Radio occultation probing of the turbulent circumsolar plasma by pulsar pulses at small elongations

Details Radio occultation probing of the turbulent circumsolar plasma by pulsar pulses at small elongations Radio occultation probing of the turbulent circumsolar plasma by pulsar pulses at small elongations

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006arep...50..762a&link_type=abstract

Astronomy Reports, vol. 50, Issue 9, p.762-772

Astronomy and Astrophysics

Astronomy

1

Pacs Numbers 96.60.P-, 52.35.Ra, 97.60.Gb

Scientific paper

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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