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Akademický článek
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Solar radio emission features a large number of fine structures demonstrating great variability in frequency and time. We present spatially resolved spectral radio observations of type IIIb bursts in the $30-80$ MHz range made by the Low Frequency Ar
Externí odkaz:
http://arxiv.org/abs/1806.01046
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:
http://arxiv.org/abs/1805.10729
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
The X9.3 flare of September 6, 2017, was the most powerful flare of Solar Cycle 24. It generated strong white-light emission and multiple helioseismic waves (sunquakes). By using data from Helioseismic and Magnetic Imager (HMI) onboard the Solar Dyna
Externí odkaz:
http://arxiv.org/abs/1804.06565
Publikováno v:
The Astrophysical Journal, Volume 840, Issue 2, article id. 84, 13 pp. (2017)
We study flare processes in the solar atmosphere using observational data for a M1-class flare of June 12, 2014, obtained by New Solar Telescope (NST/BBSO) and Helioseismic Magnetic Imager (HMI/SDO). The main goal is to understand triggers and manife
Externí odkaz:
http://arxiv.org/abs/1801.04921
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
Autor:
R. Е. Sharykin
Publikováno v:
Informatika, Vol 19, Iss 1, Pp 88-95 (2022)
Software development methodology based on the model of distributed object-based stochastic hybrid systems is proposed. Such mathematical model is planned to be created for the system being designed along with the system specification at all stages of
Externí odkaz:
https://doaj.org/article/18ea5a0970dd40f7800fba04abd73e3a
Autor:
Sharykin, I. N.1 (AUTHOR) ivan.sharykin@phystech.edu, Zimovets, I. V.1,2 (AUTHOR), Radivon, A. V.1,2 (AUTHOR)
Publikováno v:
Cosmic Research. Aug2023, Vol. 61 Issue 4, p265-282. 18p.