January 2002 No Yohkoh data from 14 Dec 1 - !Interesting chains! Outstanding at E1,E2, NOBE (movie)! !19 UT: powerful W CME! !Large Forbush on 31d_01d! 2 - !Interesting chains! Outstanding at E1,E2, NOBE (movie)! 3 - !Interesting chains! Outstanding at E1,E2, NOBE (movie)!ILLUSTRATION! !Continuation of large and long composite Forbush!! +4 - !Interesting/outstanding chains! E1,E2, NOBE (movie)! !09 UT: spectacular NE-limb filament eruption, butiful CME! ILLUSTRATION! our type II burst! See Events!! Polarimetric Reconstruction of Coronal Mass Ejections from LASCO-C2 Observations O. Floyd, P. Lamy Solar Physics November 2019, 294:168 https://link.springer.com/content/pdf/10.1007%2Fs11207-019-1553-0.pdf The origin, early evolution and predictability of solar eruptions Review Lucie Green, Tibor Torok, Bojan Vrsnak, Ward Manchester IV, Astrid Veronig Space Science Reviews 2018 https://arxiv.org/pdf/1801.04608.pdf File A New Method to Determine the Temperature of CMEs Using a Coronagraph Filter System Kyuhyoun Cho, Jongchul Chae, Eun-kyung Lim, Kyung-suk Cho, Su-Chan Bong, Heesu Yang J. of Korean Astronomical Society (JKAS) 2016 http://arxiv.org/pdf/1603.07047v1.pdf 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 Some properties of the development of the perturbed zone and shock preceding a coronal mass ejection M. V. Eselevich & V. G. Eselevich Astronomy Reports, Volume 55, Number 11, 1038-1050, 2011, File Astronomicheskii Zhurnal, 2011, Vol. 88, No. 11, pp. 1124–1136. Observed Aspects of Reconnection in Solar Eruptions Ronald L. Moore • Alphonse C. Sterling • G. Allen Gary • JonathanW. Cirtain • David A. Falconer Space Sci Rev., 2011, File Yurchishin Evidense for a flux rope model... Pr. BBSO#1144, ApJ, 576, 493, 2002 See: ftp://ftp.ias.u-psud.fr/pub/gartzner/SAF/ Sterling and Moore, ApJ, 613, 1221-1232, file, text 5 - !Interesting/outstanding chains, CH! E1,E2, NOBE (movie)! +6 - !Interesting/outstanding chains, CH! E1,E2, NOBE (movie)! !!!Evening: Clear chain inside CH; E2, E3; ILLUSTRATION !!! +7- !Interesting/outstanding chains, CH! E1,E2, NOBE (movie)! !!!Morning: Clear chain inside CH; E2, E3; ILLUSTRATION !!! +8- !Interesting/outstanding chains, CH! E1,E2, NOBE (movie)! COMET!!! !!17:36 UT: powerful W halo CME, bakside; !!18:00 UT; spectacular NW filament eruption and CME with comet!! filament brightening at 195 A before the eruption!Chains!ILLUSTRATION!!! See Events (make a new movie) Review on Current Sheets in CME Development: Theories and Observations Jun Lin, Nicholas A. Murphy, Chengcai Shen, John C. Raymond, Katharine K. Reeves,Jiayong Zhong, Ning Wu, Yan Li Space Science Reviews 2015 File Open Access Tracking a Ulysses High-latitude ICME Event Back to Its Solar Origins C. Dumitrache • N.A. Popescu • A. Oncica Solar Phys (2011) 272:137–157 Morphology and density structure of post-CME current sheets B. Vr?snak1, G. Poletto2, E. Vuji?c3, A. Vourlidas4, Y.-K. Ko4, J. C. Raymond5, A., Ciaravella6, T. ?Zic1, D. F. Webb7, A. Bemporad8, F. Landini9, G. Schettino9, C., Jacobs10, and S. T. Suess11 E-print, Feb 2009, File; A&A, 499 (2009) 905-916 SOLAR TYPE II RADIO BURSTS AND IP TYPE II EVENTS H. V. Cane and W. C. Erickson Astrophysical Journal, 623:1180–1194, 2005; File Ko et al. Dynamical and Physical Properties of a Post-CME Current Sheet. ApJ, 2003, Vol.594, p1068 (E-print http://solar.physics.montana.edu/cgi-bin/eprint/index.pl?entry=692) +9- !Interesting/outstanding chains, CH! E1,E2, NOBE (movie)! COMET!!! !! Morning: slowly-elevating SE filament and CME as a continuation of the 8d event; EIT and NOBE, SSRT? See Events !!18 UT: M9.5 central flare; see Event!! 9-12 Horizontal flow below solar filaments P. Ambroz1 and W. Potzi2 A&A 613, A39 (2018) https://www.aanda.org/articles/aa/pdf/2018/05/aa31162-17.pdf 10- !Interesting/outstanding chains, CH! E1,E2, NOBE (movie)! Spatial Offsets in Flare-CME Current Sheets John C. Raymond, Silvio Giordano, Angela Ciaravella 2017 https://arxiv.org/pdf/1706.03090.pdf 11- !Interesting/outstanding chains, CH-associated! !Morning: clear NE chain; illustration! !08 UT: significant SW-limb filament eruption!! http://www.ct.astro.it/sole/prom_c_20020111.jpg No EIT data from 11d, 18 UT to Element Abundances in Solar Energetic Particles and the Solar Corona Donald V. Reames E-print, June 2013, File; Solar Phys. Observational Study of a Peculiar Solar Limb Event Occurred on 11 January 2002 Hui Li ? Jianqi You E-print, Apr. 2009; Solar Phys (2009) 258: 89–104 12 - NOBE chains +13 - NOBE chains, no EIT data !