January 2003 1 - Low activity; Interesting chains; CH 2 - Low activity; Interesting chains; CH +3 - Low activity; Interesting chains; CH +10-14 UT: NW filament eruption and CMEs; dimmings at 304 A(!!); SEE EVENTS Spatial Offsets in Flare-CME Current Sheets John C. Raymond, Silvio Giordano, Angela Ciaravella 2017 https://arxiv.org/pdf/1706.03090.pdf 4 - Low activity; Interesting chains; CH ++5 - Low flare activity; Interesting chains; CH +07:25 UT: +faint, but fast-drifting type II burst at our spectrum; See Events +10 UT: NE filament eruption; strong dimmings; SEE EVENTS!!! +one more faint, but fast-drifting type II burst at our spectrum A STUDY OF FAST FLARELESS CORONAL MASS EJECTIONS H. Q. Song1,2, Y. Chen1, D. D. Ye1, G. Q. Han1, G. H. Du1, G. Li1,3, J. Zhang2, and Q. Hu 2013 ApJ 773 129, File 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 ++6 - Low flare activity; Interesting chains; CH; Several eruptions +11 UT: SE eruption, 3-4-line dimmings; large CME, SEE EVENTS; Similar to 7d ++7 - Interesting chains; CH +07:50 UT: SE M1 flare, eruption, 3-4-line dimmings; SEE EVENTS; Similar to 7d RESIK SOLAR X-RAY FLARE ELEMENT ABUNDANCES ON A NON-ISOTHERMAL ASSUMPTION B. Sylwester, K. J. H. Phillips, J. Sylwester, A.. Kepa ApJ 2015 http://arxiv.org/pdf/1503.00979.pdf Diagnostics of non-thermal distributions in solar flare spectra observed by RESIK and RHESSI? A. Kulinova1,2, J. Kasparova1, E. Dzifcakova1, J. Sylwester3, B. Sylwester3 and M. Karlicky A&A 533, A81 (2011) +8 - Interesting chains; CH +07 UT: central and S eruption; dimmings; See Events 9 - Interesting chains; CH 02 UT: SW eruption Several SE eruptions 10 - Interesting NOBE chains; CH 02:30 and 03:30 UT: SW eruption 13 UT: SE-limb eruption 11 - Interesting NOBE chains; CH 01 UT: SW eruption 10 UT: SW eruption 17:24 UT: SW eruption 20:30 SW eruption +12 - Interesting NOBE chains; CH +08:30 UT: our IIIGG with low-frequency positive-drifting band, similar to event of 20.12.2002 +strong displacement of NE narrow coronal stream +13 - Interesting NOBE chains; CH +13:30: NE-limb eruption; See events MAGNETIC ENERGY AND HELICITY BUDGETS IN THE ACTIVE-REGION SOLAR CORONA. II. NONLINEAR FORCE-FREE APPROXIMATION Manolis K. Georgoulis1,3, Kostas Tziotziou1, and Nour-Eddine Raouafi 2012 ApJ 759 +14 - Interesting NOBE chains; CH +>16 UT: strong central eruption; See Events 15 - Interesting NOBE chains; CH 16 - Interesting NOBE chains; CH 01 UT: NE and SW eruptions ******************** 17-24 - Several significant eruptions, CMEs, (impulsive) flares. Should be analysed ******************** ++17 - Interesting NOBE chains; CH ++02 UT: strong central eruption with clear canalized dimmings; See Events 18 - 07 UT: NE eruption +20 - >13 UT: large NW filament eruption, See Events! >20 UT: large NE filament eruption; See Events ENDPOINT BRIGHTENINGS IN ERUPTING FILAMENTS Y.-M. Wang1, K. Muglach1,2, and B. Kliem Astrophysical Journal, 699:133–142, 2009, File 21 - >00 UT: continuation of NE filament posteruption; >05 UT: N filament eruption; >13:25 UT: large E-limb eruption; On the Application of Differential Evolution to the Analysis of X-Ray Spectra Anna Kepa, Barbara Sylwester, Marek Siarkowski, Janusz Sylwester ApJ 2022 https://arxiv.org/pdf/2202.09302.pdf 21-26 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 +22 - >02 UT: NE over-limb arcade following by N on-disk eruption; See Events ++23 - Interesting chains and CH ++04:48 UT: global E-hemisphere eruption with long absorption chain (canalized) dimming along a CH boundary; SEE EVENTS!! ++13:13 UT: one more eruption with CH boundary evolution; SEE EVENTS!! ++>21 UT: significant brigtening (chain) and 4-line dimming (See 29.04.98); near a CH, CH boundary evolution before a large eruption of 24d; SEE EVENTS!! ++24 - Interesting chains and CH ++03 UT: significant central eruption, with long absorption chain (canalized) dimming along a CH boundary; partial halo CME; SEE EVENTS!! +25 - 19 UT: NE eruption with canalized dimmings and coronal wave; See Events ******************* Nearest days: several filament eruptions with 4-line dimmings, canalized, propagating along the filament!!! ******************* ++27 - Interesting chains and CH ++06 UT: significant NE eruption accompanied by a propagating canalized 4-line dimming with a frontal bright blob; See EVENTS!! +19 UT: significant SW eruption with a clear 4-line canalized dimming along a polar CH boundary; partial halo CME; See Events!! Radio-loud CMEs from the disk center lacking shocks at 1 AU N. Gopalswamy, P. Makela, S. Akiyama, S. Yashiro, H. Xie, R. J. MacDowall, M. L. Kaiser E-print, June 2012, JGR, 117, A08106, 2012 CONSTRAINTS ON CORONAL MASS EJECTION EVOLUTION FROM IN SITU OBSERVATIONS OF IONIC CHARGE STATES Jacob R. Gruesbeck1, Susan T. Lepri1, Thomas H. Zurbuchen1, and Spiro K. Antiochos2 Astrophysical Journal, 730:103 (9pp), 2011 April; File ++29 - +Interesting chains and CH! Illustration ++02:30 UT: central (filament) eruption with similar canalized dimmings at 195 and 304 A (e1,3 - no data); See Events!! ++30 - +Interesting chains and CH! Illustration ++06:30 UT: significant central filament eruption with 4-line dimmings, canalized, propagating; See Events +31 - +Interesting chains and CH! Illustration >22 UT: partial halo (see 1 Feb).