January 2001 1 - Interesting/complicated chains; CHs !A thin chain above a filament! A new catalogue of solar flare events from soft x-ray GOES signal in the period 1986-2020 Nicola Plutino, Francesco Berrilli, Dario Del Moro, Luca Giovannelli Advances in Space Research 2022 https://arxiv.org/pdf/2211.10189.pdf Thermal and magnetic field structure of near equatorial coronal holes K. M. Hiremath, Manjunath Hegde 2022 https://arxiv.org/pdf/2204.04410.pdf 2 - Interesting/complicated chains; a large AR and CHs !A thin chain above a filament! Coronal Mass Ejections Associated with Slow Long Duration Flares U. Bak-Steslicka, S. Kolomanski, T. Mrozek E-print, Feb 2013, File; Solar Phys. 3 - Interesting/complicated chains 4 - !!Interesting/outstanding chains !! Development of a large bright point inside a CH 5 - !Interesting chains ! !A clear W halo CME with a remarkabe flat E front; backside?! 6 - Interesting chains ~09 UT: a sharp appearance of a small (but clear) noise storm at the fixed frequencies Traveling ionospheric disturbances as huge natural lenses: Solar radio emission focusing effect, Koval, A., Y. Chen, A. Stanislavsky, and Q.-H. Zhang (2017). J. Geophys. Res. Space Physics, 122 DOI: 10.1002/2017JA024080 http://sci-hub.cc/10.1002/2017JA024080 7 - !!!03-04 UT: A spectacular NW filament eruption at EIT, NOBE and clear three-component CME !!! Interesting chains KINK INSTABILITIES TRIGGERING A FILAMENT ERUPTION CRISTIANA DUMITRACHE, DIANA CONSTANTIN RoAJ 20, 35-44, 2010 E-print, Dec 2010 8 - Interesting chains, including thin one along a large filament A slow but clear activity of a large NE filament 9 - Interesting chains +10 - !!01 UT: a large E halo CME, type II and activity !! !Interesting/outstanding chains and wave!! !!!10:15 UT: our fragmentary type II and extremely impulsive M3 flare!!! 11 - !Interesting/outstanding chains! 12 - 08 UT: a bright E CME !Interesting/outstanding chains! 13 - !Interesting/outstanding chains! ++14 - !!!05 UT: a large NW filament eruption (NOBE, EIT), 4-linedimming, spectacular CME with an inside prominence!!! Observations of Prominence Eruptions with Two Radioheliographs, SSRT and NoRH V. V. Grechnev et al., PASJ: Publ. Astron. Soc. Japan , 58, 69- , 2006. !Interesting/outstanding chains! ILLUSTRATION; MOVIE; See Events! 15 - Almost no SOHO data High-latitude chains as a consequence of the 14d filament eruption 16 - !Interesting chains! 17 - 01 UT: type II/IV, SE backside Interesting cchains 18 - Interesting chains 07-12 UT: SE transient events 19 - !!Interesting/outstanding chains!! 16-17 UT: M1 flare and E CME +20 - !!Interesting/outstanding chains; see NOBE!! Illustration!! 19 and 21 UT: M1, M7 flares, Two E HALO CMEs, type II bursts, dimmings!! Interacting CMEs and their associated flare and SEP activities A.Shanmugaraju, S.Prasanna Subramanian 2014 http://arxiv.org/pdf/1405.6316v1.pdf Solar Energetic Particles and Associated EIT Disturbances in Solar Cycle 23 R. Miteva, K.-L. Klein, I. Kienreich, M. Temmer, A. Veronig, O. E. Malandraki E-print, Feb 2014, File; Solar Phys. http://arxiv.org/pdf/1402.1676v1.pdf Wang, A. H., Wu, S. T., & Gopalswamy, N. 2005, Geophys. Monograph Ser., 156, GM21 The CME dynamics sometimes is also affected by interaction with other CMEs See: Gilbert et al. -- A Comparison of CME-Associated Atmospheric Waves Observed in Coronal (Fe XII 195 A) and Chromospheric (He I 10830 A) Lines, Ap. J., V. 607(1), pp. 540-553, 2004. -- Chromospheric Waves Observed in the He I Spectral Line (lambda = 10830 A): A Closer Look. The Astrophysical Journal, V.610(1),572-587, 2004. TRANSIENT CORONAL HOLES AS SEEN IN THE He i 1083 nm MLSO OBSERVATIONS G. de Toma et al. The Astrophysical Journal, 621:1109–1120, 2005 SOLAR TYPE II RADIO BURSTS AND IP TYPE II EVENTS H. V. Cane and W. C. Erickson Astrophysical Journal, 623:1180–1194, 2005; File CONSTRAINTS ON CORONAL MASS EJECTION DYNAMICS FROM SIMULTANEOUS RADIO AND WHITE-LIGHT OBSERVATIONS M. J. Reiner, A. Vourlidas, O. C. St. Cyr, J. T. Burkepile, R. A. Howard, M. L. Kaiser, N. P. Prestage, and J.-L. Bougeret Astrophysical Journal, 590:533–546, 2003; File +21 - !!Interesting/outstanding chains; see NOBE!! Illustration !! 22 - !!Interesting/outstanding chains; see NOBE!! 23 - Interesting chains A new method to detect the ICMEs boundaries Cristiana Dumitrache, Nedelia A. Popescu 2014 http://arxiv.org/pdf/1405.6002v1.pdf 24 - Interesting chains 25 - Interesting chains +26 - !01;30 UT: NW filament eruption and clear CME! preceded by two more CMEs (NE and SW) !!11:57 UT: a part of type II burst on our spectrum !16 UT: a bright NE CME An observational revisit of band-split solar type-II radio bursts Guohui Du, Xiangliang Kong, Yao Chen, Shiwei Feng, Bing Wang, Gang Li 2015 http://arxiv.org/pdf/1509.03832v1.pdf 27 - Interesting chains, CH-associated 28 - !!15:30 UT: M1.5 LDE, moderate microwaves, clear W CME, protons J10~27 How Do Shock Waves Define the Space-Time Structure of Gradual Solar Energetic Particle Events? Review Donald V. Reames Space Sci. Rev 2022 https://arxiv.org/ftp/arxiv/papers/2210/2210.16693.pdf Geoeffectiveness of the coronal mass ejections associated with solar proton events Gui-Ming Le, Chuan Li, Yu-Hua Tang, Liu-Guan Ding, Zhi-Qiang Yin, Yu-Lin Chen, Yang-Ping Lu, Min-Hao Chen, Zhong-Yi Li Research in Astronomy and Astrophysics (RAA) Vol 16, No 1 (2016) paper 14, File 29 - !!~15 UT: E filament eruption and large CME 30 - Interesting chains, CH-associated 31 - The Extended Field-aligned Suprathermal Proton Beam and Long-lasting Trapped Energetic Particle Population Observed Upstream of a Transient Interplanetary Shock D. Lario1, I. G. Richardson1,2, L. B. Wilson III1, L. Berger1, L. K. Jian1, and D. Trotta3 2022 ApJ 925 198 https://iopscience.iop.org/article/10.3847/1538-4357/ac3c47/pdf