Analysis of the Non-Gaussian Spectra of Interplanetary Scintillations

Details Analysis of the Non-Gaussian Spectra of Interplanetary Scintillations Analysis of the Non-Gaussian Spectra of Interplanetary Scintillations

Dec 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..19..271a&link_type=abstract

Astrophysics and Space Science, Volume 19, Issue 2, pp.271-278

Astronomy and Astrophysics

Astrophysics

Scientific paper

The non-Gaussian intensity fluctuation spectra observed by Cohenet al. (1967) are analysed. Computations of the length scales derived from the phase autocorrelation functions using Buckley's method (1971, I) indicate that for a rms phase deviation of 4 radians or more the diffracting medium behaves as one with its phase structure having ‘inner’ and ‘outer’ scales of turbulent blobs or eddies which are present in a turbulent medium.

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