Study of solar wind using single-station interplanetary scintillation

Details Study of solar wind using single-station interplanetary scintillation Study of solar wind using single-station interplanetary scintillation

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993basi...21..383m&link_type=abstract

Astronomical Society of India, Bulletin (ISSN 0304-9523), vol. 21, no. 3-4, p. 383-384

Astronomy and Astrophysics

Astronomy

1

Radio Sources (Astronomy), Scintillation, Solar Activity, Solar Wind, Solar Wind Velocity, Electron Density (Concentration), Turbulence, Variations

Scientific paper

This thesis is based on the study of interplanetary scintillation (IPS) measurements using compact radio sources. In this study, I have shown for the first time that the solar-wind velocities may be estimated reliably and routinely from single-station IPS observations via careful modeling of the interplanetary medium. The single-station velocity estimates show an excellent agreement with results from the simultaneous three-station measurements made at Nagoya, Japan. Based on the method of single-station velocity estimation, the three-dimensional structures of the solar-wind velocity during the minimum and maximum activity of the current solar cycle have been determined, and their evolution with the solar activity has been studied.

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