The asymmetry of the cross-correlation function of strong and weak scintillations in the interplanetary medium

Details The asymmetry of the cross-correlation function of strong and weak scintillations in the interplanetary medium The asymmetry of the cross-correlation function of strong and weak scintillations in the interplanetary medium

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975rael...20q1777l&link_type=abstract

Radiotekhnika i Elektronika, vol. 20, Sept. 1975, p. 1777-1783. In Russian.

Astronomy and Astrophysics

Astronomy

Interplanetary Medium, Radio Sources (Astronomy), Scintillation, Solar Wind Velocity, Anisotropic Media, Cross Correlation, Velocity Distribution

Scientific paper

The paper examines the effect of the velocity distribution of inhomogeneities - on the line of sight - on the form of the cross-correlation function of the interplanetary scintillations of radio sources. The dependence of the asymmetry of the cross-correlation function on the parameters which characterize the velocity structure of the solar wind is established. It is shown that the transition from saturated to weak scintillations does not affect this asymmetry.

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