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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2249
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dc.contributor.authorBarman, S. K-
dc.contributor.authorKariyappa, R-
dc.date.accessioned2008-04-22T09:48:13Z-
dc.date.available2008-04-22T09:48:13Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 245 - 247en
dc.identifier.urihttp://hdl.handle.net/2248/2249-
dc.description.abstractEmploying a law of weak acoustic wave, the ratio of population density N2/N1 with time for the Ca II H and K lines appropriate for the solar quiet chromosphere have been calculated. This has been done by solving the equations of radiative transfer and statistical equilibrium for two level plus continuum atom simultaneously. From the calculation it has been shown that even a small deposit of weak acoustic wave energy can enhance the emission peak of resonance lines.en
dc.format.extent187911 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar quiet chromosphereen
dc.subjectWeak shock waveen
dc.subjectLevel population densityen
dc.subjectTimeen
dc.titleChange of level population density with time in the solar quiet chromospheric atmosphereen
dc.typeArticleen
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