Zobrazeno 1 - 10
of 40
pro vyhledávání: '"I. N. Sharykin"'
Publikováno v:
Geomagnetism and Aeronomy. 61:956-963
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::978a896278920506e72a4f86c1a28094
https://doi.org/10.1134/s0016793221070148
https://doi.org/10.1134/s0016793221070148
Publikováno v:
Astrophysics. 63:408-420
Electric currents flow in active regions of the sun. Information on the distribution of the currents is important for understanding energy release processes on the sun’s surface and in overlying layers. This is an analysis of the probability densit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::15d4252c3667f30bd344ef8846cd4216
https://doi.org/10.1007/s10511-020-09645-0
https://doi.org/10.1007/s10511-020-09645-0
Helioseismic response to solar flares ("sunquakes") occurs due to localized force or/and momentum impacts observed during the flare impulsive phase in the lower atmosphere. Such impacts may be caused by precipitation of high-energy particles, downwar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::33ada389646ffc1a5bab83f93ba34afe
https://doi.org/10.5194/egusphere-egu21-1461
https://doi.org/10.5194/egusphere-egu21-1461
There are still debates whether particle acceleration in solar flares may occur due to interruption of electric currents flowing along magnetic loops. To contribute to this problem, we performed the first statistical study of relationships between fl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a7afae7c96c6fabd84133fca00777e4
http://arxiv.org/abs/2002.06646
http://arxiv.org/abs/2002.06646
Autor:
Chi Wang, A. B. Struminsky, S. A. Kuznetsov, Ying Liu, R. Wang, I. N. Sharykin, Ivan Zimovets, Valery M. Nakariakov
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 174:17-27
We present analysis of the magnetic field in seven solar flare regions accompanied by the pulsations of hard X-ray (HXR) emission. These flares were studied by Kuznetsov et al. (2016) (Paper~I), and chosen here because of the availability of the vect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::634f111d35632908d1d98a7f0c2e76b5
https://doi.org/10.1016/j.jastp.2018.04.017
https://doi.org/10.1016/j.jastp.2018.04.017
Publikováno v:
Astronomy Reports. 61:805-819
The solar event SOL2012–10–23T03:13, which was associated with a X1.8 flare without an accompanying coronal mass ejection (CME) and with a Type II radio burst, is analyzed. A method for constructing the spatial and temporal profiles of the differ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5136be788270a6333bebde2323d8c203
https://doi.org/10.1134/s1063772917080030
https://doi.org/10.1134/s1063772917080030
The paper presents results of a search for helioseismic events (sunquakes) produced by M-X class solar flares during Solar Cycle 24. The search is performed by analyzing photospheric Dopplergrams from Helioseismic Magnetic Imager (HMI). Among the tot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1941885defa473a2a843756f4548dbd5
Autor:
S. Vargas Domínguez, Viacheslav M. Sadykov, Alexander G. Kosovichev, Ivan Zimovets, I. N. Sharykin
Publikováno v:
Proceedings of the International Astronomical Union. 12:103-108
Initiation and development of a M 1.0 class flare of June 12, 2014, was observed by space and ground-based telescopes, including EUV and X-ray imaging spectroscopy by IRIS and RHESSI, and high-resolution optical imaging by 1.6 m New Solar Telescope (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::da5909b33a82e91c46d25056c71dc27d
https://doi.org/10.1017/s1743921317003994
https://doi.org/10.1017/s1743921317003994
Publikováno v:
The Astrophysical Journal. 893:159
This work is a continuation of Paper I [Sharykin et al., 2018] devoted to analysis of nonthermal electron dynamics and plasma heating in the confined M1.2 class solar flare SOL2015-03-15T22:43 revealing energy release in the highly sheared interactin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2713f31c6e2f132036ea29bbf2c12b9
https://doi.org/10.3847/1538-4357/ab84ef
https://doi.org/10.3847/1538-4357/ab84ef
We present a statistical study of chromospheric evaporation in solar flares using simultaneous observations by the RHESSI X-ray telescope and the IRIS UV spectrograph. The results are compared with radiation hydrodynamic flare models from the F-CHROM
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b391c08c48ebd5f36a4f745dc1bc0637
http://arxiv.org/abs/1805.10729
http://arxiv.org/abs/1805.10729