Investigation of scintillations in near-solar regions of the interplanetary medium

Details Investigation of scintillations in near-solar regions of the interplanetary medium Investigation of scintillations in near-solar regions of the interplanetary medium

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23..361b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, May-June 1983, p. 361-366. In Russian.

Astronomy and Astrophysics

Astronomy

2

Interplanetary Medium, Interstellar Masers, Radio Sources (Astronomy), Scintillation, Solar Wind, Centimeter Waves, Plasma Acceleration, Point Sources, Radial Distribution, Solar Wind Velocity, Supersonic Flow, Water Masers

Scientific paper

A technique based on the study of scintillations of water-vapor maser sources has been developed for investigating the solar wind. The radial dependence of the scintillation index is investigated at a wavelength of 1.35 cm in the regime of weak scintillations for a point source near the sun, i.e., about 10 solar radii from the sun. The existence of a region of high values of the scintillation index is detected, this region being identified with the region of supersonic-flow formation.

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