1 - !! Outstanding chains: e1 (!!!); e2 (?), e3(?) 2 - ! A clear loop NE CME at ~20 UT !!! Outstanding chains: e1 (!!!); e2 (!!!), e3(?)!!! 3 - !!! Outstanding chains: e1 (!!!); e2 (!!!), e3(?)!!! 4 - !! Interesting chains: e1 (one image) 5 - !!Interesting and then outstanding chains: e1 (!!); e2 (?), e3(?)!! 6 - !! A large loop NE CME at 11:30 UT and then a spectacular N CME with a bright prominence !! !!! Outstanding chains: e1 (!!!); e2 (!!!), e3(?)!!! !!! Good coinciding with TRACE_1,2 at 0345 UT. ILLUSTRATION !!! Automatic analysis of double coronal mass ejections from coronagraph images Matthew Jacobs, Lin-Ching Chang, Antti Pulkkinen, Space Weather Volume 13, Issue 11 November 2015 Pages 761–777 7 - ! A large loop W CME at ~20 UT !! Outstanding/interesting chains: e1 (!!); e2 (?), e3(?)!! 7-8 Formation of Two Homologous Transequatorial Loops Jie Chen, Alexei A. Pevtsov, Jiangtao Su, Robertus Erdelyi, Yuanyong Deng, Shangbin Yang & Yongliang Song Solar Physics volume 295, Article number: 59 (2020) https://link.springer.com/content/pdf/10.1007/s11207-020-01625-z.pdf 8- !! Interesting/outstanding chains: e1 (!!!); e2 (?), e3(?)!! !!! Outstanding comparison of TRACE (2340 UT) with e1 (9d, 0100 UT) !!! !!! An outstanding chain coinsiding with a CH in the SE sector!!! 9 - !!! Outstanding chains: e1 (!!!); e2 (?), e3(?)!! !!! Outstanding comparison of e1 (01 UT)with TRACE (8d, 2340 UT) !!! !!! An outstanding chain coinsiding with a CH in the SE sector!!! 10 - !!! Outstanding/interesting chains: e1 (!!!); e2 (?), e3(?)!! !!! An outstanding chain coinsiding with a CH in the SE sector!!! 11 - !! Interesting chains: EIT 12 - Two noticeable CMEs !! Interesting chains: EIT 13 - !!! Our type II burst at ~06 UT associated with a SW CME; then one more large CME !! Interesting chains: EIT High resolution observations with Artemis--JLS, (II) Type IV associated intermediate drift bursts C. Bouratzis, A. Hillaris, C.E. Alissandrakis, P. Preka-Papadema, X. Moussas, C. Caroubalos, P. Tsitsipis, A. Kontogeorgos A&A 2019 https://arxiv.org/pdf/1904.02262.pdf Fine Structure of Metric Type-IV Radio Bursts Observed with the ARTEMIS-IV Radio Spectrograph: Association with Flares and Coronal Mass Ejections C. Bouratzis, A. Hillaris, C. E. Alissandrakis, P. Preka-Papadema, X. Moussas, C. Caroubalos, P. Tsitsipis, A. Kontogeorgos Solar Phys., 2014 http://arxiv.org/pdf/1406.1202v1.pdf 14 - A Halo (or multiple) CME !! Interesting chains: EIT 15 - !! EIT (e1): Interesting/outstanding chains perhaps with over-the-limb elements !!! 16 - 17 - 18 - !! Interesting chains at e1 !! 19 - !! A faint halo CME and EIT wave at EIT and TRACE!! !!! A large NE CME at 09 UT - our event with type II/IV bursts !!! !! Interesting chains at e1 and perhaps outstanding chains at e3!! Coronal transients and metric type II radio bursts - II. Accelerations at low coronal heights: S. Mancuso A&A 463 (2007) 1137-1141, File 20,21 - !! Interesting chains at e1 with the outstanding over-the-limb structure !! !!! Outstanding thin chains (20d,13 UT; 21d,19 UT)). See similar chains in the next rotation !!! 22-26 !! Interesting NOBE images: chains and filaments 22 - 23 - !!! Outstanding thin chains at e2 (22 UT) 24 - !! Interesting thin chains at e1 25 - !!! A halo CME !!! !! Interesting chains at e1 TRACE(4) http://solar.physics.montana.edu/nuggets/1999/990910/990910.html Which Bow Shock Theory, Gasdynamic or Magnetohydrodynamic, Better Explains CME Stand-off Distance Ratios from LASCO-C2 Observations ? Jae-Ok Lee1,2, Y.-J. Moon1, Jin-Yi Lee3, R.-S. Kim2, and K.-S. Cho2 2017 ApJ 838 70 http://sci-hub.cc/10.3847/1538-4357/aa656f Вспышки, выбросы, протонные события А.В. Белов Геомагн. и аэрономия 2016 File MAGNETIC FIELD STRENGTH IN THE UPPER SOLAR CORONA USING WHITE-LIGHT SHOCK STRUCTURES SURROUNDING CORONAL MASS EJECTIONS R.-S. Kim1,3, N. Gopalswamy1,3, Y.-J. Moon2, K.-S. Cho1,3,4 and S. Yashiro 2012 ApJ 746 118, File CME reconstruction: Pre-STEREO and STEREO era A. Thernisiena, A. Vourlidasb, and R.A. Howardb, Journal of Atmospheric and Solar-Terrestrial Physics, Volume 73, Issue 10, 2011, Pages 1156-1165 https://sci-hub.ru/10.1016/j.jastp.2010.10.019 Relations estimated at shock discontinuities excited by coronal mass ejections M. V. Eselevich and V. G. Eselevich Astronomy Reports, Volume 55, Number 4, 359-373, 2011 Astronomicheskii Zhurnal, 2011, Vol. 88, No. 4, pp. 393–408 A benchmark event sequence for mass ejection onset studies - A flare associated CME with coronal dimming, ascending pre-flare loops and a transient cool loop: R.A. Harrison and D. Bewsher A&A 461 (2007) 1155-1162, file A STUDY OF FLARE-ASSOCIATED X-RAY PLASMA EJECTIONS. I. ASSOCIATION WITH CORONAL MASS EJECTIONS Yeon-Han Kim,1, 2 Y.-J. Moon,1 K.-S. Cho,1 Kap-Sung Kim,2 and Y. D. Park ApJ 622 :1240–1250, 2005 File 26 - !! Interesting/outstanding chains at e1 27 - !!! Huge NE prominence eruption and loop CME at 01 UT !!! !! Interesting chains at e1 See TRACE 28- !! Interesting NOBE images: chains and filaments !! Interesting chains at e1 and TRACE 29 - !! Interesting chains 30 - !! Interesting chains at e1 and TRACE (one TRACE image appears belong to 31d) !! Statistics of "Cold" Early Impulsive Solar Flares in X-ray and Microwave domains Alexandra L. Lysenko, Alexander T. Altyntsev, Natalia S. Meshalkina, Dmitriy Zhdanov, Gregory D. Fleishman 2018 https://arxiv.org/pdf/1802.09288.pdf 31 - !! A large partial halo (C3/NE) CME at 11 UT !! OUR EVENT!! !! Interesting/outstanding chains and wave at EIT !! See TRACE for 30d !!