~10 UT: large NE CME; backside? ! Our weak type II burst Deflection of coronal rays by remote CMEs: shock wave or magnetic pressure? Boris Filippov1 and A.K. Srivastava2 E-print, June 2009, File, Solar Phys. +14 - NOBE chains, no EIT data till 19 UT !06 UT: M4 LDE and powerful SW CME (halo) from filament eruption 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 Estimating the Height of CMEs Associated with a Major SEP Event at the Onset of the Metric Type II Radio Burst during Solar Cycles 23 and 24 P. Makela, N. Gopalswamy, S. Akiyama, H. Xie, and S. Yashiro ApJ 2015 http://cdaw.gsfc.nasa.gov/publications/makela/makela2015ApJ.pdf 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 15 - Interesting chains; No LASCO data 16 - Interesting chains; No LASCO data 17 - Interesting chains; No LASCO data 18 - Interesting chains; low flare activity 15 UT: large E CME 18-19 Solar Wind Electron Strahls Associated with a High-Latitude CME: \emph{Ulysses} Observations M. Lazar, J. Pomoell, S. Poedts, C. Dumitrache, N.A. Popescu Solar Phys., 2014 http://arxiv.org/pdf/1405.5690v1.pdf 19 - Interesting chains; low flare activity 20 - Interesting chains; low flare activity 21 - Interesting chains; low flare activity !!14 UT: clear SW-limb eruption and CME!! !17 UT: SE CME! +22 - Interesting chains; NOBE!; low flare activity !!08 UT: our short peculiar (filament) type II burst, spectacular S/central eruption !!~09 UT: W M1.3 impulsive flare. Connection? See Events 23 - Interesting chains; NOBE!; !13 UT: brightening chain, eruption, large-scale reconstruction of the corona! See Events Particle Acceleration in Plasmoid Ejections Derived from Radio Drifting Pulsating Structures N. Nishizuka1, M. Karlicky2, M. Janvier3, and M. Barta 2015 ApJ 799 126 http://arxiv.org/pdf/1412.7904v1.pdf Large Amplitude Oscillations in Prominences D. Tripathi • H. Isobe • R. Jain 2009; File, Large amplitude oscillatory motion along a solar filament B. Vrsnak, A.M. Veronig, J.K. Thalmann, T. Zic E-print, July 2007 +24 - Interesting/outstanding chains; NOBE!; Illustration! !!~03 UT: C7.3 LDE, large E-limb CME, post-eruption loops!! Over-the-limb canalized dimming!! See Events! +25 - Interesting/outstanding chains; NOBE!; !!02:30 UT: central eruption, C6.6, type II burst, NE CME See Events Radio Spectroscopic Imaging of a Solar Flare Termination Shock: Split-Band Feature as Evidence for Shock Compression Bin Chen (1), Chengcai Shen (2), Katharine K. Reeves (2), Fan Guo (3 and 4), Sijie Yu (1) ApJ 2019 https://arxiv.org/pdf/1908.09146.pdf 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 26 - Interesting/outstanding chains; NOBE!; EIT: vertical chains! +27 - Interesting chains; NOBE movie ~10 UT: large NW CME and small SPE; development of type III/noise activity at high-frequency range of our spectrum 27-28 Precursory Signals of Forbush Decreases Not Connected with Shock Waves D. Lingri, H. Mavromichalaki, M. Abunina, A. Belov, E. Eroshenko, I. Daglis & A. Abunin Solar Physics volume 297, Article number: 24 (2022) https://link.springer.com/content/pdf/10.1007/s11207-022-01951-4.pdf +28 - Interesting/outstanding chains; NOBE!; EIT: !!~10 UT: spectacular SE filament eruption and chains; moderate CME!! !!Filament-associated canalized dimmings; 304 A dimming!! Suitable for analysis with Nancay data See Event 29 - Interesting chains; 30 - Interesting/outstanding chains; NOBE!; EIT: vertical chains! Illustration! Narrowband Gyrosynchrotron Bursts: Probing Electron Acceleration in Solar Flares Gregory D. Fleishman, Gelu M. Nita, Eduard P. Kontar, Dale E. Gary ApJ 2016 http://arxiv.org/pdf/1605.00948v1.pdf 31 - Interesting/outstanding chains; NOBE!; EIT: vertical chains! CH! Illustration!