Radio images of the interplanetary turbulent plasma

Details Radio images of the interplanetary turbulent plasma Radio images of the interplanetary turbulent plasma

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56...96v&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, no. 1, 1979, p. 96-105. In Russian.

Astronomy and Astrophysics

Astronomy

5

Astronomical Maps, Interplanetary Medium, Radio Astronomy, Scintillation, Solar Wind, Geomagnetism, Graphs (Charts), Luminosity, Radio Telescopes, Solar Activity Effects, Turbulent Flow

Scientific paper

The results of the interplanetary scintillation daily observations of approximately 140 radio sources are given in the paper. The observations were carried out at the radiotelescope VLPA FIAN during 24 days in October-November 1975 and 6 days in April 1976. The maps (radio images) of interplanetary turbulent plasma are presented. The analysis of the maps reveals the presence of large-scale irregularities in the interplanetary plasma. The variability in large-scale structure of the interplanetary plasma is due mainly to transport of matter from the sun. A comparison of the scintillation with the geomagnetic activity index detected the presence of a straight connection between them.

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