Differential rotation of coronal holes

dc.contributor.author	Shelke, R. N.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2010-03-05T05:15:32Z
dc.date.available	2010-03-05T05:15:32Z
dc.date.issued	1985
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/618
dc.description.abstract	Using KPNO helium 10830Å synoptic charts of Carrington rotation 1716 through 1739, and by assembling a time sequence representing single latitude zone, rotational properties of coronal holes for five zones of latitudes (±10°, ±20°-±40°, and ±40°-±60°) have been examined. It seems that the rotation period of coronal holes is a function of latitude, thus reflecting differential rotation of coronal holes.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	sp95-193
dc.subject	Coronal holes - The Sun	en_US
dc.title	Differential rotation of coronal holes	en_US
dc.type	Article	en_US