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.
Space Science Reviews 160, 145–168
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Broadband KAW turbulence self-organizes into coherent density structures at kinetic scales with inertial-range suppression governed by moderate Reynolds-number constraints.
Long-term near-Earth solar wind observations establish a robust empirical connection between flow speed and magnetohydrodynamic turbulence energy.
Coherent structures that self-consistently emerge in strong MHD turbulence serve as the dominant sites for localized electric-field intensification and repeated particle acceleration across cosmic plasmas.
citing papers explorer
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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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Inertial-Range Suppression and Ponderomotive Density Cavitation in Broadband Sub-Alfv\'{e}nic Turbulence under Plasma Sheet Boundary Layer Conditions
Broadband KAW turbulence self-organizes into coherent density structures at kinetic scales with inertial-range suppression governed by moderate Reynolds-number constraints.
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A robust empirical relationship between speed and turbulence energy in the near-Earth solar wind
Long-term near-Earth solar wind observations establish a robust empirical connection between flow speed and magnetohydrodynamic turbulence energy.
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Strong MHD Turbulence and Coherent Structures as Drivers of Cosmic Particle Acceleration
Coherent structures that self-consistently emerge in strong MHD turbulence serve as the dominant sites for localized electric-field intensification and repeated particle acceleration across cosmic plasmas.