Investigating the Sensitivity of Alfvén Pulse Interactions to Plasma Beta in the Corona
Two competing theories, the wave theory and reconnection theory, provide explanations for solar corona heating, supported by observations of wave phenomena and magnetic reconnection on the Sun. Plasma β, the ratio of thermal plasma pressure to magnetic pressure, varies significantly in the solar cor...
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Main Authors: | Naser Karimi, Mahdi Alizadeh, Zianab Shajei |
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Format: | Article |
Language: | English |
Published: |
Damghan university
2024-01-01
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Series: | Iranian Journal of Astronomy and Astrophysics |
Subjects: | |
Online Access: | https://ijaa.du.ac.ir/article_455_293826e9a0d99ecf9b446c6b1fa7e1a5.pdf |
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