805,486,376][0,1279,2407,3126] Small twisted flux rope eruptionAnna Malanushenko<>Su: Clear change of the field structure is seen in 171 A image::http://aia.cfa.harvard.edu/filament/index.html?search=020602072011-04-27T00:41:552011-04-27T03:20:55-8355455.0ARFARYYYNN-0694FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/04/CME0116/CME.html[-476,-1193,198,891][18,1297,2596,3315]AR filament eruptionKarel SchrijverZZAR filament eruption with "coronal bright front" moving out towards the NE beyond the fov.@@ivo://helio-informatics.org/FE211_KarelSchrijver_20110428_202921SuSu: Mass is seen jetted out and a CME is followed, and this quick eruption with a clear kink results in bright arcs in the footpoints::http://aia.cfa.harvard.edu/filament/index.html?search=020702082011-04-27T15:11:552011-04-27T19:29:55495382.0QSP?ASNNNNN-N-[317,-218,266,809][1171,3090,2404,3483]QS filament eruptionKarel SchrijverA quiet-Sun filament eruption with post-eruption arcade, starting in N hemisphere at central meridian. The eruption shows dimmings on both sides of the event, one filling in quite rapidly, the other (leading) one being more persistent.@@ivo://helio-informatics.org/FE211_KarelSchrijver_20110428_202611SuRRSu: The lower layer of the filament ejected sideways, while the higher layer stays::http://aia.cfa.harvard.edu/filament/index.html?search=020802092011-05-03T07:55:012011-05-03T18:00:019574815.0QSP?SRYY?YNN-0568FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/05/CME0007/CME.html[620,1294,794,167][2816,4095,2489,3208]Large filament eruptionAnna Malanushenko,,Eruption of a large filament on the NW limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110509_224557SurrSu: Clear twisting structure is seen in 304 A movie, and a kink should be seen theoretically, but we don't find it::http://aia.cfa.harvard.edu/filament/index.html?search=020902102011-05-04T15:09:552011-05-04T19:29:55-5756044.0IPFSRYYYNB6.8kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/05/04/gev_20110504_1655/index.html0311FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/05/CME0009/CME.html[-987,-164,1053,155][0,2658,2308,3801]Large filament eruptionAnna MalanushenkoA large filament eruptionBBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110509_230022SuHHSu: Clear kink and twisting structure can be found easily in 304 A movie::http://aia.cfa.harvard.edu/filament/index.html?search=021002112011-05-04T18:52:122011-05-05T08:24:12-989-3654.0QSCARYNYNN-N-[-1190,-788,-674,-56][0,1919,900,1979] Large and slow filament eruptionAnna Malanushenko//Large and slow filament eruption on the E limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110509_233411Su]]Su: The prominence lifts off the surface, moves sideway and finally falls back on the surface::http://aia.cfa.harvard.edu/filament/index.html?search=021102122011-05-06T01:35:012011-05-06T03:25:01-1069-1112.0QSFA?RNNNNN-0353FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/05/CME0010/CME.html[-1239,-900,58,-279][0,1279,1504,2223]Faint filament eruptionAnna MalanushenkoJJA faint flux rope eruption with no apparent counterparts in 211A and 171A.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110509_193307SuSu: It's not apparent in 171 A and 193 A movies while rising prominence can be found in 304 A movie, and it happens behind the disk::http://aia.cfa.harvard.edu/filament/index.html?search=02120213-----1---------------Karel SchrijveraaFilament eruption, with leading coronal propagating front, and post-eruption cooling loop arcade.@@ivo://helio-informatics.org/FEMET_KarelSchrijver_20110519_174324---02142011-05-11T01:43:552011-05-11T03:55:557853994.0IPFSRY?NNNB8.1kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/05/11/gev_20110511_0223/index.html0413FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/05/CME0040/CME.html[1197,374,926,-128][975,4095,1837,3590]&&Eruption and coronal propagating frontKarel SchrijverFilament eruption (and two-ribbon flare), transitioning into a clear "bubble-like" coronal propagating front (EIT wave) as the eruption transitions to a CME.@@ivo://helio-informatics.org/FE211_KarelSchrijver_20110519_173145SussSu: A quick eruption with twisting and a CME followed results in many bright arcs in the footpoints of the filament::http://aia.cfa.harvard.edu/filament/index.html?search=021402152011-05-12T11:14:552011-05-12T14:39:55-8053235.0IPFSRY?YNC1.8kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/05/12/gev_20110512_1211/index.html0265FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/05/CME0044/CME.html[-1339,-272,23,623][0,1919,2047,3126]Triggered Filament Eruption Thomas BergeruuFrustrated eruption of central filament in small plage region leads directly to full eruption of peripheral filament.>>ivo://helio-informatics.org/FE304_ThomasBerger_20110519_180009Su  McCauley: Catalog entries refer to the second, successful eruption. Su: Here are two filament eruptions, and the AR brighter one displays a bright kink then failed and the larger darker one appears to be disturbed then erupts, and both of them are rolling and twisting::http://aia.cfa.harvard.edu/filament/index.html?search=021502162011-05-13T05:00:012011-05-13T21:10:01605-5855.0QSP?SYYYNN-0383FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/05/CME0047/CME.html[162,1048,-301,-869][2097,4016,534,1613]Quiescent Filament Eruption Thomas BergerModerate-to-large filament eruption on SW limb. AIA data seems to be interrupted just after lift-off. Very obvious untwisting (or twisting?) of filament during lift-off.>>ivo://helio-informatics.org/FE304_ThomasBerger_20110519_183554SuaaSu: Kink can be seen in all three movies and in 304 A movie we can find the filament move sideway::http://aia.cfa.harvard.edu/filament/index.html?search=021602172011-05-15T14:00:022011-05-16T00:00:02-60-4013.0ARP?ASYNNNN-N-[-288,168,-221,-581][1309,2588,1020,1739]Repetitive filament eruptionsWei LiuLLFilament eruptions repeated several times within hours from the same region.88ivo://helio-informatics.org/FE304_WeiLiu_20110520_040838Su\\Su: several sideway eruptions of filaments in two small ARs with twisting and rolling motion::http://aia.cfa.harvard.edu/filament/index.html?search=021702182011-05-17T02:19:562011-05-17T04:39:562913973.0IPPSRYY?YNN-0149FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/05/CME0057/CME.html[-64,647,153,640][1894,3173,2349,3068]Loop filament eruptionWei LiuBBA loop shaped active region filament erupted near the disk center.88ivo://helio-informatics.org/FE304_WeiLiu_20110521_020635SuMcCauley: Northern part of the filament (if they are the same structure) remains stable. Su: Kink is seen rising in 304 A movie?::http://aia.cfa.harvard.edu/filament/index.html?search=021802192011-05-18T00:00:022011-05-18T08:40:029535545.0QSPS?RYY?YNN-0134KKhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/05/Flow0050/CME.html[1193,713,271,836][2176,4095,2431,3510]--Filament eruption with coronal cavity liftoffAnna MalanushenkoPPThin large filament takes off the limb along with the associated coronal cavity.BBivo://helio-informatics.org/FEMET_AnnaMalanushenko_20110519_204935SuhhSu: It rises and much material falls back in the final, and it may have a kink_ U shape vertical threads::http://aia.cfa.harvard.edu/filament/index.html?search=021902202011-05-18T00:00:022011-05-18T23:07:32-5159605.0PCFA?RY?NYYN-0601JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/05/CME0073/CME.html[-947,-84,1182,738][229,2148,3016,4095]Filament eruptionAnna MalanushenkoOne end of a flament slowly rises followed by the loftoff of the entire structure. No associated cavities easily seen in 211A or 171A.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110520_004505SujjSu: Mass is seen leaving from the surface in 304 A movie, and it's a (near) polar-crown eruption U shape::http://aia.cfa.harvard.edu/filament/index.html?search=022002212011-05-21T00:00:022011-05-21T08:00:02-905-5105.0QSPS?R?NYNN-0355FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/05/CME0072/CME.html[-1169,-640,-300,-720][0,1279,839,1558]filament eruptionWei LiuNNFIlament eruption on southeast limb; some material falls back as coronal rain.88ivo://helio-informatics.org/FE304_WeiLiu_20110523_211130SuWWSu: It's a prominence eruption in SW limb, very complex structure of a partial eruption::http://aia.cfa.harvard.edu/filament/index.html?search=022102222011-05-21T06:45:022011-05-21T21:45:02-8061152.0QSCASNNYNN-N-[-947,-666,363,-133][0,1919,1700,2779],,Minor filament eruption and two-ribbon flareWei LiuA filament eruption near the east limb, associated with a minor two-ribbon flare seen at 211 (no clear indication of flare loops, but the separating ribbons are evident).88ivo://helio-informatics.org/FEMET_WeiLiu_20110523_210052Su//Su: Mass is seen moving from one leg to another::http://aia.cfa.harvard.edu/filament/index.html?search=022202232011-05-23T00:00:122011-05-23T06:45:12-2984072.0QSFSRYNYNN-0389FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/05/CME0079/CME.html[-490,-106,169,646][592,2511,2188,3267]Sigmoid filament eruptionWei LiuA sigmoid-shaped filament erupts, unwraps itself (see the dark 304 features with twists), and leads to flaring (see the separating flare ribbons seen at 211).88ivo://helio-informatics.org/FEMET_WeiLiu_20110523_214646Su11Su: Stuff is seen leaving in 304 A movie, sigmoid::http://aia.cfa.harvard.edu/filament/index.html?search=022302242011-05-27T00:49:452011-05-27T05:01:45-2708261.0PCCSRNNYNN-N-[-618,79,478,1174][959,2238,3065,3784]Non-CME eruption Nariaki Nitta;;Likely to be a failed eruption -- no obv ious CME in LASCO.99ivo://helio-informatics.org/FE304_halocme_20110530_041744SuBBSu: It happens onthe disk and it's a polar-crown filament eruption::http://aia.cfa.harvard.edu/filament/index.html?search=022402252011-05-28T09:30:022011-05-28T17:00:025516421.0QSC?S?RNNN?NN-N-[239,864,408,877][2328,3607,2759,3478]Faint filament eruption Nariaki NittaHard to see, and only in 304 A images, probably related to the narrow CME observed by LASCO (starting 17:46 UT at PA of ~340 deg).99ivo://helio-informatics.org/FE304_halocme_20110530_221901SuMcCauley: Can be seen very faintly in 304--the HEK movie has better scaling for it. No CME detection by CACTus. Su: It displays no signal to suggest a eruption on the disk, but there is a small eruption behind the limb::http://aia.cfa.harvard.edu/filament/index.html?search=022502262011-05-28T14:30:022011-05-28T16:58:50435-5822.0QSO?SYNNNN-N-[224,646,-740,-423][2134,3413,719,1438]Small filament eruption Nariaki Nitta44A filament seems to break up and part of it erupted.99ivo://helio-informatics.org/FE304_halocme_20110603_234112SuooSu: Filament is seen moving sideway while it looks like just a kind of simple activation rather than a eruption::http://aia.cfa.harvard.edu/filament/index.html?search=022602272011-05-29T12:30:022011-05-29T14:30:02-367-8351.0QSC?S?RNNNNN-N-[-480,-254,-745,-926][797,2076,296,1015]Minor filament eruption Nariaki Nitta$$A minor eruption seen only in 304 A.99ivo://helio-informatics.org/FE304_halocme_20110531_013707SuNNMcCauley: Very faint absorption visible in 193. Su: No apparent motion is seen::http://aia.cfa.harvard.edu/filament/index.html?search=022702282011-05-30T08:00:022011-05-30T12:30:02-6886943.0QSFARYNNYN-0248FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/05/CME0103/CME.html[-1235,-141,147,1242][0,3241,2274,4095]&&Prominence eruption with legs occulted Nariaki Nitta99The filament on this side of the limb seems to be intact.99ivo://helio-informatics.org/FEMET_halocme_20110604_015414SuSu: Mass is seen leaving from the surface in 304 A movie and twisting legs are seen in 171 A movie and 193 A movie displays a cavity::http://aia.cfa.harvard.edu/filament/index.html?search=02280229-----1---------------Karel SchrijverccQS filament, north of smallish AR, erupts, followed by the evolution of post-eruption loop systems.@@ivo://helio-informatics.org/FEMET_KarelSchrijver_20110608_142943---02302011-06-05T01:59:562011-06-05T07:59:56-3096043.0QSP?ARYNYNN-0511FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/06/CME0027/CME.html[-756,138,157,1051][574,2493,2515,3594]''Filament eruption in a quiescent region Nariaki NittaooThis eruption may account for a slow proton event. There is no trace of this event in GOES X-ray light curves.99ivo://helio-informatics.org/FEMET_halocme_20110606_053627Su33Su: It's a asymmetric filament eruption, untwisting::http://aia.cfa.harvard.edu/filament/index.html?search=023002312011-06-06T01:40:042011-06-06T09:48:045562905.0IPP?SRYYYNB6.7kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/06/06/gev_20110606_0524/index.html0374FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/06/CME0037/CME.html[207,905,38,542][2335,3614,2172,2891]Filament eruptionKarel SchrijverFilament eruption@@ivo://helio-informatics.org/FEMET_KarelSchrijver_20110608_163746Su55Su: A beautiful kink is displayed in all three movies::http://aia.cfa.harvard.edu/filament/index.html?search=023102322011-06-06T03:36:042011-06-06T09:44:04-946-4272.0QSC?ARNNYNN-N-[-1215,-677,-769,-84][0,2029,768,1907]Prominence eruptionKarel Schrijver))Prominence eruption and hot coronal rain.@@ivo://helio-informatics.org/FEMET_KarelSchrijver_20110608_164028Su]]Su: The filament is seen rising slightly and mass is seen moving back to the surface, tornado::http://aia.cfa.harvard.edu/filament/index.html?search=023202332011-06-06T04:36:042011-06-06T13:08:04816-8255.0QSPSRNNYNN-0374FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/06/CME0037/CME.html[429,1202,-527,-1124][2176,4095,133,1212]Polar-crown prominence eruptionKarel SchrijverPolar-crown prominence eruption@@ivo://helio-informatics.org/FEMET_KarelSchrijver_20110608_164640SuSu: Stuff is seen leaving in 304 A movie and dark fibre is seen in 193 A movie, the nearby tornado is disturbed by the eruption, tornado, U shape::http://aia.cfa.harvard.edu/filament/index.html?search=023302342011-06-07T05:35:562011-06-07T10:31:56611-3555.0ARPS?RY?NN?NM2.5kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/06/07/gev_20110607_0616/index.html0694FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/06/CME0040/CME.html[-6,1228,-881,171][2039,4094,879,2034]Vast filament eruptionKarel Schrijver""An M2.5 flare associated with the largest, most impressive filament eruption seen to date with AIA. Large amounts of chromospheric material are thrown upward (much is part of a CME), with subsequently much falling down again and creating impact brighteninings over half a solar radius away.