Solar wind observations using interplanetary scintillations

Details Solar wind observations using interplanetary scintillations Solar wind observations using interplanetary scintillations

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ijrsp..19..519a&link_type=abstract

Indian Journal of Radio and Space Physics (ISSN 0367-8393), vol. 19, Oct.-Dec. 1990, p. 519-524.

Physics

Space Physics

Interplanetary Space, Radio Spectra, Scintillation, Solar Wind Velocity, Radio Telescopes, Velocity Measurement

Scientific paper

Solar wind velocities can be estimated from high signal-to-noise interplanetary scintillation spectra obtained from a single radio telescope. The magnitudes of the velocity estimates correlate well with 3-station measurements. This is a convenient method to study many large scale interplanetary phenomena in and out of the ecliptic and over a large range of heliocentric distances.

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