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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4146
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dc.contributor.authorSivaraman, K. R-
dc.date.accessioned2008-12-19T14:32:09Z-
dc.date.available2008-12-19T14:32:09Z-
dc.date.issued1982-03-
dc.identifier.citationAstrophysical Journal, Part 1, Vol. 254, pp. 814 - 815en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/4146-
dc.description.abstractThe K2V/K2R asymmetry in the self-reversed emission peaks of the Ca II K line in the sun is the result of the redward displacement of K3. This redward displacement is explained as caused by the dark condensations in K3 and not due to the supergranulation flow pattern. Arguments are presented to show that such asymmetries in the spectra of stars provide evidence for the presence of these structures in their chromospheresen
dc.language.isoenen
dc.publisherThe American Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1982ApJ...254..814Sen
dc.rights©The American Astronomical Societyen
dc.subjectCalcium, Chromosphereen
dc.subjectEmission Spectraen
dc.subjectK Linesen
dc.subjectRed Shiften
dc.subjectSolar Spectraen
dc.subjectStellar Spectraen
dc.subjectVisible Spectrumen
dc.subjectAsymmetryen
dc.subjectOptical Emissionen
dc.subjectSpectroscopyen
dc.titleK2V/K2R asymmetries in the sun and starsen
dc.typeArticleen
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