@@ivo://helio-informatics.org/FE211_KarelSchrijver_20110608_152355SuqqSu: A strong eruption results in a mount of mass jetted out and a CME is follwed, famous and magnificent eruption::http://aia.cfa.harvard.edu/filament/index.html?search=023402352011-06-09T11:47:562011-06-09T17:44:561335942.0QSF?SRNNN?NN-N-[-151,418,834,354][1631,2910,2679,3398]Minor filament eruption Thomas BergerDDSmall filament erupts from central meridian in Northern hemisiphere.99ivo://helio-informatics.org/FE211_TBerger_20110610_184536SuMcCauley: Seems like a full eruption whose material may have escaped, but it becomes too diffuse to distinguish on the disk and there wasn't enough material to produce a signature at LASCO. Su: An eruption with poor seeing on the disk::http://aia.cfa.harvard.edu/filament/index.html?search=023502362011-06-09T18:08:562011-06-09T23:56:56-6158535.0QSFSRNNNNN-0234GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/06/Flow0034/CME.html[-979,-251,1073,634][384,1663,3111,3830]Backside filament eruption Thomas Berger>>Eruption of moderately sized filament from behind the NE limb.99ivo://helio-informatics.org/FE304_TBerger_20110610_184321SuYYSu: This arcade-like filament eruption is behind the limb with clearly no twist signature::http://aia.cfa.harvard.edu/filament/index.html?search=023602372011-06-11T08:14:562011-06-12T08:29:56-34210575.0PCP?RYNYYN-Y?-[-597,-88,1321,793][518,2437,3016,4095]High latitude filament eruptio Mark Cheung&&Quiescent filament lifting off gently.<>A long arched quiescent filament lifts off the southwest limb.< CME associated with a B4.7 flare Nariaki Nitta""A well-observed filament eruption.99ivo://helio-informatics.org/FEMET_halocme_20110718_233738SuwwSu: Opening field lines are seen and mass is seen thrown out and at the footpoints of the filament bright arcs are seen::http://aia.cfa.harvard.edu/filament/index.html?search=025202532011-07-09T19:00:042011-07-09T23:48:04-5686282.0QSP?A?R?NYYN-N-[-639,-498,589,666][461,1740,2734,3453]Miniature filament eruption Thomas Berger[[Relatively tiny eruption of a filament above what appears to be an ephemeral active region.99ivo://helio-informatics.org/FE171_TBerger_20110712_011535SuMcCauley: Any signature at LASCO is washed out by a large eruption to the north. Su: A small jet near a tornado filament which rises but no evidence of eruption in the movie::http://aia.cfa.harvard.edu/filament/index.html?search=025302542011-07-14T04:10:092011-07-14T14:10:09-1419112.0PCPASYNYNN-N?-[-513,232,769,1052][1174,2453,3206,3925]%%Spiraling quiescent filament eruption Mark Cheung77This quiescent filament spirals around as it lifts off.<>Su: A sharp flare with much mass thrown out and a CME followed::http://aia.cfa.harvard.edu/filament/index.html?search=02690270-----1---------------Wei LiuffA large filament eruption during the M9.3 flare, on a spatial scale similar to the 2011 June 07 event.88ivo://helio-informatics.org/FE304_WeiLiu_20110809_012037---02712011-08-05T15:20:042011-08-05T22:50:048306154.0QSC?S?RYNYYN-N-[703,957,541,689][2792,4071,2714,3433]Mini Filament eruptionWei LiuDDMini Filament eruption near the west limb, to the north of AR 11260.88ivo://helio-informatics.org/FE304_WeiLiu_20110809_014759Su11Su: A small filament eruption with rolling motion::http://aia.cfa.harvard.edu/filament/index.html?search=027102722011-08-06T08:00:042011-08-06T12:00:04771-6423.0QSFARYNNNN-0299FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/08/CME0019/CME.html[480,1061,-887,-398][2693,3972,618,1337]""Prominence eruption southwest limbWei Liu..A filament lifted off from the southwest limb.88ivo://helio-informatics.org/FE304_WeiLiu_20110809_014039Su$$Su: Mass is seen leaving the surface::http://aia.cfa.harvard.edu/filament/index.html?search=027202732011-08-07T00:00:042011-08-08T12:50:04478262.0PCCASNNYNN-N-[-718,812,568,1083][852,3401,2662,4095]Filament Eruption Coronal RainAlberto SainzdaldaiiFilament eruption in the North polar cap, ending with a broken loop returning to the Sun as coronal rain.CCivo://helio-informatics.org/FEMET_AlbertoSainzDalda_20110811_005320Su[[Su: This polar-crown filament rises up then moves sideways, appears to be a failed eruption::http://aia.cfa.harvard.edu/filament/index.html?search=027302742011-08-10T00:00:042011-08-10T13:18:04510382.0PCP?S?NNNN-N?-[-250,260,871,1205][1417,2696,3376,4095]''Filament crawling across the north poleAnna MalanushenkoA filament literally crawls across the North pole. Part of it slowly takes off as it passes across the pole (as seen in the plane of the sky). No associted structures are seen in 211A and 171A.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110811_181525Su88Su: it looks like a tornado moving across th polar-crown::http://aia.cfa.harvard.edu/filament/index.html?search=027402752011-08-10T15:16:042011-08-10T16:56:04-8192594.0IPP?SSYYNNN-0347FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/08/CME0047/CME.html[-1114,-523,93,425][44,1323,2120,2839]Fast filament eruptionAnna MalanushenkoA small flux rope lifts up extemely fast, the kinks at a slower pace and then takes off. This is followed by footpoint brightening.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110811_183240SuMcCauley: Part of the southern leg, seen best in the 193 absorption, seems not to erupt and goes from absorption to emission at the very end of the event, perhaps from being heated. Su: A fast eruption with a small kink. Bright arcs are seen at the footpoints::http://aia.cfa.harvard.edu/filament/index.html?search=027502762011-08-11T09:12:042011-08-11T11:56:041027935.0ARFSSYYNNC6.2kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/08/11/gev_20110811_0934/index.html0976FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/08/CME0049/CME.html[861,1192,-89,274][2816,4095,1843,2562],,Spectacular large inclined filament eruptionAnna MalanushenkoHHLarge filament eruption following a flare in the same AR. The flux rope is clearly kinked. The eruption is going outwards in a direction at least (visually) 45 degrees off the radial direction. A brignt dot is seen in the core. The outline of the cavity is seen in all channels including 304A. The eruption prodices an EUV wave.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110812_233225SuCCSu: A beautiful kink is appears after a bright flare in 304 A movie::http://aia.cfa.harvard.edu/filament/index.html?search=027602772011-08-12T01:32:042011-08-12T05:02:04-5227563.0QSF?ARYNYNN-0346FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/08/CME0050/CME.html[-899,-144,512,1001][539,1818,2949,3668]Thin filament eruptionAnna MalanushenkoWWThin filament eruption on the disk with clear brightening of the footpoints afterwards.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20110815_193420SuAASu: Opening field lines and twisting legs are seen in 304 A movie::http://aia.cfa.harvard.edu/filament/index.html?search=027702782011-08-13T00:00:042011-08-13T08:25:04-7897653.0PCPSRYNYNN-0235FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/08/CME0060/CME.html[-1031,-548,582,948][93,1372,2964,3683]Prominence eruption Thomas BergerSmall/medium prominence on NE limb erupts to the NE and onto the disk. Most 304 emission appears to come down on disk to the West of the eruption.99ivo://helio-informatics.org/FEMET_TBerger_20110816_004806Su$$Su: tornado U-shape vertical threads::http://aia.cfa.harvard.edu/filament/index.html?search=027802792011-08-16T02:35:042011-08-16T12:00:04-7997375.0PCPSRYNYNN-0471FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/08/CME0070/CME.html[-1277,-321,280,1195][0,1919,2738,3817]Filament eruption on NE limb Thomas Berger00Large intermediate prominence on NE limb erupts.99ivo://helio-informatics.org/FE304_TBerger_20110819_214134Su||Su: Material is seen rising and falling back on the surface and twisting legs are seen in 171 A movie, lots of twist, arcade::http://aia.cfa.harvard.edu/filament/index.html?search=027902802011-08-16T04:15:042011-08-16T12:00:041599512.0PCF?ARNNNNN-0301FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/08/CME0069/CME.html[-169,487,750,1152][1674,2953,3274,3993]polar eruption Thomas Berger{{Polar crown filament material (not really visible beforehand) erupts across the North pole. May be occuring on back side...99ivo://helio-informatics.org/FEMET_TBerger_20110819_214359Su33Su: A quick large-scale eruption in the polar-crown::http://aia.cfa.harvard.edu/filament/index.html?search=028002812011-08-28T10:00:042011-08-28T15:20:047288822.0QSP?ARYNNNN-N-[601,855,663,1100][2176,4095,2978,4057]Off limb filament eruption Mark CheungSeems like a flux rope is lifted off the limb. The source region is likely on the far side since no footpoint brightening can be seen.< CME Nariaki NittaThe movie is given in reverse color. The northern leg got loose first. Part of the prominence material is shared in the three wavelengths, but these images indicate a distribution in temperature.99ivo://helio-informatics.org/FE171_halocme_20111201_002847McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=032903302011-11-30T18:48:042011-12-01T00:00:04981165.0IPF?SY?NNC3.6kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/11/30/gev_20111130_2153/index.html0548JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2011/11/CME0135/CME.html[745,1218,-276,309][2176,4095,1536,2615]Filament eruptionKarel SchrijverFilament eruption@@ivo://helio-informatics.org/FE211_KarelSchrijver_20111202_010243McCauleyQQMcCauley: A spectacularly twisted structure that is perhaps most dramatic in 171.::http://aia.cfa.harvard.edu/filament/index.html?search=033003312011-12-02T04:46:242011-12-02T21:08:245079894.5PCF?ARN?NYY?N-0416FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/CME0010/CME.html[343,671,782,1197][2254,3533,3338,4057]Eiffel Tower eruptionAnna MalanushenkoA thin long vertical prominence somewhat resembling Eiffel Tower slowly takes off on the limb; the remnants flow down towards its footpoint on the visible disk.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20111212_210920McCauleyppMcCauley: There are fascinating upflows alow the tower that are visible in 304 but perhaps most apparent in 171.::http://aia.cfa.harvard.edu/filament/index.html?search=033103322011-12-02T14:34:242011-12-02T18:18:241083745.0ARPSSYYN?NN-0484FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/CME0009/CME.html[947,1219,-57,205][2816,4095,1812,2531]Spectacular prominence eruptionAnna Malanushenko**Prominence erupts from an AR on the W limbBBivo://helio-informatics.org/FE304_AnnaMalanushenko_20111212_211615McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=033203332011-12-03T10:26:042011-12-03T13:14:0410056094.0ARF?RYN?NDN-0595FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/CME0015/CME.html[776,1235,414,804][2816,4095,2704,3423]Beautiful prominence eruptionAnna MalanushenkoA beautiful prominence eruption in AR on the W limb, in the same site as the previous day's eruption took place. Spiral structures moving upwards (unspinning?) can be seen in this prominence.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20111212_215435McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=033303342011-12-03T13:28:042011-12-03T15:24:0427111341.0PC?FS?NR?Y?NNNN-0317FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/CME0018/CME.html[37,505,1051,1217][1860,3139,3376,4095]Minor eruptionAnna MalanushenkovvMinor flux rope eruption on the NW limb. Notice the upside-down arch in 171A running upwards along with the flux rope.BBivo://helio-informatics.org/FE171_AnnaMalanushenko_20111212_220720McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=033403352011-12-03T17:34:042011-12-03T19:26:04-9524512.0IP?PARYNY?DN-0177GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/Flow0014/CME.html[-1088,-817,282,619][0,1279,2439,3158]Sympathetic eruptions?Anna Malanushenko~~A small eruption on the E limb interesting mainly because it is contemporal with a few other eruptions elsewhere on the globe.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20111212_215916McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=033503362011-12-04T00:00:042011-12-04T06:56:04-6165963.0QSPARNNYNN-0416FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/CME0022/CME.html[-910,-322,324,868][382,1661,2682,3401]Filament eruptionAnna Malanushenko00Faint eruption of large filament on the NE disk.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20111213_021247McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=033603372011-12-04T19:20:042011-12-04T20:18:04-944-3053.5ARFS?RY??NNC1.3kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2011/12/04/gev_20111204_1937/index.html0345FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/CME0025/CME.html[-1079,-809,-413,-198][0,1279,1179,1898]Small flux rope eruptionAnna Malanushenko$$Small flux rope eruption on SE limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20111213_022542McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=033703382011-12-08T03:00:042011-12-08T12:00:04-596-5473.0QS?FSRYNYDN-0193GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/Flow0042/CME.html[-1208,17,-959,-134][35,2076,564,1711]prominence on east limb Marc Derosa44Prominence eruption on the east limb next to AR11374<>Filament eruption and two-ribbon flaring near north east limb.88ivo://helio-informatics.org/FE304_WeiLiu_20120120_055508McCauleyMcCauley: The eruption looks confined in the AIA images but there is a significant CME that is seemingly associated. Edit: The overlying field can be seen opening in the 171 movie in response perhaps to the ejecta, so this is listed as a partial eruption.::http://aia.cfa.harvard.edu/filament/index.html?search=036103622011-12-27T20:50:042011-12-28T01:05:04-7294712.0QSPSRYYYN2?-0411GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/Flow0102/CME.html[-845,-613,393,549][194,1473,2474,3193]44Small filament eruption, expulsion into outer coronaWei LiuhhSmall filament eruption, expulsion into outer corona seen at 211 near the edge of the AIA field of view.88ivo://helio-informatics.org/FEMET_WeiLiu_20120120_060931McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=036203632011-12-28T11:00:042011-12-28T15:50:047206161.0QSCAR?NNYN3?-N-[560,879,493,739][2608,3887,2715,3434]Limited filament eruptionWei Liu[[a small filament eruption, most material falls back toward the one end of the filament leg.88ivo://helio-informatics.org/FE304_WeiLiu_20120120_060343McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=036303642011-12-29T15:30:002011-12-29T16:59:248974313.0QSF?RY?NN?NN-0573FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/CME0141/CME.html[571,1223,248,615][2816,4095,2408,3127],,Prominence eruption with a helical structure Nariaki NittaThe eruption is most vividly seen at 304 A with 211 A and 171 A images showing only a small part of it. The source region apears to be on the back side. Nothing like a CME front is recognized at 211 A.99ivo://helio-informatics.org/FEMET_halocme_20120102_174050McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=036403652011-12-30T17:20:242011-12-30T19:20:242087912.0PC?FSRYNNNN-0543FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/CME0149/CME.html[-548,964,366,1215][1135,3654,2658,4073]//Prominence eruption possibly from the back side Nariaki NittaNNThe eruption is best seen at 304 A. Images in other wavelengths show only part of the eruption without front-like structures ahead of the prominence as seen in some other events. The prominence appears to be linked to a region on the back side, although part of disk filaments show increased motions around the time of the eruption.99ivo://helio-informatics.org/FE211_halocme_20120102_202447McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=036503662011-12-31T20:20:242011-12-31T22:50:24-697-5892.0QSPS?RYN?YNN-0225FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2011/12/CME0155/CME.html[-1230,-163,-889,-289][0,1919,527,1606],,Prominence eruption from a front side region Nariaki NittaThe filament/prominence itself is best viewed at 304 A. It pushes material ahead of it, which is captured at 211 A and 171 A as a front (in emission). This eruption was associated with a slow CME that first appeared in the LASCO C2 image at 23:12 UT.99ivo://helio-informatics.org/FEMET_halocme_20120102_210720McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=03660367-----1---------------Karel Schrijver44QS filament eruption with post-eruption loop system.