Multifluid and Kinetic 2D and 3D Simulations of Thermal Farley–Buneman Instability Turbulence in the Solar Chromosphere

Multifluid and Kinetic 2D and 3D Simulations of Thermal Farley–Buneman Instability Turbulence in the Solar Chromosphere

Models currently fail to reproduce observations of the coldest regions in the Sun’s atmosphere, though recent work suggests the thermal Farley–Buneman instability (TFBI) may play a critical role. This meter-scale, electrostatic, multifluid plasma instability causes turbulence and heating in the cold...

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Bibliographic Details
Main Authors: Samuel Evans, Meers Oppenheim, Juan Martínez-Sykora, Yakov Dimant
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar chromosphere
Solar chromospheric heating
Plasma physics
Astronomical simulations
Online Access:https://doi.org/10.3847/1538-4357/adcd70
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https://doi.org/10.3847/1538-4357/adcd70

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