Three-station observations of interplanetary scintillation at 327 MHz. I

Details Three-station observations of interplanetary scintillation at 327 MHz. I Three-station observations of interplanetary scintillation at 327 MHz. I

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984prian..31....1k&link_type=abstract

Nagoya University, Research Institute of Atmospherics, Proceedings (ISSN 0077-264X), vol. 31, March 1984, p. 1-10.

Physics

1

Scintillation, Solar Wind Velocity, Velocity Measurement, Magnetic Dipoles, Solar Magnetic Field, Solar Rotation, Velocity Distribution

Scientific paper

Regular observations of interplanetary scintillation at 327 MHz have been started with a new three-station system. This paper is a preliminary report of the observations. The distribution of the solar wind velocity in heliographic latitude and longitude on the solar surface in March-June 1982 has been derived. In the Northern Hemisphere, the polar high-speed region with a uniformly high (800 km/s) speed at all latitudes above 45 degrees, such as that observed in 1974-1976, was not yet developed in early 1982.

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