Interplanetary scintillations of 3C 279 observed with the RATAN-600 radio telescope

Details Interplanetary scintillations of 3C 279 observed with the RATAN-600 radio telescope Interplanetary scintillations of 3C 279 observed with the RATAN-600 radio telescope

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..218s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Apr. 1980, p. 218-222.) Soviet Astronomy Letters, vol. 6, Mar.-Apr. 1980, p. 119-122

Astronomy and Astrophysics

Astronomy

1

Cosmic Plasma, Radio Astronomy, Radio Sources (Astronomy), Scintillation, Radio Telescopes, Solar Wind Velocity

Scientific paper

During 1976 and 1977, interplanetary scintillations of the radio source 3C 279 were observed at centimeter wavelengths with the RATAN-600. At gamma = 3.9 cm the scintillation index becomes saturated at solar distances of 4R from the sun. At the solar distance of 5 R the solar-wind velocity was 140 km/sec; at the solar distance of 10 R it rises to about 400 km/sec.

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