The Effect of Steady Flow on the Physical Quantities of Slow mMagneto Acoustic Waves in Solar Coronal Plasma
textbf{Damping of slow magnetohydrodynamic(MHD) waves and oscillations are believed to contribute to the heating of the solar corona. Since the launch of solar space telescopes, many observational evidences for the occurrence of slow MHD waves have been detected in various structures of the solar co...
| Autor principal: | |
|---|---|
| Format: | Article |
| Idioma: | English |
| Publicat: |
Damghan university
2020-04-01
|
| Col·lecció: | Iranian Journal of Astronomy and Astrophysics |
| Matèries: | |
| Accés en línia: | https://ijaa.du.ac.ir/article_184_9e3ceb566cb63f484cfe67a7c9bfb1b7.pdf |