December 2002 1 - Several eruptions 2 - Several eruptions 2-7 Long-Term Oscillations of Sunspots and a Special Class of Artifacts in SOHO(MDI) and SDO(HMI) Data V.I. Efremov, A.A. Soloviev, L.D. Parfinenko, A. Riehokainen, E. Kirichek, V.V. Smirnova, Y.N. Varun, I. Bakunina, I. Zhivanovich 2018 https://arxiv.org/ftp/arxiv/papers/1802/1802.06379.pdf 3 - Impulsive flare +4- Flare: very impulsive NE near-limb M2.5/2N flare at 22:49 UT, type II/IV; dimmings; See Events 9- Interesting chains; CHs 10- Interesting chains; CHs 12:30 UT: SE eruption 11- Interesting chains; CHs 11 UT: S filament eruption and partial halo CME ++12- Interesting chains; CHs +02 UT: SE eruption, 3-line canalized dimmings; See EVENTS 11:30 UT: W-limb eruption; See events The injection of ten electron/3He-rich SEP events Linghua Wang1, Sam Krucker2,3, Glenn M. Mason4, Robert P. Lin2 and Gang Li A&A 585, A119 (2016) http://arxiv.org/pdf/1605.07882v1.pdf ++13- Interesting chains; CHs ++11 UT: SE eruption; 3-line dimming; brightening at e4; interaction with CH SEE EVENT 17:30 UT: NE eruption +14- Interesting chains; CHs 07 UT: SW filament eruption; See Events +17:30 UT: SE eruption near a vertical CH; dimmings; SEE Events and 13d +15- Interesting chains; CHs +03 UT: SW filament eruption; large dimmings near a CH; e4-separate dimming?; See Events +16- Interesting chains; CHs +11:15 UT: M2.5 NE flare, eruption without CME, See Events 3-line dimmings (no e4 data at present time) +Our clear, but narrow-band type II burst consisting from vertical bands +19 UT: SE eruption near a vertical CH; canalized dimmings; e4-separate dimming?; SEE Events and other days 16-21 Pre-Flare Dynamics of Sunspot Groups M. B. Korsos, T. Baranyi, A. Ludmany 2014 http://arxiv.org/pdf/1405.7485v1.pdf +17- Interesting chains; CHs +>14 UT: significant brightening of the S CH boundary at 4 lines and dimmings; SEE EVENTS!! +18 - Interesting chains; CHs +06:40 UT: central M2.4 flare, Noise Sterm ++19 - Interesting chains; CHs +08 UT: halo CME +21:40 UT: central M2.4 flare, halo CME; 4-line dimmings!!!See Events!!! http://science.nasa.gov/spaceweather/images2002/20dec02/cme_c3_big.gif The Origin of Sequential Chromospheric Brightenings Michael S. Kirk, K.S. Balasubramaniam, Jason Jackiewicz, Holly R. Gilbert Solar Phys. 2017 https://arxiv.org/pdf/1704.03828.pdf Properties of solar energetic particle events inferred from their associated radio emission A. Kouloumvakos, A. Nindos, E. Valtonen, C.E. Alissandrakis, O. Malandraki, P. Tsitsipis, A. Kontogeorgos, X. Moussas, A. Hillaris A&A 2015 http://arxiv.org/pdf/1507.03776v1.pdf Trend of photospheric magnetic helicity flux in active regions generating halo coronal mass ejections_ A. Smyrli1,2, F. Zuccarello1, P. Romano3, F. P. Zuccarello4, S. L. Guglielmino1, D. Spadaro3, A. W. Hood2, and D. Mackay2 A&A 521, A56 (2010), File Sequential Chromospheric Brightenings beneath a Transequatorial Halo Coronal Mass Ejection, Balasubramaniam, K. S.; Pevtsov, A. A.; Neidig, D. F.; Cliver, E. W.; Thompson, B. J.; Young, C. A.; Martin, S. F.; Kiplinger, A. The Astrophysical Journal, Volume 630, Issue 2, pp. 1160-1167, 2005. +20 - Interesting chains; CHs +08:30 UT: type III grope with reverse-drifting low-frequency component; See our compressed spectrum ; See Events KW-Sun: The Konus/WIND Hard X-ray Solar Flare Database Alexandra Lysenko and the Konus/WIND Team RHESSI Science Nuggets #287 Dec 2016 http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/KW-Sun:_The_Konus/WIND_Hard_X-ray_Solar_Flare_Database Solar flares at submillimeter wavelengths A review Sam Krucker • C.G. Gimenez de Castro • H.S. Hudson • G. Trottet • T.S. Bastian • A.S. Hales • J. Kasparova • K.-L. Klein • M. Kretzschmar • T. Luthi • A. Mackinnon • S. Pohjolainen • S.M. White Astronomy and Astrophysics Review, Volume 21, Issue 1, (2013) 21:58; File Radio-loud CMEs from the disk center lacking shocks at 1 AU N. Gopalswamy, P. Makela, S. Akiyama, S. Yashiro, H. Xie, R. J. MacDowall, M. L. Kaiser E-print, June 2012, JGR, 117, A08106, 2012 A solar burst with a spectral component observed only above 100=GHz during an M class flare: G. Cristiani, C. G. GimΘnez de Castro, C. H. Mandrini, M. E. Machado, I. de Benedetto e Silva, P. Kaufmann and M. G. Rovira A&A 492 (2008) 215-222 ++21 - Interesting chains; CHs +Morning N filament eruption; 4-line dimmings; SEE EVENTS A STUDY OF FAST FLARELESS CORONAL MASS EJECTIONS H. Q. Song1,2, Y. Chen1, D. D. Ye1, G. Q. Han1, G. H. Du1, G. Li1,3, J. Zhang2, and Q. Hu 2013 ApJ 773 129, File ++22 - Interesting chains; CHs +02:50 UT: M1.2 LDE and NW filament eruption; Canalized dimming; See EVENTS significant FD Formation of Isolated Radio Type II Bursts at Low Frequencies Silja Pohjolainen, Nasrin Talebpour Sheshvan Solar Phys. 2021 https://arxiv.org/pdf/2104.09891.pdf 23 - Interesting chains; CHs 24 - Interesting chains; CHs The Interaction Between Coronal Mass Ejections and Streamers: A Statistical View over 15 Years (1996?–?2010) O. Floyd, P. Lamy, A. Llebaria Solar Physics, April 2014, Volume 289, Issue 4, pp 1313-1339; File 25 - Interesting chains; CHs +26 - Interesting chains; CHs +18:30 UT: significant NE-limb eruption and narrow CME; dimmings at 4 lines; SEE EVENTS A STUDY OF FAST FLARELESS CORONAL MASS EJECTIONS H. Q. Song1,2, Y. Chen1, D. D. Ye1, G. Q. Han1, G. H. Du1, G. Li1,3, J. Zhang2, and Q. Hu 2013 ApJ 773 129, File 27 - Interesting chains; CHs +28 - Interesting chains; CHs +13:20 UT: NW-limb eruption and CME; SEE EVENTS Two Successive Coronal Mass Ejections Driven by the Kink and Drainage Instabilities of an Eruptive Prominence G. P. Zhou, J. X. Wang, J. Zhang, P. F. Chen, H. S. Ji, and K. Dere The Astrophysical Journal, 651:1238Y1244, 2006 29 - Interesting chains; CHs 30 - Interesting chains; CHs 30 - Interesting chains; CHs 22 UT: halo CME, backside