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Radio occultation probing of the turbulent circumsolar plasma by pulsar pulses at small elongations
Authors:A N Afanas’ev
Institution:(1) Institute of Solar-Terrestrial Physics, Siberian Division of the Russian Academy of Sciences, P.O. Box 4026, Irkutsk, 664033, Russia
Abstract:The possibility of using the occultation of a pulsar by the solar corona for diagnostics of the magnitude of coronal electron-density inhomogeneities is analyzed. Coronal probing at small elongations is considered, when a ground-based receiver can be in the vicinity of the caustic surface due to the regular refraction of the pulsar radio emission in the circumsolar plasma.
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