Coronal Loop as an Element of the Potential Magnetic Arcade
- Autores: Solov’ev A.A.1,2, Kirichek E.A.1, Korol’kova O.A.1
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Afiliações:
- Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
- Kalmyk State University
- Edição: Volume 57, Nº 7 (2017)
- Páginas: 849-853
- Seção: Article
- URL: https://journal-vniispk.ru/0016-7932/article/view/156498
- DOI: https://doi.org/10.1134/S0016793217070209
- ID: 156498
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Resumo
A new analytical model of a fine singular 3D coronal loop is developed. The loop is a thin curved magnetic flux tube immersed in the potential magnetic arcade. The ambient corona is given by the hydrostatic model of a quiet solar atmosphere (Avrett and Loeser, 2008). The proposed 3D model of a fine coronal loop reproduces well the observed physical properties of coronal structures of this kind.
Sobre autores
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, 358000
E. Kirichek
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
Email: solov@gao.spb.ru
Rússia, St. Petersburg, 196140
O. Korol’kova
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
Email: solov@gao.spb.ru
Rússia, St. Petersburg, 196140
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