Мақаланы E-mail арқылы жіберу Possible Mechanism of Enhancement of Diamagnetic Current Dissipation during the Heating of Magnetic Flux Tubes in the Solar Corona
- Авторлар: Kovalev V.1
-
Мекемелер:
- Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
- Шығарылым: Том 44, № 2 (2018)
- Беттер: 267-269
- Бөлім: Space Plasma
- URL: https://journals.rcsi.science/1063-780X/article/view/186686
- DOI: https://doi.org/10.1134/S1063780X18020083
- ID: 186686
Дәйексөз келтіру
Ашық рұқсат
Рұқсат берілді
Тек жазылушылар үшін
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.
Авторлар туралы
V. Kovalev
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
Хат алмасуға жауапты Автор.
Email: vic.kov@yandex.ru
Ресей, Troitsk, Moscow, 142190