@@ivo://helio-informatics.org/FE171_KarelSchrijver_20120106_000511---03682012-01-01T00:20:242012-01-01T02:20:24-5315562.0QSPARNNY?NN-0630FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0002/CME.html[-1215,153,171,941][24,2303,2334,3615]''Filament eruption in a quiescent region Nariaki NittaThe eruption seems to be slow, although accompanying a weak two-ribbon flare (not showing up in GOES with a ~B4 background lebel). The associated CME is narrow, but it may reflect an edge-on perspective.99ivo://helio-informatics.org/FEMET_halocme_20120102_215537McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=036803692012-01-02T14:24:042012-01-02T15:56:049922304.0AR?F?NRYNNNC2.4kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/02/gev_20120102_1431/index.html0714FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0007/CME.html[762,1223,-138,599][1913,4095,1820,3045]**Prominence eruption from behind the W limbKarel SchrijverA prominence erupts from behind the W limb, displaying a complex rope-like structure, with high coronal oscillations excited in the process.@@ivo://helio-informatics.org/FEMET_KarelSchrijver_20120106_010033McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=036903702012-01-05T11:00:042012-01-05T14:00:041866473.5QSFARYN?YNC2.2kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/05/gev_20120105_1151/index.htmlY?-[-837,1210,71,1222][653,4064,2167,4084]..Filament eruption associated with a C2.1 flare Nariaki NittaaaOne end of the filament appears to open up, and the other end grows into what looks like a surge.99ivo://helio-informatics.org/FEMET_halocme_20120111_073735McCauley//McCauley: LASCO data gap precluded a CME entry.::http://aia.cfa.harvard.edu/filament/index.html?search=037003712012-01-07T17:10:042012-01-07T19:20:04872-4772.0IP?C?S??N?NN-N-[568,1176,-678,-276][2816,4095,894,1613]Prominence eruptionWei LiuFFA small scale prominence eruption on the limb, it opens up and erupts.<>ivo://helio-informatics.org/FE304_ThomasBerger_20120119_221331McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=037303742012-01-13T14:10:042012-01-14T00:00:04-797-2303.0QSFARY?NND?N-Y?-[-1175,-419,-442,-17][80,1359,1306,2025]""Small but bright filament eruption Thomas BergerttSmall filament in quiet Sun region erupts with a very bright two-ribbon flare and subsequent post-flare loop arcade.>>ivo://helio-informatics.org/FE304_ThomasBerger_20120119_222054McCauley66McCauley: LASCO data gap precluded a CACTus CME entry.::http://aia.cfa.harvard.edu/filament/index.html?search=037403752012-01-14T00:00:042012-01-15T00:00:046244064.0QSO??Y?NYNN-N-[429,819,197,616][2449,3728,2366,3085]!!Filament interaction and eruption Thomas Berger..Complex system of interacting large filaments near West limb. Eruption in part of Northern filament fails to disrupt the entire structure, with the remaining portion seeming to "climb" up the post-flare loop arcade left by the eruption. This eruption then activates the Southern filament significantly.>>ivo://helio-informatics.org/FE211_ThomasBerger_20120119_234614McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=037503762012-01-17T22:00:042012-01-18T03:00:04-301-2103.0ARCS?SY?NNB8.5kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/18/gev_20120118_0117/index.htmlN-[-636,33,-554,133][528,2564,1126,2269]Filament eruption in SEWei Liu,,A sizable filament in the southeast erupted.88ivo://helio-informatics.org/FE304_WeiLiu_20120120_044340McCauleyMcCauley: A small active region filament erupts, which appears to cause the collapse of the large, quiet-sun filament to the north.::http://aia.cfa.harvard.edu/filament/index.html?search=03760376b2012-01-17T22:00:042012-01-18T03:00:04-301-2103.0QSO??YNYNB8.5kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/18/gev_20120118_0117/index.htmlN-[-636,33,-554,133][528,2564,1126,2269]Filament eruption in SEWei Liu,,A sizable filament in the southeast erupted.88ivo://helio-informatics.org/FE304_WeiLiu_20120120_044340McCauleyMcCauley: A small active region filament erupts, which appears to cause the collapse of the large, quiet-sun filament to the north.;;http://aia.cfa.harvard.edu/filament/index.html?search=0376b03772012-01-18T04:30:042012-01-18T09:45:044718991.5PCPARN?NYNN-0137GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/Flow0046/CME.html[363,579,824,974][2194,3473,3187,3906]Prominence eruption on NW limbWei LiueeProminence eruption on NW limb.Most erupted material falls back along the two legs of the prominence.88ivo://helio-informatics.org/FE304_WeiLiu_20120120_045650McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=037703782012-01-19T04:15:042012-01-19T10:00:046718343.0QSFANR?N?NYNN-0422FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0063/CME.html[499,842,691,976][2526,3805,3078,3797];;Coronal Condensation at dip (cusp), and prominence eruptionWei Liu304 cool material condenses out of nowhere at a cusp (dip) seen at 171. Similar coronal condensation forming prominence/coronal rain has recently been captured (Liu, Berger, Low 2012, ApJ Letters). Shortly after this condensation, a nearby large filament/prominence erupted.88ivo://helio-informatics.org/FE304_WeiLiu_20120120_050955McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=03780379-----1---------------Wei LiuRRA large filament erupted near the north west limb, causing two-ribbon brightening.88ivo://helio-informatics.org/FE304_WeiLiu_20120120_052612---03802012-01-19T12:50:042012-01-19T17:00:04-3037315.0IPF?A?RY?ND M2.6|M3.2http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/19/gev_20120119_1343/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/19/gev_20120119_1344/index.html1714FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0065/CME.html[-864,257,415,1046][583,2502,2726,3805]Large Filament channel eruptionWei LiuA large filament channel (seems the flux rope cavity itself) erupted, causing ribbons brightenings expanding outward, and disturbance/oscillation in the ambient corona.88ivo://helio-informatics.org/FE304_WeiLiu_20120120_051730McCauley::McCauley: Beautiful supra-arcade downflows visible in 193.::http://aia.cfa.harvard.edu/filament/index.html?search=038003812012-01-20T19:45:042012-01-20T23:45:049815103.0ARPSRYYNNC1.3kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/20/gev_20120120_2101/index.html0416FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0069/CME.html[752,1210,363,657][2816,4095,2539,3258]small AR filament eruptionWei LiuddA small active region filament erupted near the northwest limib. Ejection pushes nearby loops aside.88ivo://helio-informatics.org/FE304_WeiLiu_20120131_031357McCauleyMcCauley: The CME at LASCO is pretty impressive given how small the filament was and how little of it appeared to escape in the 304 observations.::http://aia.cfa.harvard.edu/filament/index.html?search=038103822012-01-20T20:45:042012-01-20T22:45:04-994-1993.0IP?PSRYN?Y?NN-0361FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0070/CME.html[-1158,-831,-321,-78][0,1279,1356,2075]Loop-shaped prominence eruptionWei LiullLoop-shaped prominence eruption on the southeast limb. A lot of material falls back toward its southern leg.88ivo://helio-informatics.org/FE304_WeiLiu_20120131_033527McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=038203832012-01-21T07:00:042012-01-21T15:00:048634575.0IPP?RYY?YNC2.4kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/21/gev_20120121_1335/index.html0334FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0072/CME.html[630,1095,325,590][2816,4095,2451,3170],,3 sympathetic/consecutive filament eruptionsWei Liu..The filament on the disk (not the largest one near the disk center) first erupted, producing a nice two-ribbon flare. Then the one closer to the limb erupted, producing a surge (most mass falls back along a spine-fan like trajectory), rapidly followed by another filament eruption from the same region.88ivo://helio-informatics.org/FE304_WeiLiu_20120131_032842McCauleyMcCauley: After the first filament eruption occurs, the large filament to the left rapidly rises as though it might also erupt but instead reaches stability at new height.::http://aia.cfa.harvard.edu/filament/index.html?search=03830383b2012-01-21T07:00:042012-01-21T15:00:048634575.0ARPS?RYYNNC2.4kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/21/gev_20120121_1335/index.html0334FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0072/CME.html[630,1095,325,590][2816,4095,2451,3170],,3 sympathetic/consecutive filament eruptionsWei Liu..The filament on the disk (not the largest one near the disk center) first erupted, producing a nice two-ribbon flare. Then the one closer to the limb erupted, producing a surge (most mass falls back along a spine-fan like trajectory), rapidly followed by another filament eruption from the same region.88ivo://helio-informatics.org/FE304_WeiLiu_20120131_032842McCauleyMcCauley: After the first filament eruption occurs, the large filament to the left rapidly rises as though it might also erupt but instead reaches stability at new height.;;http://aia.cfa.harvard.edu/filament/index.html?search=0383b03842012-01-22T02:15:002012-01-22T06:15:00805-6303.0QSPARYYYNN-0383FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0074/CME.html[388,1222,-864,-395][2176,4095,459,1538]==Prominence eruption showing untwisting motions and down flows Nariaki NittaThese motions are most readily seen at 304 A, with the large-scale structures in 211 A and 171 A hardly affected. This results in a slow CME that contains a flux rope.99ivo://helio-informatics.org/FEMET_halocme_20120126_024034McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=038403852012-01-22T13:40:122012-01-22T16:40:126833271.0QSCA?RNNYNC3.7kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/22/gev_20120122_1238/index.htmlN-[-1,1367,-58,711][1816,4095,1952,3233]..Filament eruption dominated by dowward motions Nariaki NittaThe movie gives an impression that the filament material just comes back to the Sun, but some of it may have escaped into the heliosphere. The surrounding large-scale loops at 193 A and 171 A seem to be largely unaffected.99ivo://helio-informatics.org/FEMET_halocme_20120126_225314McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=038503862012-01-22T21:00:362012-01-23T00:00:367155781.5QSPAS?Y?NYNN-0290GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/Flow0070/CME.html[231,1198,306,850][2176,4095,2472,3551]''Filament eruption with strong downflows Nariaki NittattAgain, the movie shows downflows more than the eruption. But this is associated with a slow CME observed by LASCO.99ivo://helio-informatics.org/FE211_halocme_20120126_230212McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=038603872012-01-23T00:00:042012-01-23T06:00:043057485.0IPPARYYY?D C1.9|M8.7http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/23/gev_20120123_0039/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/01/23/gev_20120123_0338/index.html1092FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0080/CME.html[-165,775,278,1218][1597,3516,2755,3834]""Eruptions leading to two halo CMEs Nariaki NittaThis movie contains two episodes of eruptions producing two halo CMEs. The first one is less noticeable, until 02:30 or so, showing opening up of large-scale structures. The second event involves the eruption of a clear filament, whose activation already started during the first episode. The halo CME from the second event is more northward and much faster, overtaking the second one by 04:12 UT.99ivo://helio-informatics.org/FEMET_halocme_20120126_231732McCauleyMcCauley: The 171 movie is spectacular, as it appears to show loops rapidly expanding or opening just prior to the eruption. The region is also a nice sigmoid.::http://aia.cfa.harvard.edu/filament/index.html?search=038703882012-01-25T11:18:042012-01-25T13:34:04946-4062.0QSP?S?RY?NNNN-0277FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0111/CME.html[636,1257,-580,-231][2816,4095,1013,1732]Small double-staged eruptionAnna MalanushenkoSmall prominence eruption on the SW limb is followed by an appearance of a sigmoid-like structure which possibly erupts as well.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20120126_023648McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=038803892012-01-27T14:04:042012-01-27T16:20:04-1114-33.0QS?FARYY?NNN-N-[-1291,-938,-118,111][0,1279,1683,2402]DNA-like eruptionAnna MalanushenkoJJThin filament unwinds during the eruption. Two ribbons are clearly visible, somewhat resembling a DNA spiral. Note a small "puff" off the limb to the S of the filament, ejected at the same time as the filament. It seems from the movie that it was ejected from the footpoint of the filament which got disconnected from the surface.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20120128_024138McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=038903902012-01-27T17:06:042012-01-27T19:32:04-7237604.0ARC?ASYNYNN-Y?-[-933,-513,439,1081][0,1919,2775,3854]Beautiful slow eruptionAnna MalanushenkoThis beautiful slow prominence eruption takes place shortly after a major eruption and X-class flare on the other side of the limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20120128_022311McCauleyMcCauley: The CME signature is washed out by a full halo CME associated with the X-flare mentioned above: http://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/01/CME0125/CME.html::http://aia.cfa.harvard.edu/filament/index.html?search=039003912012-02-04T13:00:042012-02-04T14:00:04-1025-3792.0QS?P?S?RY?Y?NNN-0138GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/02/Flow0013/CME.html[-1222,-828,-526,-232][0,1279,1057,1776]Behind-the-limb eruption Mark CheungUUThe absence of footpoint brightenings indicates the source region is on the far side.