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The solar elongation distribution of low-frequency radio bursts

โœ Scribed by M. L. Kaiser

Book ID
104644432
Publisher
Springer
Year
1975
Tongue
English
Weight
359 KB
Volume
45
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

Over 500 days of low-frequency (< 1 MHz) radio observations from the IMP-6 spacecraft have been accumulated to produce a two-dimensional map (frequency vs elongation) of solar type II[ 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 R -7, where y can be somewhat less than 2 to perhaps 3 or higher.

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