Mathematical modeling of the Parker’s instability development of large-scale vibrations of magnetic fields in the sun convective zone

Mathematical modeling of the Parker’s instability development of large-scale vibrations of magnetic fields in the sun convective zone

Background and Objectives: The physical mechanism of the generation of a steady wave flow at the photospheric level is studied, which ensures anomalous heating of the solar atmosphere at various stages of the solar activity cycle. Background and Objectives: We study the conditions of stability loss...

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Bibliographic Details
Main Authors: Stepanov, Evgeny Alexandrovich, Mayorov, Alexandr Olegovich, Romanov, Konstantin Valeryevich, Romanov, Dmitry Valeryevich, Romanov, Valery Alexandrovich
Format: Article
Language:English
Published: Saratov State University 2021-05-01
Series:Известия Саратовского университета. Новая серия Серия: Физика
Subjects:
solar atmosphere
anomalous heating
a thin magnetic tube
the parker’s instability
finite difference scheme
Online Access:https://fizika.sgu.ru/sites/fizika.sgu.ru/files/text-pdf/2021/05/fizika_2021_2-stranicy-5-14.pdf

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https://fizika.sgu.ru/sites/fizika.sgu.ru/files/text-pdf/2021/05/fizika_2021_2-stranicy-5-14.pdf

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