September 2002 1 - EIT: brake out !>05 UT: large, slow W CME Good noise storm spectrum 2 - Noise storm 3- Narrow FD 4- Low activity; +Strong NS at our spectrum Dst=-109 nT Dependence of Great Geomagnetic Storm (?SYM-H??200) on Associated Solar Wind Parameters Ming-Xian Zhao, Gui-Ming Le, Qi Li, Gui-Ang Liu & Tian Mao Solar Physics volume 296, Article number: 66 (2021) https://link.springer.com/content/pdf/10.1007/s11207-021-01816-2.pdf https://doi.org/10.1007/s11207-021-01816-2 +5 - +16:20 UT: good filament eruption; C5.2, clear canalized dimmings; halo CME; See Events! The Wind/EPACT proton event catalog (1996-2016) Rositsa Miteva, Susan W. Samwel, Marcus V. Costa-Duarte Solar Phys. 2018 https://arxiv.org/pdf/1801.00469.pdf File +6 - 01 UT: SW filament eruption; +13:30 UT: large over-W-limb CME followed by W activity and dimmings; See Events! Effect of the Weakened Heliosphere in Solar Cycle 24 on the Properties of Coronal Mass Ejections N. Gopalswamy, S. Akiyama, S. Yashiro, G. Michalek, H. Xie, P. Makela Proc. 19th International Astrophysics Conference held in Santa Fe, New Mexico, March 9 - 13, 2020 https://arxiv.org/ftp/arxiv/papers/2007/2007.08291.pdf 7 - CH; Dst=-181 nT from halo CME of 5d Large Forbush Decreases and their Solar Sources: Features and Characteristics M. Papailiou, M. Abunina, A. Belov, E. Eroshenko, V. Yanke & H. Mavromichalaki Solar Physics volume 295, Article number: 164 (2020) https://link.springer.com/content/pdf/10.1007/s11207-020-01735-8.pdf Comparison of ICME arrival times and solar wind parameters based on the WSA-ENLIL model with three cone types and observations† Soojeong Jang, Y.-J. Moon*, Jae-Ok Lee and Hyeonock Na JGR, Volume 119, Issue 9, pages 7120–7127, 2014 Coronal Mass Ejections from the Sun - Propagation and Near Earth Effects Arun Babu THESIS, 2014 http://arxiv.org/pdf/1407.4258v1.pdf High rigidity Forbush decreases: due to CMEs or shocks? Arun Babu, H. M. Antia, S. R. Dugad, S. K. Gupta, Y. Hayashi, S. Kawakami, P. K. Mohanty, T. Nonaka, A. Oshima, P. Subramanian E-print, April 2013; A&A http://arxiv.org/abs/1304.5343 Precursor Effects in Different Cases of Forbush Decreases M. Papailiou • H. Mavromichalaki • A. Belov • E. Eroshenko • V. Yanke Solar Phys (2012) 276:337–350, File ---------------------------------------- 8-18 - Nobe: global filament and chains ---------------------------------------- 8 - 14 UT: large SE-limb eruption 9 - 17 UT: M2 impulse Dimensionality of Solar Magnetic Reconnection Review Jeongwoo Lee Reviews of Modern Plasma Physics 2022 https://link.springer.com/epdf/10.1007/s41614-022-00096-y https://doi.org/10.1007/s41614-022-00096-y CORONAL THICK TARGET HARD X-RAY EMISSIONS AND RADIO EMISSIONS Jeongwoo Lee1,2, Daye Lim2, G. S. Choe2, Kap-Sung Kim2, and Minhwan Jang 2013 ApJ 769 L11 EARLY ABNORMAL TEMPERATURE STRUCTURE OF X-RAY LOOP-TOP SOURCE OF SOLAR FLARES Jinhua Shen,1,2 Tuanhui Zhou,2 Haisheng Ji,2,3 Na Wang,1 Wenda Cao,3 and Haimin Wang3 Astrophysical Journal, 686: L37–L40, 2008 October http://www.journals.uchicago.edu/doi/pdf/10.1086/592835 Radio, Hard X-Ray, EUV and Optical Study of September 9, 2002 Solar Flare Guangli Huang1 and Ji Haisheng1 Astrophysics and Space Science V. 301, No. 1-4, p. 65-71, 2006 Magnetic Energy Release During the 2002 September 9 Solar Flare Authors: Jeongwoo Lee, Dale E. Gary and G.S. Choe Link: http://solar.njit.edu/preprints/lee1317.pdf 10- Constraints on energy release in solar flares from RHESSI and GOES X-ray observations I. Physical parameters and scalings A. Warmuth and G. Mann A&A 588, A115 (2016) http://www.aanda.org/articles/aa/pdf/2016/04/aa27474-15.pdf Long-Period Oscillations of Sunspots Observed by SOHO/MDI V. I. Efremov, L. D. Parfinenko, A. A. Solov’ev, E. A. Kirichek Solar Physics, June 2014, Volume 289, Issue 6, pp 1983-1998 http://arxiv.org/ftp/arxiv/papers/1412/1412.4107.pdf A Burst with Double Radio Spectrum Observed up to 212 GHz