JANUARY 2000 1 - !! ~14 UT: a (partial) NE/N/SE halo CME !!! !! Interesting/outstanding chains at EIT !! 2 - !! Outstanding chains at EIT !! ILLUSTRATION Investigating the Kinematics of Coronal Mass Ejections with the Automated CORIMP Catalog Jason P. Byrne Journal of Space Weather and Space Climate 2015 http://arxiv.org/pdf/1506.04046v1.pdf The Kinematics and Morphology of Solar Coronal Mass Ejections Review J. P. Byrne A thesis, 2012, File The kinematics of coronal mass ejections using multiscale methods J. P. Byrne, P. T. Gallagher1, R. T. J. McAteer1, and C. A. Young2 A&A 495, 325–334 (2009), DOI: 10.1051/0004-6361:200809811; File Improved methods for determining the kinematics of coronal mass ejections and coronal waves J. P. Byrne, D. M. Long, P. T. Gallagher, D. S. Bloomfield, S. A. Maloney, R. T. J. McAteer, H. Morgan, S. R. Habbal E-print, July 2013; A&A 3 - !! Interesting chains at EIT !! 4 - !! Interesting chains at EIT !! 5 - !! Interesting chains at EIT !! 6 - !!! Outstanding e1 chain along a CH !!! ILLUSTRATION See NOBE movies for this and nearest days 7 - No EIT data 8 - !!! Outstanding e1,2 chain along a CH !!! ILLUSTRATION Again, a filament and activity inside a CH (see the end of Dec) !!! E4: two spectacular SE eruptions at ~07 and 16 UT !!! e1-3: uncomplete data SOHO; rotate -20 degreeses; compare with H-alpha !!! e1: a clear chain along the E limb connecting the eruption site in the S hemisphere to simmetrical NE site !!! 9 - !!! Outstanding EIT chains; coincide with a CH !!! ILLUSTRATION !!! Eruptive activity in the NW quadrant 10 - !!! Outstanding EIT (e2) chains; coincide with a CH !!! ILLUSTRATION !!! Rotation of SOHO images Over-the-limb features!!! TRACE_1 11 - !!! Interesting/outstanding chains; coincide with a CH !!! Over-the-limb features!!! 12 - !!! Interesting/outstanding chains !!! Over-the-limb features!!! 13 - !!! Interesting chains !!! A Comparison of EIT and TRACE Loop Widths S. I. Chastain, J. T. Schmelz 2017 https://arxiv.org/pdf/1705.06776.pdf 13-16 Abnormal rotation rates of sunspots and durations of associated flares G. S. Suryanarayana, K. M. Hiremath, S. P. Bagare and M. Hegde A&A 580, A25 (2015), File http://www.aanda.org/articles/aa/pdf/2015/08/aa23389-14.pdf 14 - !!! Interesting/outstanding chains !!! 15 - !!! Interesting/outstanding chains !!! SE and SW eruptions at ~17 UT 16 - !!! A filament disappearence at ~03 UT in the middle of the E-hemisphere !!! See NOBE movie !!!Outstanding complex chains at e2, 19 UT (see movies) ILLUSTRATION !!! 17 - 18 - !!! A HALO CME at ~17 UT; Two LDE and large CMEs, including our time!!! !!!Outstanding but complicated chains (e2!!!) ILLUSTRATION !!! Chains along CHs The Roles of Reconnected Flux and Overlying Fields in CME Speeds Minda Deng, Brian T. Welsch 2015 http://arxiv.org/pdf/1504.02905v1.