Theory of Fluid Instabilities in Partially Ionized Plasmas: An Overview

نویسندگان

چکیده

Partially ionized plasmas (PIP) are essential constituents of many astrophysical environments, including the solar atmosphere, interstellar medium, molecular clouds, accretion disks, planet ionospheres, cometary tails, etc., where ionization degree may vary from very weak to almost full ionization. The dynamics PIP is heavily affected by interactions between various charged and neutral species that compose plasma. It has been shown partial effects influence triggering development fluid instabilities as, e.g., Kelvin-Helmholtz, Rayleigh-Taylor, thermal, magneto-rotational instabilities, among others. Here we review theory some classic present in highlight unique introduced main emphasis put on partially atmospheric plasma, although other applications also mentioned. We focus mathematical theoretical investigation onset exponential growth instabilities. Results nonlinear evolution obtained numerical simulations discussed.

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ژورنال

عنوان ژورنال: Frontiers in Astronomy and Space Sciences

سال: 2022

ISSN: ['2296-987X']

DOI: https://doi.org/10.3389/fspas.2022.789083