Photometry of the solar corona of March 7, 1970

dc.contributor.author	Bappu, M. K. V
dc.contributor.author	Bhattacharyya, J. C
dc.contributor.author	Sivaraman, K. R
dc.date.accessioned	2009-05-19T14:29:34Z
dc.date.available	2009-05-19T14:29:34Z
dc.date.issued	1973
dc.identifier.citation	Pramana, Vol. 1, No. 3, pp. 117 - 128	en
dc.identifier.uri	http://hdl.handle.net/2248/4465
dc.description	Open Access	en
dc.description.abstract	Isophotes obtained by equidensitometry techniques from four exposures of the March 7, 1970 corona are used for derivation of intensity distributions along the equator, poles, streamers and dark ' gaps ' in the visible corona. The distributions differ from the van de Hulst curves for a maximum corona. The Kodaikanal measures agree well with the NRL measures of the outer corona made from a rocket coronagraph and together provide data from 1.2R0 to 8-ORo along the solar equator. Radial intensity gradients for different position angles and €he LudendorfF parameters obtained, characterize this corona as typical of the solar maximum.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://www.ias.ac.in/pramana/	en
dc.rights	© Indian Academy of Sciences	en
dc.subject	Solar Corona	en
dc.subject	Solar Eclipse	en
dc.subject	Coronal Photometry	en
dc.title	Photometry of the solar corona of March 7, 1970	en
dc.type	Article	en