Measurements of compact radio source size and structure of cometary ion tails using interplanetary scintillation at 103 MHz

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1508

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DC Field	Value	Language
dc.contributor.author	Janardhan, P	-
dc.date.accessioned	2007-05-04T10:49:52Z	-
dc.date.available	2007-05-04T10:49:52Z	-
dc.date.issued	1993	-
dc.identifier.citation	BASI, Vol. 21, pp. 381	en
dc.identifier.uri	http://hdl.handle.net/2248/1508	-
dc.description.abstract	The work contained in this thesis was carried out at the Physical Research Laboratory, Ahmedabad and describes observations of Interplanetary Scintillation (IPS), carried out since 1984, using a large 10,000 sq m dipole array operating to 103 MHz. During the period of research the array underwent an expansion to 20,000 sq m and the later part of the observations were carried out using the enhanced array.	en
dc.format.extent	87803 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Comet tails	en
dc.subject	Radio astronomy	en
dc.title	Measurements of compact radio source size and structure of cometary ion tails using interplanetary scintillation at 103 MHz	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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