<>ivo://helio-informatics.org/FE211_ThomasBerger_20120215_204736McCauley77McCauley: Faint hint of kinking in the second eruption.::http://aia.cfa.harvard.edu/filament/index.html?search=039603972012-02-19T13:58:042012-02-19T20:14:046698493.0QSFANRYNY?YN-0393JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2012/02/CME0039/CME.html[444,894,518,1179][2137,4095,2913,4012]Beautiful eruptionAnna MalanushenkoA beautiful filament eruption on the limb. In the initial phase of the rise an unswirling "slinkie" could be seen, and later it appears as a spinning cone. Part of the filament is seen to fall back down while most of it eripts. It is a little unusual that the emission ends abruptly in the middle of the filament, as it only half of it was emitting. As if the 304A slinkie is only attached to the surface at one end and the other end is free.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20120301_225204McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=039703982012-02-23T00:00:042012-02-24T00:00:04-4035465.0TEPA?R??NYYN-N-[-776,-31,8,1084][0,3188,2063,3854]QS filament eruptionKarel SchrijverA very long, curved filament, from polar crown into low-latitude AR, destabilizes, with an eruption at high latitude and a draining flow in the AR environment.@@ivo://helio-informatics.org/FE193_KarelSchrijver_20120224_212752McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=039803992012-02-23T05:12:042012-02-23T14:56:048514472.0IP?FARY?NNNN-0403JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2012/02/CME0051/CME.html[496,1207,-185,1079][352,4095,1741,3846]Prominence eruptionKarel SchrijveraaProminence eruption over NW limb, with post-eruption arcade from AR into QS, straddling the limb.@@ivo://helio-informatics.org/FE193_KarelSchrijver_20120224_212351McCauleyiiMcCauley: Interesting swirling (twisting?) motions visible in the absorption structures seen well in 193.::http://aia.cfa.harvard.edu/filament/index.html?search=039904002012-02-24T00:00:042012-02-24T12:25:04-4344634.0QSFA?RNNYNN-0581JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2012/02/CME0061/CME.html[-768,-101,17,910][2,2646,2078,3563]99Huge filament eruption and two-ribbon flare - no Xrays... Thomas BergerA large rapid filament eruption is followed by a huge two-ribbon "flare" front moving across the disk. The GOES X-ray signature of this event is unusally faint.>>ivo://helio-informatics.org/FEMET_ThomasBerger_20120228_214113Schanche-::http://aia.cfa.harvard.edu/filament/index.html?search=040004012012-02-24T03:00:042012-02-25T04:00:04-622-6674.0QSPSRY?NYYN-0534JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2012/02/CME0068/CME.html[-903,-342,-1077,-258][0,2427,254,1617]>>Another larger filament eruption with no X-ray flare signature Thomas Berger--Similar to the larger event earlier in the day, this filament eruption shows no GOES X-ray signature in spite of the large two-ribbon "flare" front that follows the filamant eruption. There is a marked rise in proton flux starting at ~3 UT on the 25th. Was this event or the earlier event responsible?>>ivo://helio-informatics.org/FE211_ThomasBerger_20120228_215648Schanche-::http://aia.cfa.harvard.edu/filament/index.html?search=040104022012-03-05T09:30:002012-03-05T12:00:00-8134642.0IPFSNR?Y?NYN1?-0638JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2012/03/CME0014/CME.html[-1231,-396,230,699][0,1919,2283,3362]Hesitant filament eruption Nariaki NittaThe eruption of the filament material is well traced in the three channels, but the 211 A images do not clearly show a front. The associated CME is narrow and not spectacular.99ivo://helio-informatics.org/FE211_halocme_20120313_005518Schanche-::http://aia.cfa.harvard.edu/filament/index.html?search=040204032012-03-08T03:00:002012-03-08T04:32:00924-3001.0QS?P?NRYYYNN-N?-[642,1205,-458,-141][2816,4095,1189,1908]''Prominence eruption and coronal dimming Nariaki Nitta]]As a prominence moves out untwisted the overlying corona appears to dim (at 171 A and 211 A).99ivo://helio-informatics.org/FEMET_halocme_20120315_075507SchancheWWSchanche: LASCO data in the Cactus catalog are no good at this time, so CME is unknown.::http://aia.cfa.harvard.edu/filament/index.html?search=040304042012-03-08T09:50:242012-03-08T12:20:243966441.0ARC??NNNNC1.7kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/03/08/gev_20120308_1019/index.htmlN-[-323,1115,240,1048][1511,3906,2449,3794] Two filament eruptions far apart Nariaki Nitta``Two filament eruptions are seen around the same time near central meridian and on the west limb.99ivo://helio-informatics.org/FE211_halocme_20120315_151906SchanchevvSchanche: The first value is the eruption near the central meridian; the second is the small eruption near the W limb.::http://aia.cfa.harvard.edu/filament/index.html?search=04040404b2012-03-08T09:50:242012-03-08T12:20:243966441.0QSCS?NNYYC1.7kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/03/08/gev_20120308_1019/index.htmlN-[-323,1115,240,1048][1511,3906,2449,3794] Two filament eruptions far apart Nariaki Nitta``Two filament eruptions are seen around the same time near central meridian and on the west limb.99ivo://helio-informatics.org/FE211_halocme_20120315_151906SchanchevvSchanche: The first value is the eruption near the central meridian; the second is the small eruption near the W limb.;;http://aia.cfa.harvard.edu/filament/index.html?search=0404b04052012-03-08T14:30:002012-03-08T18:32:00-962762.0IP?PARYNYNC1.1kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/03/08/gev_20120308_1617/index.html0440JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2012/03/CME0029/CME.html[-1552,-373,-255,408][0,1963,1624,2727]22Activation and eruption of a prominence into a CME Nariaki NittaQQThe prominence standing over the limb is seen to gradually rise. It is not clear if a small eruption in the disk region has to do with triggering the eruption of the prominence. The southern part is more clearly opened up, throwing material northward, hence the appearance of the associated CME in LASCO data that is extended to north.99ivo://helio-informatics.org/FE304_halocme_20120315_160103Schanche<>ivo://helio-informatics.org/FEMET_ThomasBerger_20120326_173714Schanche-::http://aia.cfa.harvard.edu/filament/index.html?search=041504162012-03-25T14:20:042012-03-26T02:21:40-6767823.0QSCSRY?NY?Y?N-N-[-884,-467,580,984][283,1562,2992,3711]**Interacting filament systems with eruption Thomas BergerTwo of the large mid-latitude filaments near the East limb interact to cause multiple eruptions. Small coronal cavities are visible above the filaments on the East limb.>>ivo://helio-informatics.org/FE211_ThomasBerger_20120326_181312Schanche-::http://aia.cfa.harvard.edu/filament/index.html?search=04160416b2012-03-25T14:20:042012-03-26T02:21:40-6767823.0QSPSRYYYY?N-N?-[-884,-467,580,984][283,1562,2992,3711]**Interacting filament systems with eruption Thomas BergerTwo of the large mid-latitude filaments near the East limb interact to cause multiple eruptions. Small coronal cavities are visible above the filaments on the East limb.>>ivo://helio-informatics.org/FE211_ThomasBerger_20120326_181312Schanche-;;http://aia.cfa.harvard.edu/filament/index.html?search=0416b04172012-03-26T21:45:042012-03-27T04:00:04-7904564.0QSCSRN?NYNN-N-[-1049,-531,292,619][92,1371,2448,3167]Ring filament eruption Thomas BergerNearly closed ring filament erupts, apparently in response to massive eruption behind the East limb and subsequent coronal wave.>>ivo://helio-informatics.org/FEMET_ThomasBerger_20120402_175353SchancheSchanche: Filament event occurs just after a large eruption behind the limb. There is a lot of interesting structure in the surrounding absorption features in 171.::http://aia.cfa.harvard.edu/filament/index.html?search=041704182012-03-27T00:50:042012-03-27T04:00:041014592.0ARFAR?N?NNNC5.3kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/03/27/gev_20120327_0250/index.html0822FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/03/CME0122/CME.html[-31,234,371,547][1578,2857,2454,3173]Compact AR eruption and flare Thomas BergerVery bright compact AR 11442 unleashes C5.3 flare and filament eruption, possibly in response to massive eruption and coronal wave event that takes place behind the East limb several hours earlier.>>ivo://helio-informatics.org/FEMET_ThomasBerger_20120402_180324Schanche-::http://aia.cfa.harvard.edu/filament/index.html?search=041804192012-03-27T03:20:042012-03-27T06:20:041774231.0ARF?A?S?YNNNC1.7kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2012/03/27/gev_20120327_0421/index.htmlN-[-105,460,262,584][1704,2983,2394,3113]AR 11442 filament eruption Thomas Berger99Filament eruption from compact, very EUV bright, AR 11442. The eruption is preceded by large-scale topological rearrangement that appears to propagate around the dome-like AR to finally expel material to the West. Note the nteresting "prarie fire" flare that expands and then contracts just prior to the eruption.>>ivo://helio-informatics.org/FEMET_ThomasBerger_20120402_213159SchancheMcCauley: Seems like a full eruption of the filament. It's not positioned favorably for a CME to register at LASCO and any minor signature would have been washed out by a large halo event around the same time from the back side.::http://aia.cfa.harvard.edu/filament/index.html?search=041904202012-03-29T14:56:042012-03-29T22:20:04438261.0QSFSRN?NYNN-0946FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/03/CME0140/CME.html[-517,604,512,1139][1161,3080,2884,3963]//Filament eruption and post-eruption loop bundleAnna MalanushenkoA large filament in the N heisphere slowly takes off northwards. Some of the plasma in it could be seen in 171A flowing down the footpoints of the flux rope. Right after the eruption, a compact bundle of loops brighten up, that might belong to the post-eruption arcade. Given the length of this filament, the arcade is probably long too; why one small bundle in the middle of it brightens up and th rest does not?BBivo://helio-informatics.org/FEMET_AnnaMalanushenko_20120405_004124SchancheMcCauley: Seems like a full eruption of the filament. It's not positioned favorably for a CME to register at LASCO and any minor signature would have been washed out by a large halo event around the same time from the back side.::http://aia.cfa.harvard.edu/filament/index.html?search=042004212012-03-29T23:04:042012-03-30T05:32:042528811.0PCPSRYNYNN-0131GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/03/Flow0041/CME.html[-251,756,578,1184][1509,3428,2977,4056]Slow filament eruptionAnna MalanushenkoLarge filament close to the N pole becomes activated, slowly lifts up and seemingly breaks into two halves, which sink back into the surface.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20120405_031859Schanche-::http://aia.cfa.harvard.edu/filament/index.html?search=042104222012-03-30T11:38:042012-03-30T19:20:04-6277393.0QSPA?NRY?YNN-0744FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/03/CME0143/CME.html[-786,-468,448,1030][44,1963,2740,3819]Filament reconnectionAnna MalanushenkoOne end of a large filament appears to lift up, swirl around, making a cone-like shape in the plane of the sky, and seemingly reconnects to some other part on the disk.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20120405_032615SchancheWWSchanche: Movie error : There is a jump in the 304 movie right when it reaches its max.::http://aia.cfa.harvard.edu/filament/index.html?search=042204232012-03-30T22:30:042012-03-31T07:00:04-5587634.0QSPA?Y?NYNN-N?-[-874,-242,377,1149][0,2285,2678,3961]Partial filament eruption Mark CheungThe northeastern portion of this quiescent filament erupts. Some material is seen to flow back down toward the remaining anchored portion of the original filament.<>Filament eruption associated with a CME and very minor flaring Nariaki NittaThe off-limb outflow is seen at 211 A and 171 A. This eruption is associated with gradual increase in the GOES 1-8 A X-rays from B1.4 to B2.0. The CME carries a long-lasting internal structure.99ivo://helio-informatics.org/FEMET_halocme_20120831_050932SchancheMcCauley: Filament seems only to activate, while a structure higher in the corona off-limb erupts. See 193 or HEK movie. Schanche: I wouldn't so much call this a filament eruption as a filament movement. The material never rises far from the surface.::http://aia.cfa.harvard.edu/filament/index.html?search=053505362012-08-23T04:30:352012-08-23T06:30:35769-3342.0QSFSRYNYN2?-0571FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/08/CME0115/CME.html[285,1252,-606,-62][2176,4095,952,2031],,Filament eruption and foot-point brightening Nariaki NittaThe filament looked already fragmented prior to the eruption. The area underneath the filament brightened, especially around the two legs. By the time the erupted material reached the LASCO field of view, it was deflected to north. The CME was not impressive.99ivo://helio-informatics.org/FE304_halocme_20120831_053541Schanche-::http://aia.cfa.harvard.edu/filament/index.html?search=053605372012-08-23T15:00:032012-08-23T22:00:03504-5092.0QSC?SRNNYNN-N-[138,870,-875,-143][2249,3528,840,1559]Clear filament eruption, but... Nariaki Nitta,,This movie captures the activation of a filament, followed by eruption and post-flare loops (although there was hardly a flare on top of the ~B2 GOES background level). The eruption did not continue over the limb, nor was it observed as a CME. The eruption was probably inclined toward disk center.99ivo://helio-informatics.org/FE171_halocme_20120831_062637McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=053705382012-08-24T13:00:032012-08-24T18:00:039235521.0QSFSR?YNYNN-0232FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/08/CME0120/CME.html[375,1470,5,1099][2176,4095,2429,3508]))Untwisting motions in a filament eruption Nariaki NittaThe eruption seems to arise from the northern end of the filament becoming loose. There is an indication of untwisting or helical motions early in the eruption. The associated CME contains complex internal structures.99ivo://helio-informatics.org/FE304_halocme_20120831_055630Schanche-::http://aia.cfa.harvard.edu/filament/index.html?search=053805392012-08-25T16:00:032012-08-25T17:30:03-1014-2851.0?FSRNNNNN-0466FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/08/CME0127/CME.html[-1217,-810,-523,-48][0,1919,1033,2112]Loop-shaped prominence eruptionWei Liu[[A loop-shaped prominence eruption on SW limb, likely from the far side of the visible disk.88ivo://helio-informatics.org/FE304_WeiLiu_20120828_202039SchancheSchanche: Very little information about this eruption, as it is faint and occurred behind the limb. Very interesting double-bulb structure in the LASCO data.::http://aia.cfa.harvard.edu/filament/index.html?search=053905402012-08-25T16:00:032012-08-26T06:00:03-8606735.0QSPA?RYY?NY1?