Enviar artigo por via de e-mail Modeling of the Fine Filament Structure of Quiescent Solar Prominences
- Autores: Korolkova O.A.1, Solov’ev A.A.1,2
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Afiliações:
- Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
- Kalmyk State University
- Edição: Volume 57, Nº 8 (2017)
- Páginas: 1018-1022
- Seção: Article
- URL: https://journal-vniispk.ru/0016-7932/article/view/156558
- DOI: https://doi.org/10.1134/S0016793217080138
- ID: 156558
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Resumo
Several new models of solar prominences with helical geometry of the magnetic field were suggested; the possibility of the construction of a filament model with a fine filament structure was shown. For the first time, numerical solutions of the magnetohydrostatical problem, in which a fine structure of an equilibrium solar filament is expressed not only in the vertical direction but also in the direction along the filament axis, were obtained.
Sobre autores
O. Korolkova
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
Email: solov@gao.spb.ru
Rússia, St. Petersburg, 196140
A. Solov’ev
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences; Kalmyk State University
Autor responsável pela correspondência
Email: solov@gao.spb.ru
Rússia, St. Petersburg, 196140; Elista
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