Coronal Loop as an Element of the Potential Magnetic Arcade


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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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