UV astronomy and stellar chromosphere

dc.contributor.author	Kameswara Rao, N
dc.date.accessioned	2021-02-14T06:01:21Z
dc.date.available	2021-02-14T06:01:21Z
dc.date.issued	1995
dc.identifier.citation	Sinha,B and Bhattacharya, M eds, From Astronomy to Astrophysics:Proceedings of symposium on Astronomy and Astrophysics, pp. 149 - 170	en_US
dc.identifier.uri	http://hdl.handle.net/2248/7622
dc.description	© Saha Institute of Nuclear Physics	en_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.iso	en	en_US
dc.publisher	Saha Institute of Nuclear Physics	en_US
dc.subject	UV Astronomy	en_US
dc.subject	Solar UV Spectrum	en_US
dc.subject	Chromospheric & Coronal Studies	en_US
dc.title	UV astronomy and stellar chromosphere	en_US
dc.type	Book chapter	en_US