June 2002 --------------------------------------------- !! 01d-05d High (7 min) cadence at 195 A !! --------------------------------------------- 1 - Interesting/outstanding chains; Illustration Several eruptions Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. I. Reconciliation of “EIT Waves”, Type II Radio Bursts, and Leading Edges of CMEs V. V. Grechnev, A. M. Uralov, I. M. Chertok, I. V. Kuzmenko, A. N. Afanasyev, N. S. Meshalkina, S. S. Kalashnikov and Y. Kubo Solar Physics, Volume 273, Number 2, 433-460, 2011, File in Chertok’s papers Grechnev, FIAN-09 Meshalkina et al., направлена в PASJ (cм. презентацию Grechnev IKI-09) Eruptions of Magnetic Ropes in Two Homologous Solar Events of 2002 +2 - Interesting/outstanding chains; ILLUSTRATION Several eruptions +10:17 UT: our fragmentary type II burst (3 harmonics?); See Events 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 Return-current Model Spectra and Enhanced Plasma Resistivity Meriem Alaoui and Gordon Holman RHESSI Science Nuggets #259 August, 2015 http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Return-current_Model_Spectra_and_Enhanced_Plasma_Resistivity Negative bursts Grechnev et al., PASJ, 2013 Nonthermal X-Ray Spectral Flattening toward Low Energies in Early Impulsive Flares Sui, Linhui; Holman, Gordon D.; Dennis, Brian R. Astrophysical Journal, Volume 670, Issue 1, pp. 862-871. 2007 https://iopscience.iop.org/article/10.1086/522198/pdf Meshalkina et al., направлена в PASJ (cм. презентацию Grechnev IKI-09) Eruptions of Magnetic Ropes in Two Homologous Solar Events of 2002 Plasma heating in solar flares and their soft and hard X-ray emissions R. Falewicz E-print, May 2014; http://arxiv.org/pdf/1405.6038v1.pdf Radio and X-Ray Signatures of Magnetic Reconnection behind an Ejected Flux Rope Pick, M.; Demoulin, P.; Krucker, S.; Malandraki, O.; Maia, D. Astrophysical Journal, Volume 625, Issue 2, pp. 1019-1026, 2005. +20:30 UT: large SE eruption, of a small filament near AR Большие, хорошие димминги в 4-ех каналах, корональная волна? Нет данных LASCO, но есть MLSO; See Events A question raised from the observation of dynamic cusp formation: When and where does particle acceleration occur? Linhui Sui, Gordon D. Holman, & Brian R. Dennis E-print, Oct 2007, Adv. Space Res.Volume 41, Issue 6, 2008, Pages 976-983 the gradual formation of an EUV cusp feature is very clear. The observations also reveal the timing of the cusp formation and particle acceleration: most of the impulsive hard X-rays (>25 keV) were emitted before the cusp was seen. This suggests that fast reconnection occurred during the restructuring of the magnetic configuration, resulting in more efficient particle acceleration, while the reconnection slowed after the cusp was completely formed and the magnetic geometry was stabilized. This observation is consistent with the observations obtained with Yohkoh/Soft X-ray Telescope (SXT) that soft X-ray cusp structures only appear after the major impulsive energy release in solar flares. These observations have important implications for the modeling of magnetic reconnection and particle acceleration. The Application of Radio Diagnostics to the Study of the Solar Drivers of Space Weather Alexander Warmuth and Gottfried Mann 2005, File Radio and X-Ray Signatures of Magnetic Reconnection behind an Ejected Flux Rope Pick, M.; Demoulin, P.; Krucker, S.; Malandraki, O.; Maia, D. The Astrophysical Journal, Volume 625, Issue 2, pp. 1019-1026. 