C. G. Gimenez de Castro, G. D. Cristiani, P. J. A. Simoes, C. H. Mandrini, E. Correia, P. Kaufmann Solar Physics, June 2013, Volume 284, Issue 2, pp 541-558 Measurements of Electron Anisotropy in Solar Flares Using Albedo with RHESSI X-Ray Data E. C. M. Dickson, E. P. Kontar Solar Physics, June 2013, Volume 284, Issue 2, pp 405-425 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 Speed Distributions of Merging X-Ray Sources During Chromospheric Evaporation in Solar Flares Zongjun Ning Solar Physics, Volume 273, Number 1, 81-92, 2011 11 - >08 UT: NW filament eruption near a CH 17 UT: unusual S/SE eruption Recent Results on the Fine Structure in Cosmic Radio Emission Book Zebra Pattern in Solar and Pulsar Radio Emission G.P. Chernov, V. Fomichev, S. Fainshtein LAP LAMBERT Academic Publishing 2021 File Solar 3.04 cm hydrogen line emission revealed in observations of the active region NOAA 10105 N. G. Peterova, N. A. Topchilo & T. P. Borisevich Astronomy Reports, Volume 55, Number 9, 841-848, 2011 Astronomicheskii Zhurnal, 2011, Vol. 88, No. 9, pp. 912–919 +12 - 04:48, 07:14, 20:00 UT: SE eruptions; See Events! +13 - 07 UT: NS weakening at low frequencies Reduced Coronal Emission above Large Isolated Sunspots B. I. Ryabov, D. E. Gary, N. G. Peterova, K. Shibasaki, and N. A. Topchilo Solar Phys., 2014 http://www.ltn.lv/~ryabov/paper_1.pdf +15 - 19 UT: large NE-limb filament eruption and transient chain (ribbon) on the disk; See Events! ENDPOINT BRIGHTENINGS IN ERUPTING FILAMENTS Y.-M. Wang1, K. Muglach1,2, and B. Kliem Astrophysical Journal, 699:133–142, 2009, File +16 - 03 UT: large SW eruption; See Events! Good stable NS Analysis of SolarWind Events Using Interplanetary Scintillation Remote Sensing 3D Reconstructions and Their Comparison at Mars B.V. Jackson • J.A. Boyer • P.P. Hick • A. Buffington • M.M. Bisi • D.H. Crider Solar Phys (2007) 241: 385–396 +17 - Outstanding chains; illustration; CH +07 UT: SW eruption, C8 LDE; halo CME, canalized dimmings on and over the limb; See Events !Our event: Drifting onset of the Noise storm; Strong type III groups with probable type II burst. Last news on zebra pattern Gennady Chernov Solar Phys. 2016 http://arxiv.org/ftp/arxiv/papers/1512/1512.06311.pdf Radioheliograph Observations of Microwave Bursts with Zebra Structures A. T. Altyntsev, S. V. Lesovoi, N. S. Meshalkina, R. A. Sych and Y. Yan Solar Physics, Volume 273, Number 1, 163-177, 2011 Quadrupolar Dimmings During a Partial Halo Coronal Mass Ejection Event J. Yang, Y. Jiang, R. Zheng, J. Hong, Y. Bi and L. Yang Solar Physics, Volume 270, Number 2, 551-559, 2011 Coronal Mass Ejections, Type II Radio Bursts, and Solar Energetic Particle Events in the SOHO Era N. Gopalswamy1, S. Yashiro2, S. Akiyama2, P. Makela2, H. Xie2, M. L. Kaiser1, R. A. Howard3 and J. L. Bougeret4 E-print, Feb 2008, File; Annales Geophysicae 26, 3033–3047, 2008. sci-hub.tw/10.5194/angeo-26-3033-2008 https://www.ann-geophys.net/26/3033/2008/angeo-26-3033-2008.pdf +18 - Outstanding chains; illustration; CH Our compressed spectrum is simular to 17d, Noise storm Probing Coronal Magnetic Fields with Sungrazing Comets: H i Ly? from Pickup Ions J. C. Raymond1 and S. Giordano2 2019 ApJ 887 45 sci-hub.se/10.3847/1538-4357/ab4e95 Probing the Solar Wind Acceleration Region with the Sun--Grazing Comet C/2002 S2 Silvio Giordano, John C. Raymond, Philippe Lamy, Michael Uzzo, Danuta Dobrzycka ApJ, 2014 http://arxiv.org/pdf/1411.1300v1.pdf +19 - 05:12 UT: large E-limb eruption and CME; See Events! Noise storm ----------------------------------------------------------------------- Noise storm evolution at our and AIP spectra for this period is a subject for analysis ----------------------------------------------------------------------- +20 - 05 UT: slow SE eruption and large CME +Evolving noise storm 19:48 UT: SW EUV jet RESIK and RHESSI observations of the 20 September 2002 flare