Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1313
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dc.contributor.authorSinha, K-
dc.contributor.authorTripathi, B. M-
dc.date.accessioned2006-11-27T06:14:14Z-
dc.date.available2006-11-27T06:14:14Z-
dc.date.issued1990-03-
dc.identifier.citationBASI, Vol. 18, No. 1 & 2, pp. 33-78en
dc.identifier.urihttp://hdl.handle.net/2248/1313-
dc.description.abstractThe partial pressures of 20 ionic molecular species are reported for standard facular, photospheric, and sunspot model atmospheres with a view to picking up ionized molecules for a possible identification in the solar spectrum. Comparing the partial pressures with those of the molecule SiH(+), which is already detected in the solar spectrum, it appears probable that additional ionic species can be identified in the same spectrum. To predict the line intensities of such species, accurate values of oscillator strengths and dissociation energies are neededen
dc.format.extent3147980 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectIonic speciesen
dc.subjectSolar spectrumen
dc.subjectSolar atmosphereen
dc.titleOn ionized molecules in the solar atmosphereen
dc.typeArticleen
Appears in Collections:BASI Publications

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