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Keywords = magneto-Poincare waves

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42 pages, 1575 KiB  
Review
Variable Density Flows in Rotating Astrophysical Plasma. Linear Waves and Resonant Phenomena
by Maria Fedotova, Dmitry Klimachkov and Arakel Petrosyan
Universe 2021, 7(4), 87; https://doi.org/10.3390/universe7040087 - 1 Apr 2021
Cited by 8 | Viewed by 2960
Abstract
New observational data and modeling of physical processes constantly appear in the young and rapidly developing branch of science of plasma astrophysics. However, there is a lack of theoretical studies in the field of plasma astrophysics, that could unite the physics of various [...] Read more.
New observational data and modeling of physical processes constantly appear in the young and rapidly developing branch of science of plasma astrophysics. However, there is a lack of theoretical studies in the field of plasma astrophysics, that could unite the physics of various objects in the Universe, explain the observed phenomena and contribute to the improvement of numerical modeling schemes efficiency. This article makes up for this shortcoming by introducing different models, taking into account the various properties of plasma objects. We present a review of the latest magnetohydrodynamic theories of wave processes in rotating astrophysical plasma, taking into account important and common properties of astrophysical objects as compressibility and stratification. Full article
(This article belongs to the Section Space Science)
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