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Plasma Evolutions Around a Solar Coronal 3D Magnetic Null Point

It is investigated how the plasma evaluates due to the propagation of the nonlinear Alfven wave. Magnetic null points that are detected in the solar corona have 3D structures which are prevalent in the solar atmosphere. In this study, we consider the real 3D structure with a 3D magnetic null point....

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Autors principals: Somaiyeh Sabri, Hossein Ebadi
Format: Artigo
Idioma:Inglês
Publicat: Damghan university 2021-07-01
Col·lecció:Iranian Journal of Astronomy and Astrophysics
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Accés en línia:https://ijaa.du.ac.ir/article_255_fea317a6c0d6b1a6af4817781698489e.pdf
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