Doppler width of CH lines

dc.contributor.author	Punetha, L. M.
dc.contributor.author	Joshi, G. C.
dc.date.accessioned	2010-01-19T05:53:08Z
dc.date.available	2010-01-19T05:53:08Z
dc.date.issued	1991
dc.identifier.citation	this article is downloaded from ADS article services	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/454
dc.description.abstract	Twenty-one CH line profile at the centre of the solar disk were Fourier-transformed to derice the Doppler widths. The Doppler width increases linearly with the equivalent width.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass181-327
dc.subject	CH lines	en_US
dc.title	Doppler width of CH lines	en_US
dc.type	Article	en_US