Isotopic lines of SiO in sunspots

dc.contributor.author	Pande, M. C.
dc.contributor.author	Joshi, G. C.
dc.date.accessioned	2011-11-09T07:43:48Z
dc.date.available	2011-11-09T07:43:48Z
dc.date.issued	1978
dc.identifier.citation	This article is downloaded from ADS article service	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/858
dc.description.abstract	As the isotopic shift for the vibration rotation band is generally much larger than the isotopic shift for the corresponding electronic transitions and thus facilitating separation of isotopic lines, the vibration rotation bands of SiO may find use in the determination of isotopic abundance ratio Si²⁸:Si²⁹:Si³⁰. To help identify the isotopic lines of SiO the wavenumbers for Si²⁹O¹⁶ and Si³⁰O¹⁶ have been calculated with an uncertainty of ±0.05 cm¯¹.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	sp59-353
dc.subject	Isotropic lines, SiO, Sunspots	en_US
dc.title	Isotopic lines of SiO in sunspots	en_US
dc.type	Article	en_US