August 2004 1 - ~07 UT: Huge NW-limb prominense at 304 A; 3- filament Solar Physics (2006) 234: 115–134 IMAGING SPECTROSCOPY OF A SOLAR FILAMENT USING A TUNABLE H? FILTER JONGCHUL CHAE et al. 4 Solar Magnetic Flux Ropes Review Boris Filippov, Olesya Martsenyuk, Abhishek K. Srivastava, and Wahab Uddin Journal of Astrophysics & Astronomy, 2015 http://arxiv.org/ftp/arxiv/papers/1501/1501.02562.pdf 8 - A bright full halo CME was observed in LASCO C3 images starting at 09:42 UTC. The leading front was first observed off of the east limb and the south pole. The source of this event was likely about 5-6 days behind the southeast limb. 9 - ~13 UT: Huge SW-limb prominense at 304 A; ****************************************************************** 10 - ??: Many long collimated eruptions (as at the previous rotation) ****************************************************************** +10 - >14 UT: collimated northward eruption; faint but large SW/S CME; See Events! +11 - >22 UT: eruption and propagating brightening; See Events! ÄÈÍÀÌÈÊÀ ÌÀÃÍÈÒÍÎÃÎ ÏÎËß ÀÊÒÈÂÍÛÕ ÎÁËÀÑÒÅÉ Â ÏÐÅÄÂÑÏÛØÅ×ÍÎÌ ÑÎÑÒÎßÍÈÈ È ÂÎ ÂÐÅÌß ÑÎËÍÅ×ÍÛÕ ÂÑÏÛØÅÊ ÏÎÄÃÎÐÍÛÉ À.È.1, ÏÎÄÃÎÐÍÛÉ È.Ì.2, ÌÅØÀËÊÈÍÀ Í.Ñ. ÀÆ Òîì: 92 Íîìåð: 8 Ãîä: 2015 Ñòðàíèöû: 669 13 - Many quasi-impulsive flares and collimated eruptions Hard X-ray Emission During Flares and Photospheric Field Changes O. Burtseva, J. C. Martinez-Oliveros, G. J. D. Petrie, A. A. Pevtsov ApJ 2015 http://arxiv.org/pdf/1505.00509v1.pdf August 13-15: Several small CMEs were observed over the south pole, the southwest limb and the central west limb after flare activity in region 10656. Extreme-ultraviolet and hard X-ray signatures of electron acceleration during the failed eruption of a filament A. Netzel, T. Mrozek, S. Kolomanski, and S. Gburek E-print, Dec 2012; A&A 548, A89, 2012; File 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 +14 - Many quasi-impulsive flares and collimated eruptions +15:48 UT: 2N/M7 flare and eruption; See Events! Detection of Energy Cutoffs in Flare-accelerated Electrons Fanxiaoyu Xia1,2, Yang Su1,2, Wen Wang3, Linghua Wang3, Alexander Warmuth4, Weiqun Gan1,2, and Youping Li1,2 2021 ApJ 908 111 https://iopscience.iop.org/article/10.3847/1538-4357/abce5c/pdf Study of temporal and spectral characteristics of the X-ray emission from solar flares Veena Choithani, Rajmal Jain, Arun Kumar Awasthi, Geetanjali Singh, Sneha Chaudhari, Som Kumar Sharma Research in Astronomy and Astrophysics (RAA) 2018 https://arxiv.org/pdf/1804.08431.pdf The structure of solar radio noise storms Claude Mercier, Prasad Subramanian, Gilbert Chambe, P. Janardhan A&A, 2015 http://arxiv.org/pdf/1412.8189v2.pdf Energy-Dependent Timing of Thermal Emission in Solar Flares Rajmal Jain, Arun Kumar Awasthi, Arvind Singh Rajpurohit and Markus J. Aschwanden Solar Physics, Volume 270, Number 1, 137-149, 2011 Fig. 5 MASS COMPOSITION IN PRE-ERUPTION QUIET SUN FILAMENTS Gary Kilper1, Holly Gilbert1,2, and David Alexander1 The Astrophysical Journal, 704:522–530, 2009 October From GHz to mHz: AMultiwavelength Study of the Acoustically Active 14 August 2004 M7.4 Solar Flare J.C. Mart´ýnez-Oliveros1, H. Moradi1, D. Besliu-Ionescu1,2, A.