-0137GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/08/Flow0098/CME.html[-1006,-713,467,880][0,1279,2811,3530]Large prominence eruptionWei Liu--A large prominence eruption on the east limb.88ivo://helio-informatics.org/FE304_WeiLiu_20120828_201440Schanche\\Schanche: Very interesting, multi-limb structure. Also has a very interesting cavity in 171.::http://aia.cfa.harvard.edu/filament/index.html?search=054005412012-08-26T18:12:032012-08-26T18:56:038175313.0QSCSRNNYN?N-N-[770,864,486,575][2770,4049,2573,3292]$$Loop-shaped mini-prominence eruptionWei Liu22Loop-shaped, small-scale mini-prominence eruption.88ivo://helio-informatics.org/FE304_WeiLiu_20120828_204224SchancheSchanche: This was an adorable little loop. The structure developed into two sections. Some material formed an overlying loop, while some remained sticking up in the center.::http://aia.cfa.harvard.edu/filament/index.html?search=054105422012-08-27T08:40:032012-08-27T11:50:03977-3114.0IPPARYNYN1?-0210FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/08/CME0138/CME.html[725,1228,-610,-13][2176,4095,989,2068]Successive eruptionsWei LiuA loop-shaped prominence (304, red) erupted on the SW limb, exhibiting unwinding twists; this is immediately followed by another eruption nearby seen at 211 (pale blue).88ivo://helio-informatics.org/FE211_WeiLiu_20120828_222014SchancheNNSchanche: Very twisted structure, especially the southern leg of the eruption.::http://aia.cfa.harvard.edu/filament/index.html?search=054205432012-08-31T17:00:032012-08-31T22:18:03-492-3115.0IP?FS?RYNNNC8.4-0644FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/08/CME0150/CME.html[-1211,227,-715,93][31,2426,857,2202]..Filament eruption associated with a C8.4 flare Nariaki NittaThe filament seems to have completely erupted and the flare ribbons are extended. Some filament materials are seen to come back, at 304 A. Note that the compact active region has become part of the flare ribbon.99ivo://helio-informatics.org/FEMET_halocme_20120901_013402SchancheOOSchanche: The dark filament material shows a lot of twisted, dynamic structure.::http://aia.cfa.harvard.edu/filament/index.html?search=05430544-----1--------------- Nariaki NittaThis movie covers several hours after the spectacular filement eruption associated with a C8.4 flare. The remnant filament material shows interesting trajectories.99ivo://helio-informatics.org/FE304_halocme_20120904_050129---05452012-09-02T13:20:232012-09-02T16:20:236711993.0ARPA?R?YNNNN-N?-[-124,1466,-248,645][1446,4095,1634,3123]55Filament eruption triggered by a small-scale eruption Nariaki NittaThe event starts off as other examples in Series of minor eruptions (Eruption ), but this one has a consequence of getting a larger filament on the western side erupt. The filament eruption does not seem to have impact on large-scale loops hanging out on the limb as observed at 211 A.99ivo://helio-informatics.org/FE304_halocme_20120907_160456SchancheMcCauley: This CME may be related, but it looks like it might have come from the far side: http://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/09/CME0016/CME.html Schanche: There is a small, thin filament eruption just before and north of the AR where this event takes place.::http://aia.cfa.harvard.edu/filament/index.html?search=054505462012-09-04T22:04:352012-09-05T03:16:35-228-9243.0PCPA?RNNYN2?-0679FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/09/CME0028/CME.html[-451,-5,-1161,-687][709,2628,0,1079]Polar-crown filament eruptionKarel SchrijverPolar-crown filament eruption@@ivo://helio-informatics.org/FEMET_KarelSchrijver_20120906_002848McCauleyMcCauley: Missing data in these movies. See HEK. Listed as a partial eruption because it looks like an eastern component didn't erupt, but that may also be a separate structure.::http://aia.cfa.harvard.edu/filament/index.html?search=054605472012-09-09T17:26:032012-09-09T19:56:03438-5083.0QSPSRN?NNN1?-N-[252,625,-649,-366][2139,3418,843,1562]Filament eruption triggers distant brightening but does not disturb another filament in between the brightening and the eruptionAnna MalanushenkokkEruption of a small flux rope causes distant footpoint-like brightening, which is suggestive of that it broke throuth an arcade connecting to the region of the brightening. But there is another filament between the eruption and the footpoint brightening, and the reconnection in the overlying arcade does not seem to cause any disturbance to this second filament.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20120912_022405SchancheQQSchanche: Part of the filament breaks off and erupts, while part remains planted.::http://aia.cfa.harvard.edu/filament/index.html?search=054705482012-09-15T05:00:032012-09-15T06:00:03-5208971.0PCFSRNNNN?N-0548FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2012/09/CME0060/CME.html[-885,-156,684,1110][541,1820,3184,3903]Filament eruption Mark CheungSDO goes into eclipse in the middle of this event so the full event is not captured. However, one canbe fairly confident that the filament did erupt since it is no longer there after the eclipse. The time scale for evaporation of the filamentary material may take several hours.<>Eruption of a filament adjacent to, and connected with, an AR.<>Faint but clearly noticeable filament eruption on the SW disk.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130319_200101McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=064806492013-03-16T07:38:032013-03-16T12:36:038267283.0QSCS?RY?Y?YYN-N-[682,970,499,957][2176,4095,2722,3801]''Filament/cavity eruption on the NW limbAnna MalanushenkoA very slow filament eruption on the NW limb. 211A shows a small cavity at the top of th flux rope, which is slowly pushed upwards.BBivo://helio-informatics.org/FE211_AnnaMalanushenko_20130319_200419McCauleymmMcCauley: There may be kinking at the apex of the prominence, but the orientation makes it difficult to tell.::http://aia.cfa.harvard.edu/filament/index.html?search=064906502013-03-16T11:58:032013-03-16T19:14:038355345.0IPFSRYNYDN-0449JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/03/CME0045/CME.html[508,1161,228,840][2799,4078,2579,3298]Major filament eruptionAnna MalanushenkoA large-scale, beautiful filament eruption on the NW disk. Note that the ejected material bright in 304A floats around in the corona like a "cloud" for long time after the eruption. Note also beautiful post-eruption arcade. In the beginning phase the footpoints are bright enough to cause the diffraction pattern in 304A, however there is no GOES flare associated with this event. On the still image in this annotation, note several dark thin smoothly-shaped strands in the core of the erupting structure.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130319_205334McCauleyMcCauley: This eruption appears to be adjacent to the active region based on the position of the flare ribbons, and it's interesting that the filament running directly through the AR is unperturbed.::http://aia.cfa.harvard.edu/filament/index.html?search=06500651-----1---------------Anna MalanushenkoA close-up of the initial phase of the previously annotated eruption. Note that the erupting structure "consists" of thin dark semi-circularly shaped strand and a bright fringe around it. The fringe has uneven "outer" edge, and this edge is the brightest part of the whole structure.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130319_205921---06522013-03-17T11:18:032013-03-17T14:04:03335-9241.0PC?PS?NRNNNNN-0538JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/03/CME0047/CME.html[119,552,-1080,-768][1968,3247,149,868]Small eruption on the S limbAnna Malanushenko((A small filament eruption on the S limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130320_015829McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=065206532013-03-17T12:50:032013-03-17T17:14:036366363.5QSFS?RYNY?NN-0644JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/03/CME0050/CME.html[143,1130,321,951][2149,4068,2569,3648]Repeated eruptionAnna MalanushenkoWait a moment... didn't this thing erupt yesterday? The new eruption is much fainter but comparable in size to the previous one and seems to originate from the same location at the surface.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130320_020326McCauley33McCauley: Possible rolling motions along main axis.::http://aia.cfa.harvard.edu/filament/index.html?search=065306542013-03-17T14:08:032013-03-17T22:32:03-566-1264.5AR?FA?RYY?YNN-Y?-[-853,-278,-339,88][466,1745,1479,2198]Post-eruption arcadeAnna MalanushenkoSSA 211 view on the post-eruption arcade - a close-up of the event annotated earlier.BBivo://helio-informatics.org/FE211_AnnaMalanushenko_20130320_021137McCauley  McCauley: There is a LASCO data gap at the time when this event should have appeared there. Sigmoidal filament that runs through decayed active region polarities. This appears to be a decayed active region that might be sufficiently decayed as to instead be labeled QS.::http://aia.cfa.harvard.edu/filament/index.html?search=06540655-----1---------------Anna MalanushenkoAAA large filament eruption and a spectacular post-eruption arcade.BBivo://helio-informatics.org/FE211_AnnaMalanushenko_20130320_020629---06562013-03-17T18:52:032013-03-17T19:58:03-8155713.0ARF?S?RYNNNN-Y?-[-1075,-555,293,849][0,1919,2460,3539]Faint eruptionAnna Malanushenko^^One more filament eruption today. This one is much fainter and smaller than the previous ones.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130320_020838McCauleyMcCauley: There is a LASCO data gap that precluded an entry in the CME column. Interesting twisting motions in the southern leg, visible best in 171.::http://aia.cfa.harvard.edu/filament/index.html?search=065606572013-03-19T13:20:232013-03-19T16:20:235713723.0IPP?ARN?NNDC1.6kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/03/19/gev_20130319_1350/index.html0411JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/03/CME0055/CME.html[-19,1160,41,704][2017,3980,2117,3220]..Filament eruption associated with a C1.3 flare Nariaki NittaAlthough this eruption appers spectacular, it seems to affect a relatively small coronal volume in the north. A possible secondary effect may be the brightening of the region to the west (encircled.)99ivo://helio-informatics.org/FE171_halocme_20130320_053410McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=065706582013-03-19T23:30:352013-03-20T01:30:35-453-4252.0QS?C?S?RNNNNN-N-[-784,-121,-757,-94][654,1933,979,1698]BBSmall-scale filament eruption apparently not escaping from the Sun Nariaki NittaThis example may give a disk view of an unsuccessful eruption. The eruption appears to hit the adjacent and overlying structures, but there is no appreciable heating, judging from the lack of signatures in 94 A images.99ivo://helio-informatics.org/FE171_halocme_20130320_060000McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=065806592013-03-21T02:40:112013-03-21T03:49:47806-2231.5QSC?S?NNNNN-N-[697,916,-453,7][2176,4095,1137,2216]Sneaky filament eruption Nariaki NittaiiThis is a diffuse filament eruption seen only in 304 A channel without visible effects in other channels.99ivo://helio-informatics.org/FE304_halocme_20130322_071420McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=065906602013-03-24T16:08:032013-03-24T23:48:03-387-672.0QSF?SRNNYNN-0473JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/03/CME0091/CME.html[-656,-119,-314,180][763,2042,1577,2296]QS filament eruptionKarel SchrijverQuiet-Sun filament eruption, with ribbons and post-eruption arcade, including coronal changes towards the north at the edge of what appears to be a small coronal hole.@@ivo://helio-informatics.org/FE171_KarelSchrijver_20130325_203840McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=066006612013-03-26T06:00:032013-03-26T18:00:0318-893.0ARFSRYN?Y?NB2.7|B2.5|B3.5CChttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/03/26/gev_20130326_1218/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/03/26/gev_20130326_1418/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/03/26/gev_20130326_1527/index.html0349KKhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/03/Flow0101/CME.html[-1178,1213,-762,583][86,4069,779,3018]Mini filament eruption Marc DerosaA short filament associated with a small [unnumbered] active region first activates before erupting hours later. The activation includes several spells where helical, twisting, or untwisting motions are apparent.@@ivo://helio-informatics.org/FE171_KarelSchrijver_20130330_005818McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=066106622013-03-31T20:30:032013-03-31T23:30:03-9991861.0AR?C?RNNNNN-N-[-1131,-867,114,257][0,1279,1998,2717]Pre-April's Fool Day EruptionAnna MalanushenkoThe first eruption in the sequence of April 1st eruptions. This might even be an incomplete eruption and the flux rope is small. There is, however, a substantial brightening at the loop tops in 304A.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130403_004328McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=066206632013-03-31T20:55:032013-04-01T00:30:03764-5682.0QSP?RYN?NNN-0881FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/04/CME0001/CME.html[540,987,-664,-473][2681,3960,741,1460]))Another Eruption in April's Fool SequenceAnna MalanushenkoThe only reason I'm annotating this minor eruption on the SW limb is that there are several larger scale almost contemporary eruptions in other parts of the disk and limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130403_004617McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=066306642013-03-31T21:05:032013-04-01T05:20:03-1918445.0PCPARNNYNN-0413FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/04/CME0003/CME.html[-723,340,598,1089][769,2688,2914,3993]April's fool eruption 1Anna Malanushenko??This is a partial eruption of a large filament close to the North pole. The part of it which is clse to the disk rapidly attempts to erupt, but stops on the corona and falls back to the surface. The latter is associated with flows in the rest of the filament as well as the footpoint brightening (211A, not shown here).BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130403_003734McCauleyiiMcCauley: The way that the flow appears to skip along the length of the prominence is really spectacular.::http://aia.cfa.harvard.edu/filament/index.html?search=066406652013-03-31T23:15:032013-04-01T04:50:03-445-9322.0QSPA?NRY?N?YY?N-0777FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/04/CME0002/CME.html[-648,-242,-1102,-761][667,1946,136,855]April's Fool Eruption 2Anna MalanushenkoBBA rather unremarkable small prominence eruption at the South limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130403_003906McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=066506662013-04-02T12:05:032013-04-02T13:50:03-9623982.0QSP?RY?NYNB4.5kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/04/02/gev_20130402_1317/index.htmlN-[-1095,-830,322,474][0,1279,2352,3071]Minor eruptionAnna Malanushenko&&A small rapid eruption on the SE limb.