March 2000 29 Feb - 3 Nov 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 1 - !!!Outstanding complicated chains at e1, 07 UT!!! ILLUSTRATION!!! ++2 - !!! Our type II bursts and X1 flare (W52) without large SEPs; a large SW CME!!! Unchangable Noise storm; Good spectrum !!Interesting complicated chains!! On the relationship of shock waves to flares and coronal mass ejections A. Nindos1, C. E. Alissandrakis1 , A. Hillaris2, and P. Preka-Papadema2 A&A 531, A31 (2011), File A COMPARATIVE STUDY BETWEEN ERUPTIVE X-CLASS FLARES ASSOCIATED WITH CORONAL MASS EJECTIONS AND CONFINED X-CLASS FLARES Yuming Wang1,2 and Jie Zhang Astrophysical Journal, 665:1428Y1438, 2007 August; File 3 - Two large morning CMEs: SW and SE(backside) !!Interesting complicated chains!! Large-scale Globally Propagating Coronal Waves Review Warmuth, Alexander Living Reviews in Solar Physics, PUB.NO. lrsp-2015-3, 2015 http://solarphysics.livingreviews.org/Articles/lrsp-2015-3/ File Statistical Evidence for Contributions of Flares and Coronal Mass Ejections to Major Solar Energetic Particle Events G. Trottet, S. Samwel, K.-L. Klein, T. Dudok de Wit, R. Miteva Solar Phys. 2014 http://arxiv.org/abs/1411.4133 ; File Propagation of Moreton Waves Y.Z. Zhang, R. Kitai, N. Narukage, T. Matsumoto, S. Ueno, K. Shibata and J.X. Wang E-print, April 2011, File, PASJ an event presented by Ciaravella et al. (2005) (Ciaravella, A., Raymond, J.C., Kahler, S.W., Vourlidas, A., Li, J.: 2005, Astrophys. J. 621, 1121), where the CME leading edge was identified as the shock front with SOHO UVCS observations on 3 March 2000, at 02:19 UT. Narukage(2004); Warmuth (2004a, b) 4-15 - !!Significant chain activity, CMEs, eruptions !! ++4 - Good Noise Storm 08 UT: significant NW filament eruption; See Events!! 18 UT: significant SE filament eruption; See Events and MLSO data!! 5 - 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. SoHO/EIT Observation of a Coronal Inflow Authors: Tripathi, D.; Bothmer, V.; Solanki, S. K.; Schwenn, R.; Mierla, M.; Stenborg, G. Journal: In: Coronal and Stellar Mass Ejections, IAU Symposium Proceedings of the International Astronomical Union 226, Held 13-17 September, Beijing, edited by K. Dere, J. Wang, and Y. Yan. Cambridge: Cambridge University Press, 2005., pp.133-134 On the relationship between coronal waves associated with a CME on 5 March 2000 D. Tripathi and N.-E.Raouafi E-print, Aug. 2007 Spatial and temporal correlations show that the deflection and the propagation of the kink in the streamer (based on the LASCO data), and plasma heating and spectral line broadening (based on the UVCS data), are basically due to a CME-driven shock wave. The spatial and temporal correlations between the EIT wave and the shock wave provide strong evidence in favor of the interpretation that the EIT waves are indeed the counterpart of CME-driven shock waves in the lower corona. Although, we cannot rule out the possibility that the EIT waves are just a manifestation of the stretching of the field lines due to the outward propagation of the CMEs. A bright coronal downflow seen in multi-wavelength observations: evidence of a bifurcating flux-rope? D. Tripathi, S.K. Solanki, H.E. Mason, D.F. Webb A bright coronal downflow seen in multi-wavelength observations: evidence of a bifurcating flux-rope? D. Tripathi, S.K. Solanki, H.E. Mason, D.F. Webb E-print, July 2007; Astronomy and Astrophysics, Volume 472, Issue 2, September III 2007, pp.633-642; File 7 - Hydrogen and the Abundances of Elements in Impulsive Solar Energetic-Particle Events Donald V. Reames Solar Phys. 2019 https://arxiv.org/ftp/arxiv/papers/1901/1901.04369.pdf Statistical Analysis of Periodic Oscillations in LASCO Coronal Mass Ejection Speeds G. Michalek, A. Shanmugaraju, N. Gopalswamy, S. Yashiro, S. Akiyama Solar Phys. Volume 291, Issue 12, pp 3751–3764 2016 http://link.springer.com/article/10.1007/s11207-016-1000-4 