Turbulence from mixed-polarity magnetic carpet fields supplies enough dissipated energy to heat the solar chromosphere and lower corona, with gradual heating of spicules by entrained turbulence.
A publicly available simulation of an enhanced network region of the Sun
3 Pith papers cite this work, alongside 185 external citations. Polarity classification is still indexing.
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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.
A review summarizing observational properties, dynamics, and heating implications of transition region loops observed primarily with IRIS, distinct from coronal loops.
citing papers explorer
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Turbulence and its Potential Impact on Solar Chromospheric and Coronal Heating
Turbulence from mixed-polarity magnetic carpet fields supplies enough dissipated energy to heat the solar chromosphere and lower corona, with gradual heating of spicules by entrained turbulence.
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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.
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Magnetic loops in the solar transition region
A review summarizing observational properties, dynamics, and heating implications of transition region loops observed primarily with IRIS, distinct from coronal loops.