Research of solar wind by observations of radio wave propagation.

Details Research of solar wind by observations of radio wave propagation. Research of solar wind by observations of radio wave propagation.

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pabei..12...30m&link_type=abstract

Prog. Astron., Vol. 12, No. 1, p. 30 - 41

Physics

Solar Wind: Interplanetary Matter, Solar Wind: Structure, Solar Wind: Acceleration

Scientific paper

The results of 30 years study of solar wind using the method of radio wave scattering are reviewed, with emphasis on the interplanetary scintillation (IPS). The principal theory of radio wave propagation and its application to various observations are outlined. The electron density spectrum and solar cycle evolution of the three-dimensional solar wind structure are discussed. The results confirm the important role of scintillation measurements in studying the acceleration of solar wind. Consulting the International Solar-Terrestrial Physics Program, this review also points out major research topics of solar wind in 1990s. Finally, the feature of Miyun Synthesis Radio Telescope of Beijing Astronomical Observatory and its possibility in making IPS measurements are briefly described.

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