Two independent modeling approaches, ExPRES time-frequency simulations and adiabatic drift-rate analysis, jointly point to 20-30 keV electrons on magnetic shells with apexes at 2-10 stellar radii in AD Leo, with X-mode emission from the southern magnetic hemisphere.
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Location and energy of electrons producing the radio bursts from AD Leo observed by FAST in December 2021
Two independent modeling approaches, ExPRES time-frequency simulations and adiabatic drift-rate analysis, jointly point to 20-30 keV electrons on magnetic shells with apexes at 2-10 stellar radii in AD Leo, with X-mode emission from the southern magnetic hemisphere.