Broad Band Photometry of the Solar Corona of 1983, June 11

dc.contributor.author	Sivaraman, K. R
dc.contributor.author	Singh, J
dc.contributor.author	Kapoor, R. C
dc.contributor.author	Kariyappa, R
dc.date.accessioned	2005-05-18T07:01:54Z
dc.date.available	2005-05-18T07:01:54Z
dc.date.issued	1985-11
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 5, No. 1, pp. 31-36	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/399
dc.description.abstract	The solar corona was photographed at an effective wavelength of 6300A during the total eclipse of 1983, June 11 at Indonesia. From the isophotes of the corona, the intensity distributions along the equator, poles, streamers and gaps have been derived. The intensity along the equatorial and polar directions can be represented well by a 19/sup0/ polynomial. The brightness distribution and the Ludendorff parameters of this corona are typical of the intermediate phase of the solar cycle	en
dc.format.extent	173302 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar Corona	en
dc.subject	Solar Eclipse	en
dc.subject	Coronal Photometry	en
dc.title	Broad Band Photometry of the Solar Corona of 1983, June 11	en
dc.type	Article	en