The modeling of quasi-periodic oscillations propagation in the solar corona

In the general problem of oscillations observed in the solar corona, a particularly intriguing position is occupied by quasi-periodic oscillations, which are often observed in coronal holes. Most often, periods are observed in pairs of close values. Among the possible explanations of this phenomenon...

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Main Authors: N. K. Shividov, A. K. Baltykov, T. V. Velegurin, G. A. Mankaeva, B. B. Mikhalyaev
Format: Article
Language:Russian
Published: North-Caucasus Federal University 2024-03-01
Series:Современная наука и инновации
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Online Access:https://msi.elpub.ru/jour/article/view/1565
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author N. K. Shividov
A. K. Baltykov
T. V. Velegurin
G. A. Mankaeva
B. B. Mikhalyaev
author_facet N. K. Shividov
A. K. Baltykov
T. V. Velegurin
G. A. Mankaeva
B. B. Mikhalyaev
author_sort N. K. Shividov
collection DOAJ
description In the general problem of oscillations observed in the solar corona, a particularly intriguing position is occupied by quasi-periodic oscillations, which are often observed in coronal holes. Most often, periods are observed in pairs of close values. Among the possible explanations of this phenomenon, we consider the dispersion of acoustic waves under the influence of thermal conductivity. The possibility of the appearance of pairs of periods may be due to the existence of a minimum at the group velocity, which is realized under the conditions available in the corona. We show how this works, and also claim that this mechanism can serve for the purposes of coronal seismology to determine the parameters of coronal plasma.
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institution Kabale University
issn 2307-910X
language Russian
publishDate 2024-03-01
publisher North-Caucasus Federal University
record_format Article
series Современная наука и инновации
spelling doaj-art-e4ca2acb920142ae874045ff3213ccf52025-08-20T03:57:48ZrusNorth-Caucasus Federal UniversityСовременная наука и инновации2307-910X2024-03-010416016610.37493/2307-910X.2023.4.181535The modeling of quasi-periodic oscillations propagation in the solar coronaN. K. Shividov0A. K. Baltykov1T. V. Velegurin2G. A. Mankaeva3B. B. Mikhalyaev4B. B. Gorodovikov Kalmyk State UniversityKalmyk State University named after B. B. GorodovikovB. B. Gorodovikov Kalmyk State UniversityB. B. Gorodovikov Kalmyk State UniversityKalmyk State University named after B. B. GorodovikovIn the general problem of oscillations observed in the solar corona, a particularly intriguing position is occupied by quasi-periodic oscillations, which are often observed in coronal holes. Most often, periods are observed in pairs of close values. Among the possible explanations of this phenomenon, we consider the dispersion of acoustic waves under the influence of thermal conductivity. The possibility of the appearance of pairs of periods may be due to the existence of a minimum at the group velocity, which is realized under the conditions available in the corona. We show how this works, and also claim that this mechanism can serve for the purposes of coronal seismology to determine the parameters of coronal plasma.https://msi.elpub.ru/jour/article/view/1565computer modelingquasi-periodic oscillationsplasma physicsnumerical solutionacoustic waveshydrodynamicsdispersionwave packets
spellingShingle N. K. Shividov
A. K. Baltykov
T. V. Velegurin
G. A. Mankaeva
B. B. Mikhalyaev
The modeling of quasi-periodic oscillations propagation in the solar corona
Современная наука и инновации
computer modeling
quasi-periodic oscillations
plasma physics
numerical solution
acoustic waves
hydrodynamics
dispersion
wave packets
title The modeling of quasi-periodic oscillations propagation in the solar corona
title_full The modeling of quasi-periodic oscillations propagation in the solar corona
title_fullStr The modeling of quasi-periodic oscillations propagation in the solar corona
title_full_unstemmed The modeling of quasi-periodic oscillations propagation in the solar corona
title_short The modeling of quasi-periodic oscillations propagation in the solar corona
title_sort modeling of quasi periodic oscillations propagation in the solar corona
topic computer modeling
quasi-periodic oscillations
plasma physics
numerical solution
acoustic waves
hydrodynamics
dispersion
wave packets
url https://msi.elpub.ru/jour/article/view/1565
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