Polytropic stellar wind models are extended beyond extreme adiabatic cases to non-adiabatic localized heating, with added energy shown plausible relative to flares and relevant to solar wind observations.
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Nonlinear hybrid models of PSP-observed anisotropic hot-beam ion VDFs produce combined ion-cyclotron and magnetosonic instabilities whose nonlinear stage yields qualitative agreement with observed hammerhead distributions.
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Polytropic stellar wind models with strongly localized heating
Polytropic stellar wind models are extended beyond extreme adiabatic cases to non-adiabatic localized heating, with added energy shown plausible relative to flares and relevant to solar wind observations.
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Modeling hot, anisotropic ion beams in the solar wind motivated by the Parker Solar Probe observations near perihelia
Nonlinear hybrid models of PSP-observed anisotropic hot-beam ion VDFs produce combined ion-cyclotron and magnetosonic instabilities whose nonlinear stage yields qualitative agreement with observed hammerhead distributions.