Zobrazeno 1 - 10
of 48
pro vyhledávání: '"Myshyakov, I. I."'
Autor:
Grechnev, V. V., Meshalkina, N. S., Uralov, A. M., Kochanov, A. A., Lesovoi, S. V., Myshyakov, I. I., Kiselev, V. I., Zhdanov, D. A., Altyntsev, A. T., Globa, M. V.
Publikováno v:
Solar Physics, 295(2020), 128
On 23 July 2016 after 05:00\,UTC, the first 48-antenna stage of the Siberian Radioheliograph detected two flares of M7.6 and M5.5 GOES importance that occurred within half an hour in the same active region. Their multi-instrument analysis reveals the
Externí odkaz:
http://arxiv.org/abs/2009.10350
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:
http://arxiv.org/abs/1905.03352
We present the study of SOL2015-03-15 M1.2 flare, revealing acceleration of electrons and plasma heating in the sheared twisted magnetic structure in the polarity inversion line (PIL). The scope is to make the analysis of nonthermal electrons dynamic
Externí odkaz:
http://arxiv.org/abs/1805.05792
This work demonstrates the possibility of magnetic field topology investigations using microwave polarimetric observations. We study a solar flare of GOES M1.7 class that occurred on 11 February, 2014. This flare revealed a clear signature of spatial
Externí odkaz:
http://arxiv.org/abs/1801.04400
Publikováno v:
Solar-Terrestrial Physics, Vol 8, Iss 2, Pp 3-9 (2022)
A response has been found in a narrow band 5–7 GHz of microwave emission to the appearance of a coronal X-ray point. The emission source is a short X-ray loop located in the tail part of an active region and occurring when magnetic fields are recon
Externí odkaz:
https://doaj.org/article/882e7e7c094b496d9c19455f4302d516
Akademický článek
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We have analyzed multi-wavelength observations and magnetic-field data for the solar flare of May 10, 2012 (04:18 UT) and have detected a sign inversion of the signal in the line-of-sight magnetic measurements in the umbra of a small spot. This effec
Externí odkaz:
http://arxiv.org/abs/1604.07073
Autor:
Kolobov, D. Y., Kobanov, N. I., Chelpanov, A. A., Kochanov, A. A., Anfinogentov, S. A., Chupin, S. A., Myshyakov, I. I., Tomin, V. E.
In this study we combine the multiwavelength ultraviolet -- optical (Solar Dynamics Observatory, SDO) and radio (Nobeyama Radioheliograph, NoRH) observations to get further insight into space-frequency distribution of oscillations at different atmosp
Externí odkaz:
http://arxiv.org/abs/1505.02857
Autor:
Uralov, A. M., Grechnev, V. V., Rudenko, G. V., Myshyakov, I. I., Chertok, I. M., Filippov, B. P., Slemzin, V. A.
Our analysis in Papers I and II (Grechnev et al., 2014, Solar Phys. 289, 289 and 1279) of the 18 November 2003 solar event responsible for the 20 November geomagnetic superstorm has revealed a complex chain of eruptions. In particular, the eruptive f
Externí odkaz:
http://arxiv.org/abs/1404.3515
Autor:
Rudenko, G. V., Myshyakov, I. I.
An algorithm for calculating three gauge-invariant helicities (self-, mutual- and Berger relative helicity) for a magnetic field specified in a rectangular box is described. The algorithm is tested on a well-known force-free model (Low and Lou, 1990)
Externí odkaz:
http://arxiv.org/abs/1009.4057