Intensity Fluctuation in the Solar Chromosphere

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/70

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.contributor.author	Venkitachalam, P. P	-
dc.date.accessioned	2004-11-30T11:51:47Z	-
dc.date.available	2004-11-30T11:51:47Z	-
dc.date.issued	1977	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 2, pp. 34-41	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/70	-
dc.description.abstract	High resoulution spectrograms of the Balmer lines obtained at five positions from the centres to the limb have been used to study the r. m. s. intensity fluctuations and their dependence on the heliocentric angle. The intensity fluctuations at the line centre as well as several wavelength positions within the lines have been derived and the variation of these fluctuations within the lines have been studies.	en
dc.format.extent	216220 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Balmer Lines	en
dc.subject	Intensity Fluctuations	en
dc.subject	Solar Chromosphere	en
dc.title	Intensity Fluctuation in the Solar Chromosphere	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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