Page 4: 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.

How young galaxies grew magnetic fields faster than expected

How fast can a galaxy build ordered magnetic fields spanning thousands of light-years? Existing theories say several billion years, but observations of galaxies in our universe imply shorter timescales. In a study published ...

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