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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2593
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dc.contributor.authorVenkatakrishnan, P-
dc.date.accessioned2008-07-09T08:09:51Z-
dc.date.available2008-07-09T08:09:51Z-
dc.date.issued1993-12-
dc.identifier.citationSolar physics , Vol. 148, No. 2, pp. 233 - 238en
dc.identifier.urihttp://hdl.handle.net/2248/2593-
dc.description.abstractThe time-averaged equivalent width of the He 1 10830 Angstrom line is seen to be correlated with the time-averaged line width. This correlation is interpreted as evidence for the association of the chromospheric energy density with the heating of overlying coronaen
dc.format.extent632711 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/t54171037r3p4566/en
dc.relation.urihttp://adsabs.harvard.edu/abs/1993SoPh..148..233Ven
dc.subjectChromosphereen
dc.subjectCoronaen
dc.titleCoronal heating and chromospheric energy density: An observational associationen
dc.typeArticleen
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