Asymmetry in cross correlation functions of strong and weak interplanetary scintillations

Details Asymmetry in cross correlation functions of strong and weak interplanetary scintillations Asymmetry in cross correlation functions of strong and weak interplanetary scintillations

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975rael...20r1777l&link_type=abstract

(Radiotekhnika i Elektronika, vol. 20, Sept. 1975, p. 1777-1783.) Radio Engineering and Electronic Physics, vol. 20, Sept. 1975,

Astronomy and Astrophysics

Astronomy

2

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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