Space and astrophysical plasma as a physical system refers to ionized gases permeating cosmic environments such as the interstellar and intergalactic medium, stellar winds, accretion disks, and magnetospheres. These plasmas are typically low-collisionality, often magnetized, and governed by collective electromagnetic interactions described by magnetohydrodynamics (MHD), kinetic theory, or hybrid models. Key properties include Debye shielding, anisotropic pressure, and nonthermal particle distributions, with dynamics dominated by magnetic reconnection, turbulence, waves, and instabilities. Space and astrophysical plasmas are central to energy and momentum transport, cosmic ray acceleration, and radiation processes across a vast range of spatial and temporal scales.
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