March 2001 март–апрель 2001 г. Анализ форбуш-понижений в периоды сильных геомагнитных возмущений в марте–апреле 2001 г. М. В. Кравцова, В. Е. Сдобнов Письма в Астрономический журнал, - 2014, #8, С. +1 - ~20 UT: one more spectacular central filament eruption, CME, outstanding chains; ILLUSTRATION !! Two CHs 2 - Some concequences ***************************** 171 A is in a 12-min cadence ***************************** 3 - Interesting chains. Yohkoh, ~04-.. UT: a spectacular bright point and arcade formation; chains inside a CH; Forbush from the halo CME of 28 Feb 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 4 - Interesting/outstanding chains 5 - Interesting/outstanding chains ICME On the Flux-Rope Topology of Ejecta Observed in the Period 1997?–?2006 M. A. Hidalgo, T. Nieves-Chinchilla, J. J. Blanco Solar Physics, May 2013, Volume 284, Issue 1, pp 151-166 6 - Interesting/outstanding chains 7 - Interesting/outstanding chains +8 - Interesting/outstanding chains ILLUSTRATION !! !!1120 UT: very impulsive M5 flare, CME, !!! our type II burst with clear RD elements; VERY INTERESTING,ILLUSTRATION!! ***************************** 195 A is in a 12-min cadence again ***************************** Several impulsive M flares ***************************** 9 - Interesting/outstanding chains 10 - Interesting/outstanding chains Diagnostics of electron beam properties from the simultaneous hard X-ray and microwave emission in the 10 March 2001 flare V.V. Zharkova1, N.S. Meshalkina2, L.K. Kashapova2, A.A. Kuznetsov3,2, A.T. Altyntsev E-print May, 2011; A&A 532, A17 (2011) Seismic Emissions from a Highly Impulsive M6.7 Solar Flare J.C. Martnez-Oliveros, H. Moradi, A-C. Donea E-print, Jan 2008. http://www.clique.monash.edu.au/SoPh_Martinez2.pdf Energetics and Dynamics of an Impulsive Flare on March 10, 2001 Ramesh Chandra , Rajmal Jain2 et al. Solar Phys, 239(1-2), 239-256, 2006 Broadband Microwave Burst Produced by Electron Beams A.T. Altyntsev, G.D. Fleishman, G.-L. Huang and V.F. Melnikov BBSO, #1357, 2008 http://solar.njit.edu/preprints/altyntsev1357.pdf 11 - Interesting/outstanding chains; polar N CH and associated chain !!! 12 - Interesting/outstanding chains ~0 UT: a half of large NE CME ~18 UT: significant E eruption and CME; simultaneously SW eruption and CME 13 - Interesting/outstanding chains 14 - Interesting/outstanding chains +15 - !! 21:30 UT: A spectacular central eruption, E2 coronal wave Slow W halo, Outstanding chains!! ILLUSTRATION A filament eruption occurred near region 9384 and was in progress by 21:13 UT according to LASCO EIT images. The eruption is likely to have produced a geoeffective CME. 16 - Interesting/outstanding chains; Several eruptions LASCO, ~16 UT: clear concave feature !! +17 - Interesting/outstanding chains; Several eruptions, including NW limb filament at the evening ++!!11:30-11:50 UT: several type II-like bands (or large chains)!! +18 - Interesting/outstanding chains; several eruptions and two CMEs +NOBE, ~03 UT: SE over-the-limb eruption with clear displacement along the limb; CME-associated!!! Simultaneous NW over-the-limb filament eruption and CME! ++ !!08:50 UT: our type II burst, disk (SW) eruption, coronal wave, chains!! 