Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.244..691m&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 244, June 15, 1990, p. 691-695.
Astronomy and Astrophysics
Astronomy
48
Diffraction Patterns, Interplanetary Medium, Plasma-Electromagnetic Interaction, Radio Sources (Astronomy), Scintillation, Solar Wind Velocity, Fresnel Diffraction, Plasma Spectra, Power Spectra
Scientific paper
A method for determining the solar-wind velocity using single-station interplanetary-scintillation observations of compact radio sources in the weak-scattering region. This is achieved by fitting a model to the observed scintillation power spectra. The velocities obtained from single-station measurements have been compared with those from three-station observations and good agreement is found. In the presence of high-speed streams along the the line-of-sight, the single-station measurements tend to give the velocity of the stream.
Ananthakrishnan S.
Manoharan Periasamy K.
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