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130404_024059McCauleyvvMcCauley: Begins as a symmetric, loop-like eruption but evolves into an asymmetric eruption favoring the southern leg.::http://aia.cfa.harvard.edu/filament/index.html?search=066606672013-04-08T12:50:032013-04-08T15:00:03-3713374.0IPCS?RYN?YNB8.9kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/04/08/gev_20130408_1439/index.htmlN-[-593,-150,95,579][469,2388,2070,3149]((A three-way confined filament activation Mark CheungA filament connecting different ARs destablizes and results in a confined filament eruption. There seems to be material exchange between the magnetic concentrations that form the three corners of this triangular complex.<400 km/s. Much material falls back, lasting 6 hours after the initial eruption.88ivo://helio-informatics.org/FE304_WeiLiu_20130521_002805McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=069006912013-05-11T20:00:032013-05-12T01:20:035718274.2QSFS?RY?NYN1?-0434FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0052/CME.html[324,817,599,1054][2359,3638,3066,3785],,Large filament eruption and two-ribbon flareWei LiuttA large filament erupts near the northwest limb, drifting toward the west, producing a two-ribbon flare in its wake.88ivo://helio-informatics.org/FE304_WeiLiu_20130521_183246McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=069106922013-05-14T04:40:032013-05-14T07:50:03-996-1302.0QSC?SNRNNYDN-N-[-1162,-830,-260,-1][0,1279,1471,2190]Filament eruption near SE limbWei LiuFilament eruption near SE limb.88ivo://helio-informatics.org/FE304_WeiLiu_20130523_015500McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=069206932013-05-14T06:30:032013-05-14T11:40:03486-8963.5PCC???NNYY?N-0430FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0069/CME.html[399,573,-1017,-775][2219,3498,195,914]##Slow prominence eruption on SW limbWei LiuGGA prominence eruption lasts many hours. Most mass appears to fall back.88ivo://helio-informatics.org/FE304_WeiLiu_20130523_015802McCauleyMcCauley: There is a very minor CME detection in CACTus that is likely the result of the opening overlying field rather than any prominence material being expelled.::http://aia.cfa.harvard.edu/filament/index.html?search=06930694-----1---------------Wei LiussTwo prominence eruptions across the solar disk occur at the same time, one on the NE limb and the other on SW limb.88ivo://helio-informatics.org/FE304_WeiLiu_20130523_020217---06952013-05-14T22:24:032013-05-14T23:18:03995-2022.0IPFSNR?Y?NNNN-0618FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0077/CME.html[833,1158,-411,6][2816,4095,1351,2070] loop + prominence eruption, CME?Wei LiuA loop shaped prominence eruption, preceded by another faint loop shaped eruption (possibly a CME front) best seen at 211 and 171. The prominence is likely the core of the CME, as in a classic three-part CME scenario.88ivo://helio-informatics.org/FE211_WeiLiu_20130523_020848McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=069506962013-05-15T01:40:032013-05-15T16:40:03694-7462.5PCC?ARYNYY?N-N-[482,906,-984,-508][2176,4095,265,1344]Two prominence eruptionsWei Liu~~Two prominence eruptions one after another from the southwest limb. The second eruption has most of its material falling back.88ivo://helio-informatics.org/FE304_WeiLiu_20130523_231323McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=069606972013-05-15T06:10:032013-05-15T07:50:03652-3513.0IPP?S?R?Y?NNNN-0408GGhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/Flow0077/CME.html[424,880,-545,-157][2495,3774,1104,1823]FIlament eruption and flareWei Liu))A filament eruption causes flare ribbons.88ivo://helio-informatics.org/FE211_WeiLiu_20130523_230626McCauleyMcCauley: The CACTus catalog didn't register this event, but the movie listed (from a different event) seems to show some signature. There are two (sympathetic or directly connected?) eruptions that occur simultaneously on either side of the active region.::http://aia.cfa.harvard.edu/filament/index.html?search=069706982013-05-16T04:50:032013-05-16T06:00:03-932-4071.0QS?FSRNNNNN-0171FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0085/CME.html[-1177,-686,-623,-191][0,1279,1010,1729]Loop + prominence eruptionWei LiuA loop-shaped prominence eruption on the southeast limb. The prominence (red, 304) is preceded by another loop-shaped emission seen at 171 (yellow, and 211, not shown).88ivo://helio-informatics.org/FE171_WeiLiu_20130523_235556McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=069806992013-05-16T07:10:032013-05-16T08:10:03-9841733.0QS?FSRYNNNN-0976FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0086/CME.html[-1156,-813,6,339][0,1279,1976,2695]Prominence eruptionWei Liu%%Prominence eruption on the east limb.88ivo://helio-informatics.org/FE304_WeiLiu_20130523_234513McCauleyNNMcCauley: Possible rolling motions evidenced by twisting of the two arch legs.::http://aia.cfa.harvard.edu/filament/index.html?search=069907002013-05-18T01:04:032013-05-18T02:16:03-10031834.0QS?PSRYYNNN-0961FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0101/CME.html[-1031,-974,160,206][0,1279,1994,2713]Kink instability?Anna MalanushenkozzA relatively small filament takes off on the E limb. What is peciliar is that most of kinking seems to happen at its apex.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130521_015944McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=07000701-----1---------------Anna MalanushenkoWWA beautiful bright prominence eruption followed by a rather sophisticated coronal rain.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130521_211222---07022013-05-18T07:36:032013-05-18T16:02:03-955-3733.5AR?CSRNNNNB9.8kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/05/18/gev_20130518_0827/index.htmlN-[-1070,-841,-480,-267][0,1279,1066,1785]""Filament eruption and coronal rainAnna Malanushenko[[A beautiful prominence eruption followed by a rather sophisticated pattern of coronal rain.BBivo://helio-informatics.org/FE304_AnnaMalanushenko_20130521_020834McCauleyMcCauley: A large front of material is seen moving outward at LASCO as this event starts but there isn't a clear connection between the two: http://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0102/CME.html. Nice loop oscillations.::http://aia.cfa.harvard.edu/filament/index.html?search=070207032013-05-21T05:50:032013-05-21T08:20:032675535.0ARFA?NR?YNNNN-0414FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0124/CME.html[-2,537,224,881][1520,3467,2422,3515]Filamnet eruption and flareWei LiuHHA filament erupts near an active region and produces a two ribbon flare.88ivo://helio-informatics.org/FE304_WeiLiu_20130522_220520McCauleyMcCauley: Interesting response from a filament to the north of this eruption, which is displaced somewhat by the eruption, oscillates, but remains stable for many hours after this event.::http://aia.cfa.harvard.edu/filament/index.html?search=070307042013-05-21T09:40:032013-05-21T11:40:037203761.0ARCAS?NNNNC1.2kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/05/21/gev_20130521_1023/index.htmlN-[593,847,291,462][2609,3888,2316,3035]AR filament eruptionWei Liu[[A small active region filament erupts, lifting up, dumping most of its mass toward one end.88ivo://helio-informatics.org/FE304_WeiLiu_20130522_221016McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=070407052013-05-21T12:00:032013-05-21T23:10:038477073.5IPFARYNYDN-0400FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0125/CME.html[653,1041,445,969][2176,4095,2687,3766]Prominence eruptionWei LiuiiA prominence experiences first activation (as reported earlier) and then eruption while unwinding itself.88ivo://helio-informatics.org/FE304_WeiLiu_20130522_224517McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=070507062013-05-22T08:00:352013-05-22T18:00:35-662-7223.0QSP??NNYYN-1008FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0131/CME.html[-796,-527,-836,-608][306,1585,485,1204]Prominence eruption on SE limbWei LiuBBA prominence erupts on SE limb, but most material falls back down.88ivo://helio-informatics.org/FE304_WeiLiu_20130522_231922McCauleyMcCauley: CME refers to an eruption that originates in the NW, but there may be a signature from this event in the movie as well.::http://aia.cfa.harvard.edu/filament/index.html?search=070607072013-05-23T09:50:232013-05-23T11:00:23-1071-962.0AR?P?A?RNNNNN-0758FFhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/2013/05/CME0145/CME.html[-1215,-928,-192,1][0,1279,1529,2248]Eruption of a heated filament Nariaki NittaThis looks like a surge or spray, but it may be part of a filament eruption. The eruption appears bright in 304A, 211A and 171A, suggesting that the material gets heated up as it erupts. The 211A corona responds to the eruption.99ivo://helio-informatics.org/FE171_halocme_20130607_012638McCauley<>ivo://helio-informatics.org/FE171_PaulAHiggins_20130723_170518---07492013-07-21T20:50:032013-07-21T22:25:0373110083.0PCFSNRNNNDN-0244JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/07/CME0054/CME.html[-117,1578,538,1478][1270,4095,2508,4095]++Behind-the-limb Northward Filament Lift-off Paul HigginsA possible polar-crown filament lift off at a near-perfect north-ward trajectory. The event likely occurred well beyond the West limb at >45deg latitude. There does not appear to be any pole-ward deflection, but this may be a LOS effect. There appears to be a large cavity-like structure in the coronal region where the eruption took place. This may have allowed the eruption to exhibit the uncommon trajectory.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130723_165041McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=074907502013-07-24T04:30:032013-07-24T13:10:039472253.0QSCARNNYYN-N-[864,1031,143,307][2816,4095,2064,2783]A failed prominence eruption Paul HigginsA filament partially erupts at the S-E limb. Most of the material falls back southward, and some northward, outlining the overarching magnetic field structure.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130726_180759McCauley99McCauley: Movie FOV is off, should be looking at SE Limb.::http://aia.cfa.harvard.edu/filament/index.html?search=075007512013-07-24T22:00:032013-07-26T00:10:034679625.0PCFA?RYNYYN-0380JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/07/CME0061/CME.html[238,697,700,1224][1868,3787,3016,4095];;Helical Prominence Eruption and subsequent cavity formation Paul HigginsA prominence erupts at the north-west limb. It appears to consist of two segments oriented radially to the limb, that twist about eachother in a helical pattern- like a DNA strand. The two strands twist more tightly about each other as the eruption continues. There appears to be a pinched region where the axis of the helix was by the end of the eruption. A coronal cavity or dimming region forms slowly to the west of the eruption afterward.>>ivo://helio-informatics.org/FE304_PaulAHiggins_20130726_195354McCauley''McCauley: The 171 movie is spectacular.::http://aia.cfa.harvard.edu/filament/index.html?search=075107522013-07-29T22:10:032013-07-30T00:35:0310612053.0?PS?RYYNNN-1041JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/07/CME0077/CME.html[903,1218,94,316][2816,4095,2030,2749]Kink instability leads to CME? Paul HigginsVVA prominence appears to become kink-unstable. This leads to a rapid outward motion and then dissappearance of the prominence. The coronal loop structure surrounding the promenence dissappears as well, and a radial coronal cavity forms, with radial streamer-like structures moving north and south, away from the prominence's original position.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130730_225616McCauleyBBMcCauley: Remarkably fast CME for such a seemingly minor eruption.::http://aia.cfa.harvard.edu/filament/index.html?search=075207532013-07-31T17:06:032013-08-01T00:00:03-816-5082.0IP?P?A?RNNYD?N-0434JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/07/CME0081/CME.html[-1139,-492,-708,-309][49,1328,841,1560]Faint eruptionAnna Malanushenko A faint eruption on the SE limb.>>ivo://helio-informatics.org/FE304_PaulAHiggins_20130813_234704McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=075307542013-08-02T12:18:032013-08-02T15:38:03391-4494.0QSF?RYY?YNB5.0kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/02/gev_20130802_1448/index.html0529JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0004/CME.html[205,577,-560,-337][2060,3339,941,1660]Filament eruptionAnna MalanushenkojjA filament erupts on the SW disk. Its northern end has a nice "swirl" shape. Post-eruption arcade follows.>>ivo://helio-informatics.org/FE304_PaulAHiggins_20130814_003414McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=075407552013-08-03T02:00:352013-08-03T12:00:354739863.0PCPA?NRYNNN?N-0136KKhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/Flow0001/CME.html[72,873,755,1218][1876,3795,3016,4095]Slow prominence eruption Nariaki NittaAlthough the origin of this activity is TBD, it may reperesent at least part of the diffuse, slow and long-lasting outflow (and yet containing a flux-rope-like feature) in LASCO data. The prominence can be tracked in AIA data roughly between 03 UT and 08 UT, most notably in 171 A.99ivo://helio-informatics.org/FE171_halocme_20130805_175351McCauley77McCauley: Twisted structure apparent in the 171 images.::http://aia.cfa.harvard.edu/filament/index.html?search=075507562013-08-04T06:15:352013-08-04T07:45:35-7133363.0QS?C?SRNNNNN-0367JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0006/CME.html[-873,-553,179,492][220,1499,2248,2967]Apparent confined eruption Nariaki NittaThis may look like a failed eruption. The filament does not appear to escape. However, a CME is observed by LASCO, not very impressive but not too wimpy either. Difference images in 211 A /193 A indicate some minor dimming.99ivo://helio-informatics.org/FE171_halocme_20130806_181411McCauleyMcCauley: The response from higher in the corona is apparent in the 171 radial filter images. The eruption looks completely confined in the 304/193 images, so it is not clear if the CME material came from the filament structure or somewhere higher in the corona from these observations.::http://aia.cfa.harvard.edu/filament/index.html?search=075607572013-08-04T14:30:352013-08-04T16:00:35731-3693.0IPPA?SY?NNNN-0488JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0008/CME.html[494,968,-576,-161][2627,3906,1074,1793]Minor eruption Nariaki NittaAlthough the eruption itself is minor, it produces a ribbon-like emission at footpoints. Besides the eruption, the filament mateiral is seen to escape sideway to north. The associated small CME in LASCO data shows closed loops following a spiky structure.99ivo://helio-informatics.org/FE171_halocme_20130806_202359McCauleyMcCauley: Note the interesting, rapid twisting motions (or the illusion of them, it's not clear to me) that occur at low heights between the southerly and northerly components of the eruption.::http://aia.cfa.harvard.edu/filament/index.html?search=075707582013-08-05T01:10:112013-08-05T03:50:11379-8921.0PCPARNNNNN-N-[214,544,-1061,-724][2040,3319,201,920]Minor prominence eruption Nariaki NittaThis erption appears to originate on the viisble side because we can identify both legs. The prominence is in the same line of sight as the cavity seen in 211 A images, but they seem to be not related. The eruption is so minor that there are no coronagraphic consequences.99ivo://helio-informatics.org/FE171_halocme_20130806_210413McCauleyMcCauley: The 171 radial filter images show a very faint structure extending much farther north than is apparent in the 304 images. The cavity is associated with a background filament that does not appear to be connected to this one.::http://aia.cfa.harvard.edu/filament/index.html?search=075807592013-08-05T13:50:232013-08-05T15:20:239323361.0?C?RN?N?NNN-N-[839,1025,254,418][2816,4095,2249,2968]Failed eruption Nariaki Nitta,,The prominence eruption is probably from the back side. It clearly fails to break into interplanetary space (no CME), which is partly understood by noticing that there is no dimming in the background structure. Unlike other well-known examples, this eruption is not reminiscent of kink instability.99ivo://helio-informatics.org/FEMET_halocme_20130806_212102McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=075907602013-08-06T01:12:032013-08-06T02:20:03923-3164.5IPPA?NRYN?YNN-0387JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0009/CME.html[668,1177,-492,-140][2816,4095,1162,1881]Filament eruptionKarel Schrijver44Filament eruption from moderate AR near the SW limb.