19 - Interesting/outstanding chains; Eruptions 04-05 UT halo 360 389 S20W01 n Эрупция небольшого центрального волокна недалеко от АО. Два димминга на 195 А. Протяженные аркада и ленты (304 А). Events. The Solar Connection of Enhanced Heavy Ion Charge States in the Interplanetary Medium: Implications for the Flux-rope Structure of CMEs N. Gopalswamy, P. Makela, S. Akiyama, H. Xie, S. Yashiro, and A. A. Reinard Solar Physics, 2013, File ******** 19d-20d - Forbush ~3 % and Severe Geomagnetic Storm Dst~ -152 nT Characterization of the Complex Ejecta Measured In Situon 19?–?22 March 2001 by Six Different Methods Arian Ojeda-Gonzalez, Virginia Klausner, Odim Mendes, Margarete Oliveira Domingues, Alan Prestes Solar Physics November 2017, 292:160 The Interaction of Successive Coronal Mass Ejections: A Review Noe Lugaz Manuela Temmer Yuming Wang Charles J. Farrugia Sol Phys (2017) 292: 64. File http://sci-hub.cc/10.1007/s11207-017-1091-6 ******** 20 - Interesting/outstanding chains 21 - Interesting/outstanding chains A STUDY OF FLARE-ASSOCIATED X-RAY PLASMA EJECTIONS. I. ASSOCIATION WITH CORONAL MASS EJECTIONS Yeon-Han Kim,1, 2 Y.-J. Moon,1 K.-S. Cho,1 Kap-Sung Kim,2 and Y. D. Park ApJ 622 :1240–1250, 2005 File +22 - !04 UT: SW filament eruption (NOBE) and CME! !08:20 UT: Our clear type II burst associated with an impulsive M2 flare! Interesting/outstanding chains; CH 23 - Interesting/outstanding chains; CH 24 - Interesting/outstanding chains; CH; Noise storm CME Interaction with Coronal Holes and their Interplanetary Consequences N. Gopalswamy1, P. Makela1,2, H. Xie1,2, S. Akiyama1,2, and S. Yashiro1,2 JGR, 2009; File; J. Geophys. Res., Vol. 114, No. A3, A00A22 ************* !!! 24 - 2?: HIGH ACTIVITY and INTENSE NOISE STORM !!! ************* 25 - Interesting/outstanding chains; CH; Noise storm 11:20 UT: interesting type IIIGG 17 UT: NE eruption and halo CME (faint) Statistical properties of radio flux densities of solar flares Wang Lu, Liu Si-ming, Ning Zong-jun Research in Astronomy and Astrophysics 2020 https://arxiv.org/pdf/2006.02121.pdf 26 - Interesting/outstanding chains; CH; Noise storm Several eruptions; ~17 UT Mar 26 - 03 Apr 2001 On flare predictability based on sunspot group evolution Marianna Korsos, Andras Ludmany, Robert Erdelyi, Tunde Baranyi 2015 http://arxiv.org/pdf/1503.04634v1.pdf 26 March-26 Apr The Interaction of Successive Coronal Mass Ejections: A Review Noe Lugaz Manuela Temmer Yuming Wang Charles J. Farrugia Sol Phys (2017) 292: 64. File http://sci-hub.cc/10.1007/s11207-017-1091-6 27 - Interesting/outstanding chains; CH; Noise storm !!Large FORBUSH!! SOLAR TYPE II RADIO BURSTS AND IP TYPE II EVENTS H. V. Cane and W. C. Erickson Astrophysical Journal, 623:1180–1194, 2005; File +28 - Interesting/outstanding chains; CH; Noise storm !!11:20 UT: our event; eruption from S and N regions; S halo CME !!! Pre-Flare Dynamics of Sunspot Groups M. B. Korsos, T. Baranyi, A. Ludmany 2014 http://arxiv.org/pdf/1405.7485v1.pdf Solar and interplanetary triggers of the largest Dst variations of the solar cycle 23 Y. Cerrato, E. Saiz, C. Cid, , , W.D. Gonzalez, J. Palacios Journal of Atmospheric