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.
archivePrefix = "arXiv", eprint =
2 Pith papers cite this work, alongside 13 external citations. Polarity classification is still indexing.
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Derives a nonlinear equation for dust drift waves including both nonlinear dust density and vorticity terms, which reduces to 2D solitary waves or the Hasegawa-Mima equation in limiting cases.
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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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Nonlinear Equation for Dust Drift Waves
Derives a nonlinear equation for dust drift waves including both nonlinear dust density and vorticity terms, which reduces to 2D solitary waves or the Hasegawa-Mima equation in limiting cases.