On the Polar Coronal Rays of the Sun

dc.contributor.author	Bhatnagar, A
dc.contributor.author	Raheem, K. C. A
dc.date.accessioned	2006-04-06T07:03:25Z
dc.date.available	2006-04-06T07:03:25Z
dc.date.issued	1970-10
dc.identifier.citation	KOB No 204	en
dc.identifier.uri	http://hdl.handle.net/2248/830
dc.description.abstract	A study of the polar coronal rays made on two eclipse photographs is presented. From the frequency distribution of polar rays, it is shown that the maximum distribution of polar rays occurs in an annular zone arround 10/supo/ from the poles and a minimum at the poles. From the orientation of the polar rays the length of the hypothetical bar magnet has been determined. A variation in the length of the hypothetical bar magnet with the phase of solar activity cycle is confirmed.	en
dc.format.extent	658531 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Kodaikanal Observatory	en
dc.subject	Polar Coronal Rays	en
dc.title	On the Polar Coronal Rays of the Sun	en
dc.type	Article	en