Отправить статью по E-mail Possible Mechanism of Enhancement of Diamagnetic Current Dissipation during the Heating of Magnetic Flux Tubes in the Solar Corona
- Авторы: Kovalev V.1
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Учреждения:
- Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
- Выпуск: Том 44, № 2 (2018)
- Страницы: 267-269
- Раздел: Space Plasma
- URL: https://journals.rcsi.science/1063-780X/article/view/186686
- DOI: https://doi.org/10.1134/S1063780X18020083
- ID: 186686
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Аннотация
It is shown that dissipation of the diamagnetic current heating the coronal plasma with the classical conductivity in the absence of a longitudinal current can increase significantly due to the cellular transverse microstructure of the flux tube, thereby compensating for intense radiative losses.
Об авторах
V. Kovalev
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
Автор, ответственный за переписку.
Email: vic.kov@yandex.ru
Россия, Troitsk, Moscow, 142190
