Dispersion analysis of scintillations for an extended medium

Details Dispersion analysis of scintillations for an extended medium Dispersion analysis of scintillations for an extended medium

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22..177l&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 22, Mar.-Apr. 1982, p. 177-181. In Russian.

Astronomy and Astrophysics

Astronomy

Dispersion, Interplanetary Medium, Scintillation, Solar Wind Velocity, Astronomical Models, Cross Correlation, High Frequencies, Magnetic Storms

Scientific paper

The paper examines the influence of the extent of the pertinent medium on the characteristic form of the dispersion dependence of interplanetary scintillations. Two models are considered: the spherically symmetric solar wind and a fast flux on the background of the spherically symmetric solar wind. It is shown that the dispersion curve in the high-frequency region is determined primarily by velocities in regions of the medium close to the observer.

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