and Solar-Terrestrial Physics, Voume 80, May 2012, Pages 111–123, File Three-dimensional MHD simulation of two coronal mass ejections' propagation and interaction using a successive magnetized plasma blobs model Shen, F.; Feng, X. S.; Wang, Yuming; Wu, S. T.; Song, W. B.; Guo, J. P.; Zhou, Y. F. J. Geophys. Res., Vol. 116, No. A9, A09103, 2011 Magnetic Properties of Metric Noise Storms Associated with Coronal Mass Ejections ? Ya-Yuan Wen, Jing-Xiu Wang and Yu-Zong Zhang Chin. J. Astron. Astrophys. Vol. 7 (2007), No. 2, 265–280, File !!++29 - !!!10:14 UT: our X1.7 and powerful microwace flare; type II burst (?); halo CME; See Events !!! see TRACE NOISE storm (weakening) Sourse of Severe magnetic storm, Dst~-377 nT Characteristics of Radio-Loud CMEs Pankaj Kumar, P.K. Manoharan, K.S. Cho 2017 https://www.researchgate.net/publication/315637846_Characteristics_of_radio-loud_CMEs Solar and interplanetary triggers of the largest Dst variations of the solar cycle 23 Y. Cerrato, E. Saiz, C. Cid, , , W.D. Gonzalez, J. Palacios Journal of Atmospheric and Solar-Terrestrial Physics, Voume 80, May 2012, Pages 111–123, File Speed Evolution of Fast CME/Shocks: Analysis of Kilometric Type II Emissions J. A. Gonzalez-Esparza and E. Aguilar-Rodriguez Ann. Geophys., 27, 3957-3966, 2009, File JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 111, A11104, 2006 A two-ejecta event associated with a two-step geomagnetic storm C. J. Farrugia et al. 28-31 Acceleration and deceleration of coronal mass ejections during propagation and interaction Shen, F., S. T. Wu, X. Feng, and C.-C. Wu J. Geophys. Res., 117, A11101, doi:10.1029/2012JA017776, 2012 30 - Interesting/outstanding chains; NOISE storm 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 Microwave Type III-Like Bursts as Possible Signatures of Magnetic Reconnection A. T. Altyntsev, V. V. Grechnev, N. S. Meshalkina, Y. Yan Solar Phys., 242(1-2), Page: 111 – 123, 2007. Predicting the occurrence of super-storms N. Srivastava Annales Geophysicae, 23, 2989–2995, 2005, File 30-31 A scheme for forecasting severe space weather N. Balan, Y. Ebihara,R. Skoug,K. Shiokawa,I. S. Batista,S. Tulasi Ram,Y. Omura,T. Nakamura, M.-C. Fok JGR 2017 DOI: 10.1002/2016JA023853 http://sci-hub.cc/doi/10.1002/2016JA023853 +31 - !!Severe magnetic storm, Dst~-377 nT!! !!!~11:30 UT: our unusual type II burst (questionable!) Should be verified NW activity (?) and Large SE CME Interesting/outstanding chains; NOISE storm Sun-Earth connection Event of Super Geomagnetic Storm on March 31, 2001: the Importance of Solar Wind Density Li-Bin Cheng, Gui-Ming Le, Ming-Xian Zhao Research in Astronomy and Astrophysics 2019 https://arxiv.org/pdf/1910.07932.pdf CME front and severe space weather N. Balan1,2,6,*, R. Skoug3, S. Tulasi Ram4, P. K. Rajesh2, K. Shiokawa1, Y. Otsuka1, I. S. Batista5, Y. Ebihara6 andT. Nakamura7 JGR, 2014 http://onlinelibrary.wiley.com/doi/10.1002/2014JA020151/pdf Solar and interplanetary triggers of the largest Dst variations of the solar cycle 23 Y. Cerrato, E. Saiz, C. Cid, , , W.D. Gonzalez, J. Palacios Journal of Atmospheric and Solar-Terrestrial Physics, Voume 80, May 2012, Pages 111–123, File