June 1999 ****************************** 26 May - ... !! NOBE: Outstanding longitudinal chains in the north hemisphere ****************************** 1 - !!! A pronounced back-side halo CME at ~14 UT EIT data start at 13 UT !! EIT: interesting chains at e1.e2 2 - !!! A large W/NW CME !!! EIT: outstanding chains at e1.e2 between two large CMEs COMPARING SPATIAL DISTRIBUTIONS OF SOLAR PROMINENCE MASS DERIVED FROM CORONAL ABSORPTION Holly Gilbert1, Gary Kilper1, David Alexander2, and Therese Kucera1 Astrophysical Journal, 727:25 (12pp), 2011, File 3 - !!! A pronounced evening halo CME !!! EIT: outstanding chains at e1.e2 4 - !!! A continuation of the pronounced evening halo CME !!! Our M4 LDE (with a type II burst) associated with partial halo and loop CMEs !!! EIT: outstanding chains at e1,e2,e3,e4(!) ************A subject for a comprehensive study**************** Distinguishing the Rigidity Dependences of Acceleration and Transport in Solar Energetic Particles Donald V. Reames Solar Phys. 2020 https://arxiv.org/ftp/arxiv/papers/2006/2006.11338.pdf Large gradual solar energetic particle events Review Mihir Desai, Joe Giacalone Living Reviews in Solar Physics, December 2016, 13:3 http://solarphysics.livingreviews.org/ What are the Sources of Solar Energetic Particles? Element Abundances and Source Plasma Temperatures Review Donald V. Reames Space Sci. Rev 2015 http://arxiv.org/pdf/1510.03449v1.pdf File Interplanetary magnetic field line mixing deduced from impulsive solar flare particles. Mazur JE, Mason GM, Dwyer JR, Giacalone J, Jokipii JR, Stone EC (2000) Astrophys J 532:L79–L82. doi:10.1086/ 312561 https://iopscience.iop.org/article/10.1086/312561/pdf 5 - !!! EIT: outstanding chains at e1,e2,!!! A remarkable, but confused, coronal hard X-ray source Alexandra Lysenko, Larisa Kashapova, Hugh Hudson RHESSI Science Nuggets #325 June 2018 http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/A_remarkable,_but_confused,_coronal_hard_X-ray_source 6 - !!! EIT: outstanding chains at e1,e2,!!! 7 - !!! EIT: outstanding chains at e1,e2,!!! 9 - EIT: interesting chains TRACE!! 10 - Many CMEs !! EIT: outstanding chains, including a looop above NE limb (e1) !! TRACE!!! Good correspondance !!! 11 - !!! Partly our C7 LDE (with a type II burst) at 1145 UT associated with a very large NE/E CME Plasma Physical Parameters along CME-driven Shocks. II. Observation–Simulation Comparison F. Bacchini1, R. Susino2, A. Bemporad2, and G. Lapenta1 2015 ApJ 809 58 Plasma physical parameters along Coronal Mass Ejection-driven shocks: I observations A. Bemporad, R. Susino, G. Lapenta ApJ, 2014 http://arxiv.org/pdf/1403.0870v1.pdf IDENTIFICATION OF SUPER- AND SUBCRITICAL REGIONS IN SHOCKS DRIVEN BY CORONAL MASS EJECTIONS A. Bemporad and S. Mancuso 2011 ApJ 739 L64 Coronal transients and metric type II radio bursts - II. Accelerations at low coronal heights: S. Mancuso A&A 463 (2007) 1137-1141, File 12 - !!! Outstanding chains: e1 (19 UT !!!); e2 (?), e3(?) 13 - 15:30 UT: coronal wave at TRACE - Wills-Davey & Thompson 1999. - Ballai et al. The Astrophysical Journal, 633:L145–L148, 2005 November 10 !!! A two-petal (E and S) halo CME at ~ 17 UT !!! Outstanding chains: e1 (!!!); e2 (?), e3(?) 14 - !!! A spectacular SE CME at ~14 UT associated with S filament eruption See Events! !!! Outstanding chains: e1 (!!!); e2 (?), e3(?) http://solar.physics.montana.edu/nuggets/1999/990618/990618.html 15 - !!! Outstanding chains: e1 (!!!); e2 (?), e3(?) 16 - A number of morning CMEs !!! Outstanding chains: e1 (!!!); e2 (?), e3(?) 17 - !!! Outstanding chains: e1 (!!!); e2 (?), e3(?) 18 - !!! Outstanding chains: e1 (!!!); e2 (?), e3(?) 19 - !! A partial N galo at ~13 UT !!! Interesting chains (perhaps absorptions): e1 (!!!); e2 (?), e3(?) 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 20 - !! Interesting chains: e1 (!!!); e2 (?), e3(?) 21 - !! Interesting chains: e1 (!!!); e2 (?), e3(?) 22 - !! Interesting chains: e1 (!!!); e2 (?), e3(?) !! NOBE: a high latitute chain !! 23 - !! Interesting chains: e1 (!!!); e2 (?), e3(?) !! NOBE: a high latitute chain !! +24 - ! A partial halo CME at ~14 UT! Complicated eruption including filament, See Events! !! Interesting chains: e1 (!!!); e2 (?), e3(?) TRACE: 17 UT, but chains are not outstanding Coronal Flux Ropes and their Interplanetary Counterparts N. Gopalswamy, S. Akiyama, S. Yashiroa, H. Xie J. Atmos. Solar-Terr. Phys. 2017 https://arxiv.org/pdf/1705.08912.pdf 25 - !! Interesting chains: e1 (!!!); e2 (?), e3(?) !! NOBE: a high latitute chain !! Noise storm at our spectrum 26 - !!! Very Interesting chains: e1 (!!!); e2 (?), e3(?) !! NOBE: a high latitute chain coinciding with e1 !! Global eruption does not affected almost strong NS. 26-28 Magnetic Field Configuration Models and Reconstruction Methods for Interplanetary Coronal Mass Ejections N. Al-Haddad, T. Nieves-Chinchilla, N. P. Savani, C. Mostl, K. Marubashi, M. A. Hidalgo, I. I. Roussev, S. Poedts, C. J. Farrugia Solar Phys. 2013; File +27 - !! Interesting chains: e1 (!!!); e2 (?), e3(?) +09 UT: Strong eruption, coronal wave, dimmings, small manifestations at E4, Our event; Global eruption does not affected almost strong NS. See Events !! NOBE: a high latitute chain !! 28 - !! Interesting chains: e1 (!!!); e2 (?), e3(?) !! NOBE: interesting chains !! Coronal Sources and In Situ Properties of the Solar Winds Sampled by ACE During 1999–2008 Hui Fu, Bo Li, Xing Li, Zhenghua Huang, Chaozhou Mou, Fangran Jiao, Lidong Xia Solar Phys. 2015 http://arxiv.org/pdf/1505.00407v1.pdf 29 - !!! A spectacular halo CME at ~07 UT !! Interesting chains: e1 (!!!); e2 (?), e3(?) TRACE: 02 UT, but e1 at 07 UT only ILLUSTRATION !! NOBE: interesting chains !! 30 - !!! A large W CME, halo at ~05 UT !! Interesting chains: e1 (!!!); e2 (?), e3(?) !! NOBE: interesting chains !! Relationship between non-thermal electron energy spectra and GOES classes R. Falewicz1, P. Rudawy1, and M. Siarkowski2 E-print, Apr 2009, File; A&A