Effects of Ion Magnetization on the Farley–Buneman Instability in the Solar Chromosphere
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/857/i=2/a=129/pdf
Reference34 articles.
1. Radiative Energy Loss from the Solar Chromosphere and Corona
2. Plasma wave heating during extreme electric fields in the high-latitudeEregion
3. Excitation of Field Aligned Sound Waves by Electron Streams
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1. Unified fluid theory of the collisional thermal Farley–Buneman instability including magnetized multi-species ions;Physics of Plasmas;2023-10-01
2. Multifluid Simulation of Solar Chromospheric Turbulence and Heating Due to Thermal Farley–Buneman Instability;The Astrophysical Journal;2023-05-30
3. Theory of Fluid Instabilities in Partially Ionized Plasmas: An Overview;Frontiers in Astronomy and Space Sciences;2022-05-05
4. Toward An Integrated View of Ionospheric Plasma Instabilities: 5. Ion‐Thermal Instability for Arbitrary Ion Magnetization, Density Gradient, and Wave Propagation;Journal of Geophysical Research: Space Physics;2020-09
5. Newly Discovered Source of Turbulence and Heating in the Solar Chromosphere;The Astrophysical Journal;2020-02-27
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