Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4062
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dc.contributor.authorMurty, P. S-
dc.date.accessioned2008-12-15T14:57:35Z-
dc.date.available2008-12-15T14:57:35Z-
dc.date.issued1979-08-
dc.identifier.citationSolar Physics, Vol. 63, No.1, pp. 83 - 85en
dc.identifier.issn0038-0938 (Print) 1573-093X (Online)-
dc.identifier.urihttp://hdl.handle.net/2248/4062-
dc.descriptionOpen Access-
dc.description.abstractFor use in the investigations of magnesium monoxide lines in sunspot spectra, values of Franck-Condon intensity factors for the red bands and the wavelength regions for the intense bands of the red and near-ultraviolet transitions of MgO are presented. The results indicate that a search for the lines of the red and near-ultraviolet bands in the sunspot spectra could resolve the questionable presence of MgO in sunspots.en
dc.language.isoenen
dc.publisherD. Reidel Publishing Companyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1979SoPh...63...83Men
dc.relation.urihttp://dx.doi.org/10.1007/BF00155697en
dc.rightsD. Reidel Publishing Company-
dc.subjectMagnesium Oxidesen
dc.subjectSolar Spectraen
dc.subjectSunspotsen
dc.subjectFranck-Condon Principleen
dc.subjectNear Ultraviolet Radiationen
dc.subjectSpectral Line Widthen
dc.titleOn magnesium monoxide lines in sunspot spectraen
dc.typeArticleen
Appears in Collections:IIAP Publications

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