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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/830
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dc.contributor.authorBhatnagar, A-
dc.contributor.authorRaheem, K. C. A-
dc.date.accessioned2006-04-06T07:03:25Z-
dc.date.available2006-04-06T07:03:25Z-
dc.date.issued1970-10-
dc.identifier.citationKOB No 204en
dc.identifier.urihttp://hdl.handle.net/2248/830-
dc.description.abstractA 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.extent658531 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherKodaikanal Observatoryen
dc.subjectPolar Coronal Raysen
dc.titleOn the Polar Coronal Rays of the Sunen
dc.typeArticleen
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