Email this article Modeling of the Fine Filament Structure of Quiescent Solar Prominences
- Authors: Korolkova O.A.1, Solov’ev A.A.1,2
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Affiliations:
- Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
- Kalmyk State University
- Issue: Vol 57, No 8 (2017)
- Pages: 1018-1022
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/156558
- DOI: https://doi.org/10.1134/S0016793217080138
- ID: 156558
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Abstract
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.
About the authors
O. A. Korolkova
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
Email: solov@gao.spb.ru
Russian Federation, St. Petersburg, 196140
A. A. Solov’ev
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences; Kalmyk State University
Author for correspondence.
Email: solov@gao.spb.ru
Russian Federation, St. Petersburg, 196140; Elista
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