Enviar artigo por via de e-mail Possible Mechanism of Enhancement of Diamagnetic Current Dissipation during the Heating of Magnetic Flux Tubes in the Solar Corona
- Autores: Kovalev V.A.1
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Afiliações:
- Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
- Edição: Volume 44, Nº 2 (2018)
- Páginas: 267-269
- Seção: 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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Resumo
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.
Sobre autores
V. Kovalev
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
Autor responsável pela correspondência
Email: vic.kov@yandex.ru
Rússia, Troitsk, Moscow, 142190
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