Multifluid plasma simulations find that the Thermal Farley-Buneman Instability boosts neutral heating by (43±7)% on average, increases charged-species temperatures proportionally to driving field strength, and rotates current density components in the solar chromosphere.
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The Unstable Chromosphere: Effects of the Thermal Farley-Buneman Instability Across a Broad Range of Solar Chromospheric Conditions
Multifluid plasma simulations find that the Thermal Farley-Buneman Instability boosts neutral heating by (43±7)% on average, increases charged-species temperatures proportionally to driving field strength, and rotates current density components in the solar chromosphere.