Power spectrum of small-scale irregularities in the solar wind

Details Power spectrum of small-scale irregularities in the solar wind Power spectrum of small-scale irregularities in the solar wind

Aug 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973p%26ss...21.1367h&link_type=abstract

Planetary and Space Science, Volume 21, Issue 8, p. 1367-1379.

Physics

9

Scientific paper

Day to day observations of interplanetary scintillation on ten strongly scintillating radio sources over a period of twelve months show that the power spectrum of the small scale irregularities flattens considerably at temporal frequencies ν < 0.5 Hz. This flattening defines a scale which increases uniformly between 0.1 and 1.0 a.u. from the Sun. The implication of this result will be discussed. Permanent address: The Radio Observatory, National Committee for Space Research, Haifa, Israel.

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