First-year SWAYS observations report a superflare on EK Draconis with no low-frequency radio signal, interpreted as evidence that dense coronae in active stars inhibit type II/III burst instabilities.
year = 1965, month = sep, volume =
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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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Summary of the First Year of the Space Weather Around Young Suns Program: 900 Hours of Low-frequency Radio and Optical Data Dedicated to Young, Solar-type Stars
First-year SWAYS observations report a superflare on EK Draconis with no low-frequency radio signal, interpreted as evidence that dense coronae in active stars inhibit type II/III burst instabilities.
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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.