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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7622
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dc.contributor.authorKameswara Rao, N-
dc.date.accessioned2021-02-14T06:01:21Z-
dc.date.available2021-02-14T06:01:21Z-
dc.date.issued1995-
dc.identifier.citationSinha,B and Bhattacharya, M eds, From Astronomy to Astrophysics:Proceedings of symposium on Astronomy and Astrophysics, pp. 149 - 170en_US
dc.identifier.urihttp://hdl.handle.net/2248/7622-
dc.description© Saha Institute of Nuclear Physicsen_US
dc.description.abstract"The abrupt termination of solar and stellar spectrum below A 2900 has been a great handicap to the advancement of our knowledge of the heavenly bodies ; because the information gained from the study of the spectrum beyond A, 2900 is not sufficient 'to explain the problems of stellar mechanisms operative there."en_US
dc.language.isoenen_US
dc.publisherSaha Institute of Nuclear Physicsen_US
dc.subjectUV Astronomyen_US
dc.subjectSolar UV Spectrumen_US
dc.subjectChromospheric & Coronal Studiesen_US
dc.titleUV astronomy and stellar chromosphereen_US
dc.typeBook chapteren_US
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