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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/328
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dc.contributor.authorAnanthakrishnan, S-
dc.contributor.authorKaufman, J. J-
dc.date.accessioned2005-02-08T13:25:30Z-
dc.date.available2005-02-08T13:25:30Z-
dc.date.issued1982-03-
dc.identifier.citationBASI, Vol. 10, No.1, pp. 1-15en
dc.identifier.urihttp://hdl.handle.net/2248/328-
dc.description.abstractSolar wind velocity estimation using the method of multi-station interplanetary scintillation observations has been reviewed. It is shown that the interred model for the electron density fluctuations in the solar wind differs significantly from that for the proton density. The high latitude solar wind has a strong correlation with the presence of coronal hole regions.en
dc.format.extent1350733 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectsolar winden
dc.subjectintensity scintillationen
dc.subjectcoronal holesen
dc.titleMulti-station observations of interplanetary scintillationsen
dc.typeArticleen
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