@@ivo://helio-informatics.org/FEMET_KarelSchrijver_20130807_220439McCauleyMcCauley: Another filament erupts nearly simultaneously father south and both contribue to the Type II halo CME detection in the CACTus catalog. There are very interesting twisting motions (possibly roll) evident in the northern leg. The eruption begins in a fairly standard loop-like fashion. As the loop collapses, the northern leg appears to twist and part of the downfalling material is accelerated outward again along a seemingly new connectivity to the north.::http://aia.cfa.harvard.edu/filament/index.html?search=076007612013-08-06T01:16:032013-08-06T05:24:03-6453832.0QSFSRYNNNB4.5kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/06/gev_20130806_0142/index.html0527JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0010/CME.html[-1073,-216,-21,786][14,1933,2146,3225]Filament eruptionKarel SchrijverUUQS filament eruption with distant, over-the-limb coronal oscillations towards the NE.@@ivo://helio-informatics.org/FE171_KarelSchrijver_20130807_220025McCauley@@McCauley: Apparent untwisting in the southern leg post-eruption.::http://aia.cfa.harvard.edu/filament/index.html?search=076107622013-08-06T05:28:032013-08-06T09:12:03-975-5483.0IP?P??RYY?NNB6.0kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/06/gev_20130806_0633/index.html0340JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0013/CME.html[-1207,-744,-858,-238][0,1919,595,1674]Limb-filament eruptionKarel SchrijverffFilament eruption from just over the SE limb, with some oscillatory motions in the surrounding corona.@@ivo://helio-informatics.org/FE171_KarelSchrijver_20130807_220305McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=076207632013-08-07T11:28:032013-08-07T23:48:03270-5243.5ARPAS?N?NNN B5.3|B6.3http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/07/gev_20130807_1712/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/07/gev_20130807_1713/index.html0294JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0025/CME.html[-7,548,-796,-253][1859,3138,814,1533]Moderate-AR filament eruptionKarel SchrijverA moderate-AR filament erupts from the southern hemisphere, creating a beautifully shaped, strongly sheared, sigmoid post-eruption arcade with a transient CH at the ends. Potentially related to nearby emergence of a small bipole towards the NE.@@ivo://helio-informatics.org/FE171_KarelSchrijver_20130809_005009McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=076307642013-08-10T06:48:032013-08-10T12:28:03681-4543.5ARPAR?YNNNB4.3kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/10/gev_20130810_0844/index.html0325JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0036/CME.html[461,901,-589,-319][2544,3823,932,1651]$$Filament eruption followed by cavityRtimmons__Eruption of a filament on the SW disk, followed by a cavity developed around the eruption site.>>ivo://helio-informatics.org/FEMET_PaulAHiggins_20130814_013733McCauleyMcCauley: Beautiful sigmoid eruption from AR 11810 with some interesting twisted flows visible in the later, eastern part of the event. There's also a nice EUV wave visible in the 193 images.::http://aia.cfa.harvard.edu/filament/index.html?search=076407652013-08-12T19:40:112013-08-12T21:10:11-289-7142.0QSP?SSY?NNNN-N-[-425,-154,-902,-526][926,2205,499,1218]Minor filament eruption Nariaki NittaThe filament looks like a linear structure in 211 A images before eruption. It becomes an arc as it erupts, seen only in 304 A images, with brightening at the footprints. The surrounding structures, especially those in the west, are pushed sideways.99ivo://helio-informatics.org/FE304_halocme_20130815_184523McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=076507662013-08-14T05:00:032013-08-14T08:00:03648-8081.0QSPS?RNNNYN-N-[458,838,-920,-697][2489,3768,341,1060]MInor prominence eruption Nariaki NittaFollowing gradual outword motions, the small prominence seems to erupt. But is has negligible effect on the surrounding corona, and no CME is observed by LASCO.99ivo://helio-informatics.org/FE304_halocme_20130815_233345McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=076607672013-08-14T18:30:352013-08-14T23:30:35665-5353.0QSP?SRYNYN C1.0|C1.6http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/14/gev_20130814_1900/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/14/gev_20130814_2249/index.html0263JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0053/CME.html[133,1197,-814,-255][2176,4095,618,1697]++Eruption of a filament with fine structures Nariaki NittaThe presence of the filament is noted in all of the 304, 211 and 171 A channels. Eruption of such a filament indeed results in a decent three-part CME in LASCO data.99ivo://helio-informatics.org/FE171_halocme_20130816_002025McCauleyaaMcCauley: Apparent untwisting in legs after eruption. Apparent untwisting in legs after eruption.::http://aia.cfa.harvard.edu/filament/index.html?search=076707682013-08-16T18:00:032013-08-17T06:00:03-6644663.0QSFSRYNYNN-0279JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0068/CME.html[-1212,-116,-123,1054][0,3487,1843,3804]Faint filament forges forth Marc DerosaccA faint, U-shaped filament located in the northeast quadrant of the solar disk decides to lift off.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130822_173253McCauleyffMcCauley: Apparent untwisting motions in the legs after the eruption, particularly in the eastern one.::http://aia.cfa.harvard.edu/filament/index.html?search=076807692013-08-17T10:00:032013-08-17T19:00:03-8844263.0QS?P?NR?YNYDC1.8kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/17/gev_20130817_1327/index.html0249JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0070/CME.html[-1221,-547,1,852][0,2519,2051,3466]44Prominence eruption on limb excites an active regionRtimmonsProminence on northeast limb lifts off, and affects an active region in its surrounding environment, causing significant loop brightenings.>>ivo://helio-informatics.org/FEMET_PaulAHiggins_20130822_173852McCauleyMcCauley: The cavity is not very apparent prior to the eruption due to other structures along the line-of-sight, but it can be seen erupting in a non-radial direction as the prominence lifts off.::http://aia.cfa.harvard.edu/filament/index.html?search=076907702013-08-17T16:00:032013-08-18T00:00:03689-5614.0ARFSRYYNNN-0726JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0071/CME.html[163,1215,-1227,106][146,4095,4,2223]((Flare/Filament Eruption/CME from AR11818 Marc DerosaAn M3 flare occurs in AR11818, a filament lifts off, post-flare loops appear, and much of the region between AR11818 and 11819 is evacuated and becomes dark. This flare is associated with a CME that can be seen in, e.g., LASCO coronagraph images.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130822_174710McCauleyMcCauley: Sigmoidal active region and clear kinking in the filament eruption. Hinode/XRT observations can be found here: http://xrt.cfa.harvard.edu/xpow/20130904.html::http://aia.cfa.harvard.edu/filament/index.html?search=077007712013-08-18T13:40:032013-08-18T16:52:03926-4602.5ARP?SRY?Y?NNN-0422JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0082/CME.html[695,1156,-632,-287][2816,4095,923,1642]//Filament eruption with high-coronal disturbanceKarel Schrijver__Filament eruption for a region nearing the SW limb, associated with a high coronal disturbance.@@ivo://helio-informatics.org/FE193_KarelSchrijver_20130819_173225McCauleyMcCauley: The filament appears to kink (though not so obviously) before much of the dark material visible in 193 collapse and some of the bright material visible in 304 sprays outward.::http://aia.cfa.harvard.edu/filament/index.html?search=077107722013-08-18T19:44:032013-08-18T22:36:03809-5182.0IPPSRYNND?N-0431JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0083/CME.html[428,1191,-755,-281][2758,4037,825,1544]Eruption complexKarel SchrijverA high coronal - over the W limb - eruption is followed by the eruption of an adjacent filament (with a propagating front) and the beginnings of a filament activation trailing into QS.@@ivo://helio-informatics.org/FE193_KarelSchrijver_20130819_173749McCauley99McCauley: Apparent untwisting motions in the eastern leg.::http://aia.cfa.harvard.edu/filament/index.html?search=077207732013-08-20T03:44:032013-08-20T12:44:03333-6574.0QSFSRNNYN C1.3|C1.1http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/20/gev_20130820_0454/index.html|http://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/20/gev_20130820_0458/index.html0541JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0091/CME.html[-551,1217,-1189,-125][1131,4076,126,1781]//Limb eruption and polar-crown filament eruptionKarel SchrijverAn AR at the W limb erupts (with some oscillatory motions high in the corona), upon which a long quiet-Sun (near polar-crown) filament erupts on the S hemisphere. The timing is suggestive of a sympathetic set of events, but direct evidence is not obvious.@@ivo://helio-informatics.org/FE211_KarelSchrijver_20130820_182601McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=077307742013-08-21T00:16:032013-08-21T03:20:039023213.0QSP?SRY?Y?YNB7.7kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2013/08/21/gev_20130821_0204/index.htmlN-[571,1233,216,427][2816,4095,2224,2943]Filament/cavity eruptionAnna Malanushenko~~A thin filament erupts on the W disk/limb. As it reaches to certain height, an associated erupting cavity can also be visible.>>ivo://helio-informatics.org/FE211_PaulAHiggins_20130827_234951McCauleyMcCauley: There is a hint of kinking at the apex of the erupting filament, but the projection makes it difficult to be more confident in that.::http://aia.cfa.harvard.edu/filament/index.html?search=077407752013-08-27T06:45:032013-08-27T21:35:031001-1353.0AR?FSRYNYNN-0538JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0116/CME.html[682,1321,-374,104][2816,4095,1464,2183]22filament loop reconfiguration followed by eruption Paul HigginsFilament material off the West limb rapidly reconfigures and appears to flow downward toward the surface. This is followed by a large rapid, radially directed eruption of filament material.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130829_181217McCauleyMcCauley: Interesting twisting motions in the 193 images before the first filament collapses. Note the very faint vertical threads at large heights over the limb at the beginning of the 193 movie. That structure appears to be destabilized by the eruption below, but it's not clear if the two structures are related (in roughly the same plane) or not. Either way, it's unusual to see such threads.::http://aia.cfa.harvard.edu/filament/index.html?search=077507762013-08-28T00:00:032013-08-28T14:00:034459984.0PCP?RNNYYN-0208KKhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/Flow0041/CME.html[247,642,776,1219][1829,3748,3016,4095]Squid-like prominence lift-off Paul HigginsA graceful prominence lift-off. On the previous day, the prominence exhibited a change in loop configuration ( SOL2013-08-27T02:40:03L138C026 ). This may have destabilised the prominence which has slowly lifted off, leaving a radial evacuated region in its wake. The top of the eruption appears to be threaded by U-loops, whiich become transversally compressed into V loops. A strange trail of prominence material follows the main structure like the tentacles of a squid as the creature swims away.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130829_183329McCauleyMcCauley: The cavity is at a very high altitude at the start of these observations but is a bit lower and more prominent in the 193 images a day earlier.::http://aia.cfa.harvard.edu/filament/index.html?search=077607772013-08-28T12:25:032013-08-28T21:10:031028-1542.0QS?FSRNNYNN-0212JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0127/CME.html[782,1273,-417,110][2176,4095,1253,2332]Slow filament eruption Paul HigginsA large arc of filament material slowly lifts off from the W limb. The eruption appears diffuse, as there was not much visible filament material on the surface to begin with. Could this be related to the 'phantom CME'?>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130829_184304McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=077707782013-08-28T13:20:032013-08-28T17:20:03-812-8482.0QSFSRYNNNN-0466JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0124/CME.html[-1200,-424,-1223,-473][0,1919,95,1174]$$Behind the SE-limb filament eruption Paul Higgins[[A faint eruption of filament material is observed to propagate radially off of the SE limb.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130829_184756McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=077807792013-08-29T00:00:032013-08-29T10:00:03285-7694.0QSFSRY?NYNN-0440JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0132/CME.html[-446,1017,-1273,-265][1305,3742,82,1451]&&Massive slow on-disk filament eruption Paul HigginsA long filament spanning >45 degrees in the southern henisphere slowly erupts. Afterward, a dim front of reconnecting field expands from the filament channel, similar in morphology to a flare ribbon.