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Formation of Sources for Solar Cosmic Rays in Eruptive Flares X6.9 and M5.1 Observed August 9, 2011, and May 17, 2012
DOI: 10.1134/S106377292206004X Bibcode: 2022ARep...66..481G

Struminsky, A. B.; Grigorieva, I. Yu.

A coronal mass ejection (CME) and solar proton event (SPE) succeeding weak flares in soft X-rays and being observed in the interplanetary space (IS) is not any unusual. However, it remains unclear in what way extreme CME and SPE characteristics can be realized in such cases. The present work compares solar and IS observations associated with the l…

2022 Astronomy Reports
SOHO 9
Study of the Magnetic Properties of Sunspot Umbrae
DOI: 10.1134/S1063772922030064 Bibcode: 2022ARep...66..116Z

Obridko, V. N.; Fainshtein, V. G.; Rudenko, G. V. +1 more

The paper presents the results of the study of sunspots, obtained by the authors and other researchers in recent years. The results regarding the atmosphere above sunspot umbrae, based on the observational data in the spectral lines of the upper chromosphere and lower corona, are discussed. It is shown that individual parameters of the profile of …

2022 Astronomy Reports
SOHO 5
Solar Photospheric Magnetic Fields, Coronal Mass Ejections, and Type II Radio Bursts in Cycles 23 and 24
DOI: 10.1134/S1063772922080017 Bibcode: 2022ARep...66..579B

Bilenko, I. A.

We consider the events of type II radio bursts (RBII) in the decametric and hectometric ranges from 1 to 16 MHz and the dependence of the parameters of associated coronal mass ejections (CMEs) on the background characteristics of the plasma and interplanetary magnetic field (IMF) in the regions where each radio burst was detected in solar cycles 2…

2022 Astronomy Reports
SOHO 0