MODELING OF SOUND WAVE PROPAGATION IN THE SOLAR CORONA
https://doi.org/10.37493/2307-910X.2022.4.10
Abstract
In this paper we aim to simulate the propagation of magnetosonic waves in the solar corona by modeling the decay of a wave packet due to the thermal misbalance and the dispersion effect. Slow sound waves are considered as a wave model for two reasons, the first is that the effect is most pronounced here, the second is the presence of a significant number of observations of waves in the lower corona, which are interpreted as slow waves. Formation of quasi-periodic slow magnetosonic wave trains by the heating/cooling misbalance is constructed.
About the Authors
N. K. Shividov
Kalmyk State University named after B. B. Gorodovikov
Russian Federation
Russian Federation
Shividov Nikolai K., Assistant of the Department of Theoretical Physics
Elista, Pushkin street, 11
G. A. Mankaeva
Kalmyk State University named after B. B. Gorodovikov
Russian Federation
Russian Federation
Mankaeva Galina A., Senior Lecturer of the Department of Algebra, Analysis and Methods of Teaching Mathematics
Elista, Pushkin street, 11
N. A. Kurkudinova
Kalmyk State University named after B. B. Gorodovikov
Russian Federation
Russian Federation
Kurkudinova Natalia A., Senior Lecturer, Department of Environmental Management and Environmental Protection
Elista, Pushkin street, 11
D. B. Bembitov
Kalmyk State University named after B. B. Gorodovikov
Russian Federation
Russian Federation
Bembitov Dzhirgal B., Associate Professor, Department of Theoretical Physics
Elista, Pushkin street, 11
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Review
For citations:
Shividov N.K., Mankaeva G.A., Kurkudinova N.A., Bembitov D.B. MODELING OF SOUND WAVE PROPAGATION IN THE SOLAR CORONA. Modern Science and Innovations. 2022;(4):103-107. (In Russ.) https://doi.org/10.37493/2307-910X.2022.4.10
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