1. IIA Institutional Repository
  2. Publications of Astronomical Society of India
  3. BASI Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/344
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSinha, K-
dc.date.accessioned2005-02-09T04:22:27Z-
dc.date.available2005-02-09T04:22:27Z-
dc.date.issued1982-09-
dc.identifier.citationBASI, Vol. 10, No. 3, pp. 223-233en
dc.identifier.urihttp://hdl.handle.net/2248/344-
dc.description.abstractThe line intensities of the umbral MgH molecules reported by Sotirovski (1971) are re-analysed utilizing the latest laboratory data. It appears probable that because of a neglect of the role of blurring in producing stray light, Sotirovski's (1971) results are under estimated. The need of a laboratory check upon the theoretical oscillator strengths of the weak bands (Triangle Nu not = 0) calculated by Kirby et al. (1979) is steressed.en
dc.format.extent747480 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectsunspot umbraeen
dc.subjectMgHen
dc.titleOn MgH line intensities in sunspot unbraeen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
SINHA.pdf729.96 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.