On the relationship of shock waves to flares and coronal mass ejections A. Nindos1, C. E. Alissandrakis1 , A. Hillaris2, and P. Preka-Papadema2 A&A 531, A31 (2011), File 10 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 10-22 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 13 Microwave Signature of Relativistic Positrons in Solar Flares G. D. Fleishman, A. T. Altyntsev, and N. S. Meshalkina Publ. Astron. Soc. Japan 65, No. SP1, S7 [5 pages] (2013) http://pasj.asj.or.jp/v65/sp1/65S007/65S007.pdf 16 - !Complication of the chains! Compare with the 17 Feb 17 - !!Interesting/outstanding chains!! 18 - !!Interesting/outstanding chains!! Not full data 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 19 - A number of CMEs !!Interesting/outstanding chains!! !! Chains inside a CH !! *20 - !!! A large SE CME and then a filament eruption in the S hemicphere !!! !! Our type II burst !! !!Interesting chains!! !! Chains inside a CH !! 21 - A number of large CMEs !Usual/Interesting chains! !!! Activity and chain inside a large CH !!! ILLUSTRATION!!! (see movies and previous rotations) 22 - A number of large CMEs; 18:50 UT: X1.1 flare and a partial HALO CME!! See: Lee et al., BBSO#1164, 2002 !Usual/Interesting chains! !!! Activity and chain inside a large CH !!! ILLUSTRATION!!! (see movies and previous rotations) Frequency rising sub-THz emission from solar flare ribbons E.P. Kontar, G.G. Motorina, N.L.S. Jeffrey, Y.T. Tsap, G.D. Fleishman, A.V. Stepanov A&A 2018 https://arxiv.org/pdf/1810.03922.pdf 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 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 22-25 Streamer Blowout Coronal Mass Ejections: Their Properties and Relation to the Coronal Magnetic Field Structure Angelos Vourlidas, David F. Webb ApJ 2018 https://arxiv.org/ftp/arxiv/papers/1806/1806.00644.pdf 23- Not enough SOHO data Possible manifestation of large-scale transverse oscillations of coronal loops in solar microwave emission M. L. Khodachenko1, K. G. Kislyakova2, T. V. Zaqarashvili1,3, A. G. Kislyakov2, M. Panchenko1, V. V. Zaitsev4, O. V. Arkhypov5 and H. O. Rucker1 A&A 525, A105 (2011) Observations of The Magnetic Reconnection Signature of An M2 Flare on 2000 March 23 Leping Li and Jun Zhang E-print, July 2009, ApJ *24 - !!! Our event: type II/IV bursts, X1.8 flare !!! Not enough SOHO data A Comparison of EIT and TRACE Loop Widths S. I. Chastain, J. T. Schmelz 2017 https://arxiv.org/pdf/1705.06776.pdf Particle Acceleration and Propagation in Strong Flares without Major Solar Energetic Particle Events K.-L. Klein • G. Trottet • S. Samwel • O. Malandraki Solar Phys (2011) 269: 309–333; File +25 - Not enough SOHO data Strong unchangable Noise storm !! Yohkoh, ~07 UT: clear soft X-ray wave(?) ILLUSTRATION!! Streamer Blowout Coronal Mass Ejections: Their Properties and Relation to the Coronal Magnetic Field Structure Angelos Vourlidas, David F. Webb ApJ 2018 https://arxiv.org/ftp/arxiv/papers/1806/1806.00644.pdf 26 - !!Two eruptive events!! !!!Outstanding chains (including ones inside a CH)!!! ILLUSTRATION Millisecond Radio Spikes in the Decimetric Band B. P. Dabrowski, P. Rudawy and M. Karlicky Solar Physics, Volume 273, Number 2, 377-392, 2011 *27 - !!!Our type II burst at 07:50 UT and a SE CME!! !!Interesting complicated chains !! 28 - !!Interesting complicated chains !! !!!Clear high-latitude eruption in the NW quadrant at ~22 UT!!! 29 - !!Clear backside(?) HALO at ~10:30UT!! !!!Interesting/outstanding chains after the NW filament eruption of 28d, 22 UT (see NOBE, e3 and so on)!!! ILLUSTRATION 30 - !! Interesting chains !! NOBE A Statistical Study on Property of Spatial Magnetic Field for Solar Active Region Liu Suo Ap&ss 2014 http://arxiv.org/pdf/1405.2149v1.pdf 31 - !! A partial SE halo CME at ~08 UT !! !! Interesting chains !! NOBE !! Activity inside a NW CH!!