Intensity Fluctuation in the Solar Chromosphere

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