-C Donea1, P.S. Cally1, C. Lindsey3 E-print, July 2004 sun quake 15 - Many quasi-impulsive flares andcollimated eruptions August 16: A full halo CME was observed beginning at 15:18 in LASCO C3 images. The source of this event was likely a few days behind the west limb. ++17 - 04:30 UT: NOBE SE filament eruption; 4-line dimmings; See Event!!! A full halo CME was observed in LASCO C3 images starting at 07:42 UT. Most of the ejected material was observed over the southeast limb, faint extensions were noted at the west limbs. The source of this CME was a fairly large filament eruption to the south and southeast of region 10661. This eruption began around 04h UT and peaked near 06h UT. ++18 - +10:50 UT: Spectacular type II burst at our spectrum from E/central eruption; See Events!! +17:40 UT: SW-limb X2 flare and large CME; See Events!! RHESSI AND TRACE OBSERVATIONS OF MULTIPLE FLARE ACTIVITY IN AR 10656 AND ASSOCIATED FILAMENT ERUPTION Bhuwan Joshi1, Upendra Kushwaha1, K.-S. Cho2, and Astrid M. Veronig 2013 ApJ 771 1 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 A Coronal Mass Ejection and Hard X-Ray Emissions Associated with the Kink Instability Kyung-Suk Cho, Jeongwoo Lee, Su-Chan Bong, Yeon-Han Kim, Bhuwan Joshi and Young-Deuk Park BBSO preprint #1400, June 2009 A Study of CME and Type II Shock Kinematics Based on Coronal Density Measurement K.-S. Cho, J. Lee, Y.-J. Moon, M. Dryer, S.-C. Bong, Y.-H. Kim and Y.D. Park Link: http://solar.njit.edu/preprints/lee1316.pdf MAGNETIC FIELD STRENGTH IN THE SOLAR CORONA FROM TYPE II BAND SPLITTING K.-S. Cho,1,2 J. Lee,2 D. E. Gary,2 Y.-J. Moon,1 and Y. D. Park1 E-print, June 2007, File, Astrophysical Journal, 665: 19 - Region 10656 behind the southwest limb continued to be active and produced several flares: M3.0 at 07:01; M2.1 at 13:51 19-24 Aug Evidence of Twisted Flux-Tube Emergence in Active Regions M. Poisson, C. H. Mandrini, P. Demoulin, M. Lopez Fuentes Solar Physics March 2015, Volume 290, Issue 3, pp 727-751 http://arxiv.org/pdf/1505.01805v1.pdf 24 Aug Good type II spectrum Fine structures of solar radio bursts: origins and radio-wave propagation effects Nicolina Chrysaphi PhD Thesis, University of Glasgow, 2021. https://arxiv.org/pdf/2103.13745.pdf 30 Aug Magnetic field-line lengths inside interplanetary magnetic flux ropes Qiang Hu, Jiong Qiu, Sam Krucker JGR Special Section: VarSITI, 2015 http://arxiv.org/pdf/1502.05284v1.pdf 31 Aug Coronal hard X-ray sources revisited Brian R. Dennis, Miguel A. Duval-Poo, Michele Piana, Andrew R. Inglis, A. Gordon Emslie, Jingnan Guo, Yan Xu ApJ 2018 https://arxiv.org/pdf/1809.04631.pdf Solar hard X-ray imaging by means of compressed sensing and finite isotropic wavelet transform M. A. Duval-Poo1, M. Piana1,2 and A. M. Massone2 A&A 615, A59 (2018) https://www.aanda.org/articles/aa/pdf/2018/07/aa31765-17.pdf