Dependence of molecular dissociation equilibrium on magnetic field strength in sunspots

dc.contributor.author	Gaur, V. P.
dc.contributor.author	Pande, M. C.
dc.contributor.author	Tripathi, B. M.
dc.contributor.author	Joshi, G. C.
dc.date.accessioned	2011-12-07T09:21:53Z
dc.date.available	2011-12-07T09:21:53Z
dc.date.issued	1971
dc.identifier.uri	http://hdl.handle.net/123456789/875
dc.description.abstract	It is shown that the total number of CO, CN, C₂, UH, NH and CH molecules varies significantly with magnetic field strength in sunspots. The equivalent widths of two first overtone lines of CO belonging to 0-2 vibration-rotation band as a function of magnetic field strength are also given. It appears that upto 2500 gauss the equivalent widths change linearly with magnetic field strength.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	bac22-157
dc.subject	Sunspots, Magnetic Field Strength	en_US
dc.title	Dependence of molecular dissociation equilibrium on magnetic field strength in sunspots	en_US
dc.type	Article	en_US