Plume-like structures of extinction clouds at 19 Saturn radii

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DC Field	Value	Language
dc.contributor.author	Vasundhara, R	-
dc.contributor.author	Bhattacharyya, J. C	-
dc.contributor.author	Rozario, M	-
dc.date.accessioned	2006-04-10T09:38:01Z	-
dc.date.available	2006-04-10T09:38:01Z	-
dc.date.issued	1986-12	-
dc.identifier.citation	BASI, Vol. 14, No. 4, pp. 232-235	en
dc.identifier.uri	http://hdl.handle.net/2248/922	-
dc.description.abstract	Observations of the occultation of the star SAO 158763 by Saturn's magnetospheric region around 19 Saturn radii on May 12, 1984 are compared with the observations by Mahra et al. (1985) of the same event. Certain disparities between the Naini Tal and Kavalur data suggest that the extinction signatures are likely to be caused by irregular density enhancements of ions, charged dust grains, or gas.	en
dc.format.extent	274049 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Saturn	en
dc.subject	Ring system	en
dc.title	Plume-like structures of extinction clouds at 19 Saturn radii	en
dc.type	Article	en
Appears in Collections:	BASI Publications J.C.Bhattacharyya (1982 - 1990)

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