>>ivo://helio-informatics.org/FE211_PaulAHiggins_20130829_191020McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=077907802013-08-30T13:05:032013-08-31T04:00:03-563-9314.0PCF?ARNNNYN-0107KKhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/Flow0053/CME.html[-1053,-73,-1185,-677][150,2069,0,1079]Filament+V-loop lift-off Paul HigginsA prominence becomes unstable and appears to be partially siphoned up into a coronal V-loop structure which also lifts off along radial streamer-like structures visible in 171A and 211A.>>ivo://helio-informatics.org/FE211_PaulAHiggins_20130903_173128McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=078007812013-08-31T00:00:032013-08-31T19:20:037917474.5QSCAR?N?NYNN-N-[528,1055,508,985][2728,4007,2933,3652]//horizontal coronal structures+filament eruption Paul Higgins::A radial oriented prominence appears suspended by horizontal loop structures that kinks into a V-shape at the location of the intersection (possibly pulled down by the weight of the prominence material like a slingshot). A connected filament then lifts off and is siphoned into the region of horizontal structures.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130903_175657McCauley&&McCauley: See 171 radial filter movie.::http://aia.cfa.harvard.edu/filament/index.html?search=078107822013-08-31T17:20:032013-09-01T08:30:03-885-5245.0QSP??Y?N?YNN-0281JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/08/CME0155/CME.html[-1159,-610,-771,-276][0,1279,816,1535]Filament lift-off trapped Paul HigginsA filament in the S-W quadrant partially erupts and some of the material is trapped and suspanded abover the region, and then siphoned back down to the surface away from the eruption site along other over-arching loops>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130903_174312McCauleyMcCauley: There's an eruption behind the limb at the start of this event that can be seen in the STEREO movie (and somewhat in the AIA/171 movie).::http://aia.cfa.harvard.edu/filament/index.html?search=078207832013-09-01T19:45:032013-09-02T06:30:03-386-7872.0QSFSRYNYNN-0219JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/09/CME0001/CME.html[-750,-23,-1215,-358][135,2672,25,1450]Faint filament eruption Paul Higgins``Avery faint filament erupts rapidly off the south limb, and shows no apparent coronal signature.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130903_180604McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=078307842013-09-02T05:40:032013-09-02T13:40:03-6338491.0QSCSNRNNNNN-N-[-838,-428,621,1076][34,1953,2923,4002]Failed filament eruption Paul HigginsProminence material becomes unstable and partially erupts. As it does, it becomes trapped on open field lines and appears to flow back to the surface.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130903_181304McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=078407852013-09-04T20:00:032013-09-05T00:00:03-818-3083.0ARPA?YYNNN-0538JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/09/CME0010/CME.html[-1221,-415,-629,12][0,1919,994,2073]Nice filament eruption on limb Marc DerosaFilament from an off-limb active region shows a lot of dynamics involving both colder filament material and warmer coronal loop structures.>>ivo://helio-informatics.org/FE171_PaulAHiggins_20130911_173219McCauleyppMcCauley: Filament seen in 304 appears to collapse but overlying field just to the south exhibits lightbulb CME.::http://aia.cfa.harvard.edu/filament/index.html?search=078507862013-09-05T09:50:032013-09-05T14:32:034849862.0PCP?ANRNNNY?N-0203JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/09/CME0014/CME.html[323,645,808,1163][2215,3494,3331,4050]A lazy eruptionAnna Malanushenko;;A northward eruption with a very slow onset at the NW limb.>>ivo://helio-informatics.org/FE304_PaulAHiggins_20130908_032657McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=078607872013-09-10T10:44:032013-09-10T17:16:03-614-7602.0QSFS?R?ANYYN-0505JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/09/CME0040/CME.html[-935,-293,-1083,-437][65,1984,242,1321]Filament eruptionKarel Schrijver##QS (polar crown?) filament eruption@@ivo://helio-informatics.org/FE171_KarelSchrijver_20130923_154014McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=078707882013-09-11T02:30:352013-09-11T03:30:35-6614242.0QSONANAYNNNN-N-[-805,-517,247,600][307,1586,2394,3113]Minor eruption Nariaki NittaThe eruption involves motions that look like counter-clockwise. Loops to the north are affected by the eruption, leaving temporary dimming notably in 193 A images. No CME is observed by LASCO.99ivo://helio-informatics.org/FE171_halocme_20130914_230553McCauley;;McCauley: No obvious outward eruption. Filament activation.::http://aia.cfa.harvard.edu/filament/index.html?search=078807892013-09-11T08:00:032013-09-11T10:00:03-807-8144.0QSFSRNNYYN-0428JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/09/CME0045/CME.html[-1105,-509,-1210,-417][0,2349,33,1352]((Prominence eruption with some untwisting Nariaki NittaThe untwisting is more readily seen in the southern leg. There is clear connection of the northern leg with the filement (channel) on the visible side. The eruption drives a decent CME that is first seen by LASCO C2 at 09:24 UT and traceable to the edge og C3 (around 19 UT).99ivo://helio-informatics.org/FE171_halocme_20130913_165700McCauleyQQMcCauley: Very similar to ID 0791 two days later. Large PCTR area visible in 171.::http://aia.cfa.harvard.edu/filament/index.html?search=078907902013-09-13T14:00:032013-09-13T21:00:03-45-9704.0PCPA?S???YYN-0209JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/09/CME0050/CME.html[-586,495,-1223,-718][1013,2932,0,1079]''Slow eruption from a south polar region Nariaki Nitta==The slow ascent of the prominence had started before 14 UT. It is hard to link this eruption with the filaments lying on the visible disk. The associated CME, which was first found around 19 UT in LASCO C2 data, was quite major in the sense that it was still visible at the southern or souteastern limit of C3 data.99ivo://helio-informatics.org/FE171_halocme_20130914_163949McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=079007912013-09-14T00:10:032013-09-14T05:20:03-909-7714.0QSFSRNNYYN-0250JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2013/09/CME0051/CME.html[-1216,-603,-1190,-352][0,2480,67,1460]Quiescent filament eruption Mark Cheung44Quiescent filament eruption from the southeast limb.<>Prominence eruption possibly deflected by overlying structures Nariaki Nitta}}As the prominence erupts, it appears to deflect southward. The prominence itself seems to have complex internal structures.99ivo://helio-informatics.org/FE211_halocme_20140109_083810McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=085208532014-01-01T08:12:032014-01-01T16:32:03-763-6665.0QS?FA?RY?NYYN-0286JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2014/01/CME0003/CME.html[-1145,-381,-1085,-247][0,2480,242,1635]Prominence eruptionRtimmons%%Prominence eruption over the SE limb.@@ivo://helio-informatics.org/FEMET_KarelSchrijver_20140102_210745McCauleyTTMcCauley: Stunning example of the prominence-corona transition region (PCTR) in 171.::http://aia.cfa.harvard.edu/filament/index.html?search=085308542014-01-01T18:00:032014-01-02T04:16:03-419-6363.0QSF?SRNNYNN-0229JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2014/01/CME0007/CME.html[-699,-138,-980,-292][333,2369,417,1560]Filament eruptionRtimmonsQS filament eruption@@ivo://helio-informatics.org/FE171_KarelSchrijver_20140102_211017McCauleyMcCauley: Interesting activity below the filament and a very unsteady rise with pauses that had me thinking the filament would collapse.::http://aia.cfa.harvard.edu/filament/index.html?search=085408552014-01-01T18:20:232014-01-01T19:40:47756-3154.0ARPSRN?N?NNM9.9kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2014/01/01/gev_20140101_1840/index.html0281JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2014/01/CME0005/CME.html[476,1036,-539,-90][2669,3948,1164,1883]First major flare in 2014 Nariaki NittaThis flare is quite similar to the last major (M6.4) flare in 2013 from the same region (AR 11936). Although the way the filament erupted was spectacular because they looked fragmented, it was almost a failed eruption. Most of the stuff came back. The associated CMEs were wimpy at best. The CME associated with the M9.9 flare was a little more decent than that with the M6.4 flare partly because of its location closer to the limb and possibly larger energy released.99ivo://helio-informatics.org/FEMET_halocme_20140102_202527McCauleyWWMcCauley: Looks a junior version of the famous June 2011 event (#0234 in this catalog).::http://aia.cfa.harvard.edu/filament/index.html?search=08550856-----1---------------RtimmonsAn M9 flare from a region in the SW quadrant associated with a filament eruption, with much (most?) of the material falling back onto the surface.@@ivo://helio-informatics.org/FE171_KarelSchrijver_20140102_210415---08572014-01-02T03:32:032014-01-02T12:04:03376-6762.0QSPANR?YNYDN-0147KKhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2014/01/Flow0006/CME.html[27,725,-915,-436][2035,3314,563,1282]QS filament eruptionRtimmonsQuiet-Sun filament eruption with post-eruption arcade. The filament connects to, and largely falls back to, near to what appears to be the S polar cap boundary. No CME is suggested from AIA observations@@ivo://helio-informatics.org/FEMET_KarelSchrijver_20140103_164948McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=085708582014-01-02T09:04:032014-01-02T11:32:0358863.0QSC?ANRYYYNN-N?-[-20,1197,-317,328][2015,4042,1488,2627]Sympathetic (?) eventsRtimmonsA near-equatorial QS filament erupts from near the W limb. Synchronously, an AR filament near DC activates, as does a filament SE of the primary eruption. A fragment of a prominence to the S of the eruption exhibits briefly oscillations.@@ivo://helio-informatics.org/FE193_KarelSchrijver_20140103_165435McCauleyZZMcCauley: There looks to be some associated material that made it to LASCO/C2, but it wasn't enough to register as an event in the CACTus catalog. Here's a nearby event: http://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2014/01/Flow0007/CME.html. Most of the material seems to get caught up in the overlying field and flow back down to the north.::http://aia.cfa.harvard.edu/filament/index.html?search=085808592014-01-03T00:40:032014-01-03T04:52:03-9193994.0IP?P?SRYYY?DN-0625JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2014/01/CME0013/CME.html[-1132,-707,139,658][0,1919,2173,3252]Prominence eruptionRtimmonsProminence eruption@@ivo://helio-informatics.org/FE171_KarelSchrijver_20140107_001129McCauleyMcCauley: There's interesting activity in the northern part of the prominence before the main eruption, where a small parcel of material escapes out along open field near what looks like a fan-spine null point configuration. This material produces a very robust signal at LASCO, though there's a data gap for most of the main CME afterward. Much of the material in the main eruption appears to drain back down.::http://aia.cfa.harvard.edu/filament/index.html?search=085908602014-01-03T15:24:032014-01-03T19:08:03-375-6343.0QSFSR??NNN-0204JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2014/01/CME0014/CME.html[-527,-223,-919,-349][464,2383,452,1531]QS filament eruptionRtimmonsQS filament eruption@@ivo://helio-informatics.org/FE193_KarelSchrijver_20140107_001019McCauleywwMcCauley: There are some interesting oscillations near the transient coronal hole after the eruption, best seen in 193.::http://aia.cfa.harvard.edu/filament/index.html?search=086008612014-01-05T02:20:032014-01-05T02:50:03-992-225.0IP?F??SN?N?NNC4.5kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2014/01/05/gev_20140105_0224/index.htmlY-[-1207,-777,-138,94][0,1279,1652,2371]"Reflecting" filament eruption Mark CheungThe filamentary material ejected from this eruption seems to experience an abrupt change in flow direction, as if it were reflecting off a stiff barrier in the mid-corona.< 100 MeV (thanks, Sam, for reporting this.)99ivo://helio-informatics.org/FE211_halocme_20140106_153743McCauleyKKMcCauley: Strong SEP event obviated by the particle hits in the LASCO data.::http://aia.cfa.harvard.edu/filament/index.html?search=086308642014-01-13T04:30:032014-01-13T06:50:03-9452491.5QSC?SRY?NNNN-Y-[-1222,-668,10,487][0,1279,2103,2822]&&Another of multiple filament eruptions Mark CheungThis off-limb filament lifts off at around the same time as the on-disk filament. Thereafter, another filament in the northwestern limb lifts off.<>McCauley: One of the nicest untwisting examples in the catalog::http://aia.cfa.harvard.edu/filament/index.html?search=094409452014-05-03T07:30:032014-05-03T08:40:03-8562252.0ARCSRNNNNN-N-[-906,-807,182,268][0,1279,2064,2783]mini filament eruptionWei LiuiiA loop-shaped mini filament erupted and caused some brightening, but most of its material fell back down.88ivo://helio-informatics.org/FE304_WeiLiu_20140504_230703McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=094509462014-05-04T14:16:032014-05-04T22:24:0310253885.0QSP?RYYYD?N-0276JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2014/05/CME0030/CME.html[852,1197,166,609][2176,4095,2154,3233]Prominence eruptionRtimmons%%Prominence eruption over the NW limb.@@ivo://helio-informatics.org/FE171_KarelSchrijver_20140505_222315McCauleyMcCauley: Very interesting twisted structure in this event. It appears that the upper part of the prominence breaks off from the lower and expands upward, untwisting, while the lower part kinks and collapses. This is best seen 171. It's not clear to me whether the two segments of the original structure are largely just the opposite legs or if some new connectivity is formed during the eruption.::http://aia.cfa.harvard.edu/filament/index.html?search=094609472014-05-05T14:00:032014-05-05T15:24:0310511374.0QSPSR?YY?Y?NN-0332JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2014/05/CME0034/CME.html[902,1199,4,269][2816,4095,1916,2635]Over-the-limb eruptionRtimmonsOver-the-limb eruption@@ivo://helio-informatics.org/FE171_KarelSchrijver_20140506_214400McCauley-::http://aia.cfa.harvard.edu/filament/index.html?search=094709482014-05-07T12:00:032014-05-07T19:00:03942-2863.0QSP?S?RY?Y?NNM1.2kkhttp://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2014/05/07/gev_20140507_1607/index.html0678JJhttp://sidc.oma.be/cactus/catalog/LASCO/2_5_0/qkl/2014/05/CME0044/CME.html[674,1211,-616,44][2141,4095,1023,2120] Active filaments and prominencesRtimmonsFilament activation within a filament located near the west limb, followed by a limb-obscured flare that is associated with a filament eruption<>AIA_FOV = [x1,x2,y1,y2] Catalog movie box coordinates (pixels)HEK_Title = HEK event titleHEK_Observer = HEK observer))HEK_Comments = Comments from HEK_Observer((HEK_Link = IVO ID link for the HEK event''Cat_Observer = Primary catalog observer00Cat_Comments = Comments from catalog observer(s) Cat_Link = URL for catalog entry