The solar elongation distribution of low-frequency radio bursts

Details The solar elongation distribution of low-frequency radio bursts The solar elongation distribution of low-frequency radio bursts

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...45..181k&link_type=abstract

Solar Physics, vol. 45, Nov. 1975, p. 181-187.

Astronomy and Astrophysics

Astronomy

12

Explorer 43 Satellite, Harmonic Radiation, Plasma Frequencies, Solar Wind, Type 3 Bursts, Astronomical Maps, Electron Density (Concentration), Spaceborne Astronomy

Scientific paper

Over 500 days of low-frequency (less than 1 MHz) radio observations from the IMP-6 spacecraft have been accumulated to produce a two-dimensional map (frequency vs elongation) of solar type III burst occurrences. This map indicates that most solar bursts in this frequency range are observed at the second harmonic of the plasma frequency, rather than the fundamental. The map also shows that the solar wind electron density varies as an inverse power of heliocentric distance, with the exponent somewhat less than 2 to perhaps 3 or higher.

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