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 ÊÐÓÏÍÎÌÀÑØÒÀÁÍÛÅ “ÄÈÌÌÈÍÃÈ”, ÂÛÇÛÂÀÅÌÛÅ ÊÎÐÎÍÀËÜÍÛÌÈ ÂÛÁÐÎÑÀÌÈ ÌÀÑÑÛ ÍÀ ÑÎËÍÖÅ, ÏÎ ÄÀÍÍÛÌ SOHO/EIT  ×ÅÒÛÐÅÕ ËÈÍÈßÕ ÊÐÀÉÍÅÃÎ ÓÔ-ÄÈÀÏÀÇÎÍÀ È. Ì. ×åðòîê, Â. Â. Ãðå÷íåâ ÀÑÒÐÎÍÎÌÈ×ÅÑÊÈÉÆÓÐÍÀË, 2003, òîì 80,¹11, ñ. 1013–1025 ÊÐÓÏÍÎÌÀÑØÒÀÁÍÛÅ ÊÀÍÀËÈÇÈÐÎÂÀÍÍÛÅ ÄÈÌÌÈÍÃÈ, ÂÛÇÛÂÀÅÌÛÅ ÊÎÐÎÍÀËÜÍÛÌÈ ÂÛÁÐÎÑÀÌÈ ÌÀÑÑÛ ÍÀ ÑÎËÍÖÅ È. Ì. ×åðòîê, Â. Â. Ãðå÷íåâ ÀÑÒÐÎÍÎÌÈ×ÅÑÊÈÉÆÓÐÍÀË, 2003, òîì 80,¹2, ñ. 162–174 19 - !!!Outstanding but complicated chains (e2!!!); consequences of the 18d events !!! ILLUSTRATION !!! Chains along CHs Eruptive and quasi-eruptive disappearing solar filaments and their relationship with coronal activities. Morimoto T., Kurorawa H. Publ.Astron.Soc.Japan. 2003. V.55. No.6. P.1141–1151; File. 20 - !!! Continuation of 19th; ILLUSTRATION !!! 21 - !!! Central/south filament eruption at 10:30 !!! !!! Continuation of outstanding interesting chains; ILLUSTRATION !!! 22 - !!! An eruption SW flare at 10:30 and 18 UT !!! !!! Continuation of outstanding interesting chains; !!! Effects of Geometries and Substructures of ICMEs on Geomagnetic Storms Jae-Ok Lee, Kyung-Suk Cho, Rok-Soon Kim, Soojeong Jang, Katsuhide Marubashi Solar Physics September 2018, 293:129 File https://link.springer.com/content/pdf/10.1007%2Fs11207-018-1344-z.pdf 23 - !!!Interesting chains; Return of CH of 28 Dec!!! The Kinematics and Morphology of Solar Coronal Mass Ejections Review J. P. Byrne A thesis, 2012, File 24 - !!!Outstanding chains including ones along CH boundaries!!!ILLUSTRATION!!! See previous rotation !!! 25 - !!!Outstanding chains including ones along CH boundaries and crossing a large CH!!! ILLUSTRATION!!! See previous rotation !!! 26 - !!! A filament eruption near the interesting CH !!! Several CMEs including a W CME at the evening !!!Outstanding chains including ones along CH boundaries and crossing a large CH!!! ILLUSTRATION!!! 27 - !!! A large S CME at ~18 UT !!! !!!Outstanding chains including ones along CH boundaries and crossing a large CH!!! ILLUSTRATION!!! !!!Interesting frames on the Yohkoh/Goes movie!!! 28 - !!! A large S CME at ~20 UT !!! !!!Interesting chains including ones along CH boundaries and crossing a large CH!!! NOBE Eruptive and quasi-eruptive disappearing solar filaments and their relationship with coronal activities. Morimoto T., Kurorawa H. Publ.Astron.Soc.Japan. 2003. V.55. No.6. P.1141–1151; File. 29 - !! Interesting chains; a large CH; NOBE !! 30,31- A number of CMEs (backside) Interesting chains One more large CH !!! NOBE - outstanding chains !!! A Comprehensive Study of the Initiation and Early Evolution of a Coronal Mass Ejection from Ultraviolet and White-Light Data A. Bemporad, J. Raymond, G. Poletto, and M. Romoli The Astrophysical Journal, 655:576–590, 2007, File 2000 January 31. Based on vector magnetograph data and magnetic field models, we find that field disruption in an active region (AR) was driven by flux emergence and shearing motions, leading to the CME and to post-CME arcades seen in the EUV.