Comet Ikeya-Seki (1965) and the nature of the Interplanetary Medium During its Apparition

dc.contributor.author	Bappu, M. K. V
dc.contributor.author	Sivaraman, K. R
dc.date.accessioned	2004-11-11T05:57:51Z
dc.date.available	2004-11-11T05:57:51Z
dc.date.issued	1969-01
dc.identifier.citation	KOB No 187	en
dc.identifier.uri	http://hdl.handle.net/2248/21
dc.description.abstract	The effects of a solar wind on the different parts of a comet are discussed. In terms of the observations obtained of Comet Ikeya-Seki (1965f). The solar wind contribution to the formulation of the scattering agencies in the cometary nucleus is shown to be negligible. Isophotes of the coma in the light of the CN (0,0) emission band and Na 5893A derived from slitless spectra are presented. The heliocentric distance of the imterplanetary medium properties at different phases of the solar cycle.	en
dc.format.extent	185670 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Kodaikanal Observatory	en
dc.subject	Ikeya-Seki	en
dc.subject	Comet Ikeya-Seki	en
dc.title	Comet Ikeya-Seki (1965) and the nature of the Interplanetary Medium During its Apparition	en
dc.type	Article	en