2005 https://iopscience.iop.org/article/10.1086/429530/pdf +3 - Interesting/outstanding chains after a SE eruption; ILLUSTRATION +4 - Interesting/complicated chains 12:40 UT: N-eruption, loop dimming and chains; see Events +5 - Interesting/complicated chains +08:30 UT: SE eruption, LDE, dimmings, halo CME; See Events 6 - Interesting/complicated chains; narrow CH 18 UT: NE eruption, large CME, EIT over-the-limb eruption 7 - Interesting/complicated chains; narrow CH 8 - Interesting/complicated chains; narrow CH +9 - Outstanding/complicated chains; narrow CH +12 UT: giant SE prominence eruption; See Events +20 UT: large narrow disk eruption вдоль активизирующегося волокна; фильмы MLSO; see 10 d; See Events Noise storm +10 - Outstanding/complicated chains; narrow CH +01 UT: one more giant narrow disk eruption; see 9d; See Events Noise storm +11 - Interesting chains; CH +18 UT: one more giant narrow disk eruption вдоль активизирующегося волокна; фильмы MLSO; see 9, 10d; See Events Noise storm 12 - Interesting chains; CH 18 UT: disk eruption 21 UT: disk eruption Noise storm 13 - Interesting chains; CH 09 UT: Small type II burst http://www.gsfc.nasa.gov/topstory/20020613sohoguitar.html 14 - Interesting chains; CH 15-18 - EIT bakeout An automated classification approach to ranking photospheric proxies of magnetic energy build-up Amani Al-Ghraibah, Laura. E. Boucheron, R.T.James McAteer A&A 579, A64 (2015) http://arxiv.org/pdf/1506.08717v1.pdf 19 - Interesting/outstanding chains; CH; Low activity 20 - Interesting chains; CH 21 - Interesting/outstanding chains; CH; Low activity +22 -!!! Interesting/outstanding chains;Illuatration!! CH; Low activity !02 UT: N/NE выброс волокна из АО вызвал эрупцию волокна вне АО ! See Events! 23 - Interesting/outstanding chains; CH; Low activity !03 UT; NW-limb flare and eruption! 24 - Interesting/outstanding chains; CH; Low activity 02 UT: SW CME 22 UT: NW eruption 25 - Interesting chains; CH; Low activity +26 - Interesting/outstanding chains; Illustration; CH; Low activity !08 UT: large NE-limb eruption Which Bow Shock Theory, Gasdynamic or Magnetohydrodynamic, Better Explains CME Stand-off Distance Ratios from LASCO-C2 Observations ? Jae-Ok Lee1,2, Y.-J. Moon1, Jin-Yi Lee3, R.-S. Kim2, and K.-S. Cho2 2017 ApJ 838 70 http://sci-hub.cc/10.3847/1538-4357/aa656f 27 - Interesting chains; CH; Low activity 28 - Interesting chains; CH; Low activity 00 UT: SW CME 29 - Interesting chains; CH; Low activity The two solar flares diagnostics based on the soft X-ray emission recording Mikhail I.Savchenko, Pavel V.VataginVadim P.LazutkovDmitriy V.Skorodumov, Igor V.KudryavtsevYuriy E.Charikov St. Petersburg Polytechnical University Journal: Physics and Mathematics Volume 3, Issue 3, October 2017, Pages 292-297 https://www.sciencedirect.com/science/article/pii/S240572231730097X Nonthermal X-Ray Spectral Flattening toward Low Energies in Early Impulsive Flares Sui, Linhui; Holman, Gordon D.; Dennis, Brian R. Astrophysical Journal, Volume 670, Issue 1, pp. 862-871. 2007 https://iopscience.iop.org/article/10.1086/522198/pdf ++30 - Interesting chains; CH; Low activity +!!03 UT: significant S filament eruption!! See Events! ++10 UT; large SE CME; Sharp, drifting onset of the noise storm!!! Similar to drifting continuum events. Are chains of type I radio bursts generated by similar processes as drifting pulsation structures observed during solar flares? Marian Karlicky A&A 2017 https://arxiv.org/pdf/1704.08532.pdf 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