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.

New insights into an enigmatic form of magnetic reconnection

In magnetic reconnection, adjacent magnetic field lines break and snap together to form new lines. This process converts magnetic energy to both thermal energy, or heat, and kinetic energy, or the acceleration of particles, ...

AI model reveals secrets of dendritic growth in thin films

Thin film devices, composed of layers of materials a few nanometers thick, play an important role in various technologies, from semiconductors to communication technologies. For instance, graphene and hexagonal-boron nitride ...

New model predicts solar storm particle acceleration and escape

The sun, a searing hot sphere of gas primarily composed of hydrogen and helium, boasts surface and outer atmospheric temperatures ranging from 10,000 to 3.6 million degrees Fahrenheit on its surface and its atmosphere's outermost ...

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