Interplanetary plasma, according to radioastronomical data

Details Interplanetary plasma, according to radioastronomical data Interplanetary plasma, according to radioastronomical data

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ge%26ae..19..401v&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 19, May-June 1979, p. 401-424.) Geomagnetism and Aeronomy, vol. 19, Dec. 1979, p. 269-282. Tra

Astronomy and Astrophysics

Astronomy

13

Cosmic Plasma, Interplanetary Medium, Radio Astronomy, Solar Wind, Electron Density Profiles, Heterogeneity, Radio Scattering, Solar Activity, Solar Corona, Turbulence Effects, Velocity Distribution, Velocity Measurement, Wave Propagation

Scientific paper

The general features of radio-astronomical measurements of the interplanetary plasma are briefly reviewed with emphasis on radio wave scattering, radio source scintillations, and plasma velocity measurements. A survey is then presented of two principal aspects of the interplanetary plasma, as observed by radio astronomy: (1) turbulence spectra and (2) large scale structure. Some recommendations for future radio-astronomical exploration of the interplanetary medium are presented.

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