Multi-station observations of interplanetary scintillations

dc.contributor.author	Ananthakrishnan, S
dc.contributor.author	Kaufman, J. J
dc.date.accessioned	2005-02-08T13:25:30Z
dc.date.available	2005-02-08T13:25:30Z
dc.date.issued	1982-03
dc.identifier.citation	BASI, Vol. 10, No.1, pp. 1-15	en
dc.identifier.uri	http://hdl.handle.net/2248/328
dc.description.abstract	Solar 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.extent	1350733 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	solar wind	en
dc.subject	intensity scintillation	en
dc.subject	coronal holes	en
dc.title	Multi-station observations of interplanetary scintillations	en
dc.type	Article	en