Page 6: Research news on Space & astrophysical plasma

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.

Turbulent solar wind originates in the sun's corona, study shows

Solar wind is a never-ending stream of charged particles coming from the sun. Rather than a constant breeze, this wind is rather gusty. As solar wind particles travel through space, they interact with the sun's variable magnetic ...

New AI program helps identify elusive space plasmoids

In an ongoing game of cosmic hide and seek, scientists have a new tool that may give them an edge. Physicists at the U.S. Department of Energy's (DOE) Princeton Plasma Physics Laboratory (PPPL) have developed a computer program ...

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