Solar-wind velocity measurement by radio observations of phenomena propagated through the interplanetary plasma

Details Solar-wind velocity measurement by radio observations of phenomena propagated through the interplanetary plasma Solar-wind velocity measurement by radio observations of phenomena propagated through the interplanetary plasma

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..289v&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, June 1979, p. 289-293.) Soviet Astronomy Letters, vol. 5, May-June 1979, p. 154-156.

Astronomy and Astrophysics

Astronomy

Interplanetary Medium, Radio Observation, Scintillation, Solar Wind Velocity, Velocity Measurement, Plasma Density, Radio Sources (Astronomy)

Scientific paper

The velocity of the solar wind can be measured with a single radio telescope by observing the interplanetary scintillation of numerous radio sources. The mean solar-wind velocity in August-October 1976 is found to have been approximately 400 km/sec at low heliographic latitudes (below 10 deg) and about 850 km/sec at high latitudes (30-70 deg). The wind velocity and the interplanetary plasma density have a reciprocal relationship.

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