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Propagation and Damping of Longitudinal Intensity Oscillations in Solar Coronal Structures

Recently, the longitudinal oscillations of intensity have been frequently detected in the different structures of the solar corona using space telescope observations. Some researchers believe that the magneto-acoustic waves, which share the plasma heating processes in the corona, are responsible for...

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Autors principals: Abbas Abedini, Mahdieh Sadat Mousavi Monfared
Format: Artigo
Idioma:Inglês
Publicat: Damghan university 2017-10-01
Col·lecció:Iranian Journal of Astronomy and Astrophysics
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Accés en línia:https://ijaa.du.ac.ir/article_127_c738819b7a2425dbb17eae91b657973c.pdf
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