A. Kepa, R. Falewicz, M. Siarkowski, M. Pietras A&A 2020 https://arxiv.org/pdf/2008.05755.pdf 2D MHD and 1D HD models of a solar flare -- a comprehensive comparison of the results R. Falewicz, P. Rudawy, K. Murawski, A. K. Srivastava ApJ 2015 http://arxiv.org/pdf/1510.00254v1.pdf The spatial, spectral and polarization properties of solar flare X-ray sources Natasha L. S. Jeffrey Ph.D. Thesis, 2014 http://arxiv.org/pdf/1412.8163v1.pdf 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 PLASMA HEATING IN THE VERY EARLY AND DECAY PHASES OF SOLAR FLARES R. Falewicz1, M. Siarkowski2 and P. Rudawy 2011 ApJ 733 37 Plasma heating in the initial phase of solar flares P. Rudawy1, M. Siarkowski2 and R. Falewicz1 Solar and Stellar Variability: Impact on Earth and Planets, Proceedings IAU Symposium No. 264, 2009, p. 282-284, A.G. Kosovichev, A.H. Andrei & J.-P. Rozelot, eds. Y:\obridko\otchet09 PLASMA HEATING IN THE VERY EARLY PHASE OF SOLAR FLARES M. Siarkowski1, R. Falewicz2, and P. Rudawy2 The Astrophysical Journal, 705:L143–L147, 2009 +21 - Low activity, Nobe chains +Evolving noise storm, slow drifting enhancement at ~10 UT +22 - Low activity, Nobe chains +Evolving noise storm, slow drifting enhancement and sharp stop at ~10 UT; Comp with AIP +10 UT: NW filament eruption, See Events! The injection of ten electron/3He-rich SEP events Linghua Wang1, Sam Krucker2,3, Glenn M. Mason4, Robert P. Lin2 and Gang Li A&A 585, A119 (2016) http://arxiv.org/pdf/1605.07882v1.pdf 23 - Low activity, Nobe chains 24 - Low activity, Nobe chains The injection of ten electron/3He-rich SEP events Linghua Wang1, Sam Krucker2,3, Glenn M. Mason4, Robert P. Lin2 and Gang Li A&A 585, A119 (2016) http://arxiv.org/pdf/1605.07882v1.pdf 25 - Low activity 26 - Low activity 27 - Several not too large eruptions, CH 03 and 12:30 UT: Near and over the limb; See Events 07UT: SW filament eruption 28 - EUV chain inside a polar CH 29 - EUV chain inside a polar CH +06:30 UT: impulsive M2 flare; See Events Fitting and Reconstruction of Thirteen Simple Coronal Mass Ejections Nada Al-Haddad, Teresa Nieves-Chinchilla, Neel P. Savani, Noe Lugaz, Ilia I. Roussev Solar Phys. 2018 https://arxiv.org/pdf/1804.02359.pdf 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 ON THE RELATIONSHIP BETWEEN THE CORONAL MAGNETIC DECAY INDEX AND CORONAL MASS EJECTION SPEED Yan Xu, Chang Liu, Ju Jing, and Haimin Wang 2012 ApJ 761 52 Alena Kulinova, Elena Dzifcakova, Rastislav Bujnak, Marian Karlicky Multi-Wavelength Analysis of the 29 September 2002 M2.6/2N Flare. Solar Physics, 221 (1): 101-119, May 2004 23:30 UT: onset of the large central filament eruption! See Events! Ding. H-Alpha and Hard X-Ray Observations of a Two-Ribbon Flare Associated with a Filament Eruption. The Astrophysical Journal, Volume 598, Issue 1, pp. 683-688. http://solar.physics.montana.edu/cgi-bin/eprint/index.pl?entry=659 +30 - >00 UT: contimuation of the large central filament eruption! See Events! +07:06 UT: short and narrow-band, but intense type II burst, associated with NW-limb eruption and dimming; See Events! Flux erosion of magnetic clouds by reconnection with the Sun's open flux Sanchita Pal, Soumyaranjan Dash, Dibyendu Nandy Geophysical Research Letters,47, Issue 8, e2019GL086372, 2020 https://arxiv.org/pdf/2103.05990.pdf https://doi.org/10.1029/2019GL086372 High rigidity Forbush decreases: due to CMEs or shocks? Arun Babu, H. M. Antia, S. R. Dugad, S. K. Gupta, Y. Hayashi, S. Kawakami, P. K. Mohanty, T. Nonaka, A. Oshima, P. Subramanian E-print, April 2013; A&A http://arxiv.org/abs/1304.5343 Q. R. Chen, M. D. Ding Footpoint Motion of the Continuum Emission in the 2002 September 30 White-Light Flare. E-print, 21.12.2005 Sep 30-Oct 01 The effect of magnetic field line topology on ICME-related GCR modulation Emma E. Davies (1 and 2), Camilla Scolini (1), Reka M. Winslow (1), Andrew P. Jordan (1), Christian Mostl (2) ApJ 2023 https://arxiv.org/pdf/2310.11310.pdf