Coronal Electron Density and the Gradient of Coronal Rotation with Altitude

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2401

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DC Field	Value	Language
dc.contributor.author	Vats, H. O	-
dc.date.accessioned	2008-06-05T07:06:37Z	-
dc.date.available	2008-06-05T07:06:37Z	-
dc.date.issued	2003	-
dc.identifier.citation	BASI, Vol. 31, No. 3&4, pp. 309 - 311	en
dc.identifier.uri	http://hdl.handle.net/2248/2401	-
dc.description.abstract	The calculations of the gradient of coronal rotation period with altitude were performed using electron density model and the radio measurements of solar coronal rotation. The magnitude of the gradient reduces if the emission is at higher harmonics of the plasma frequency. The results seem to reduce the difference in the radio and optical measurements of coronal rotation.	en
dc.format.extent	86960 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2003BASI...31..309V	en
dc.subject	Solar rotation	en
dc.subject	Coronal Rotation	en
dc.subject	Electron density model	en
dc.subject	Gradient of rotation period	en
dc.title	Coronal Electron Density and the Gradient of Coronal Rotation with Altitude	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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