A Overview of Interplanetary Scintillation Method for Studying Solar Wind Physics

Details A Overview of Interplanetary Scintillation Method for Studying Solar Wind Physics A Overview of Interplanetary Scintillation Method for Studying Solar Wind Physics

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jass....5..123k&link_type=abstract

Journal of Astronomy and Space Science, vol. 5, no. 2, p. 123-127.

Astronomy and Astrophysics

Astronomy

Scientific paper

Interplanetary scintillation is the fluctuation produced in the apparent brightness of a radio source, due to refractive effects in the turbulent solar wind flowing from the sun. If this medium is illuminated coherently, analysis of the spatial and temporal properties of the radiation reaching the earth allows the stochastic properties of the medium to be understood. Here, a brief review of method of interplanetary scintillation to study solar wind behavior will be introduced.

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