Long-Wavelength Observations of Jets from Polar Regions of the Sun

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3177

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DC Field	Value	Language
dc.contributor.author	Ramesh, R	-
dc.date.accessioned	2008-08-18T10:51:22Z	-
dc.date.available	2008-08-18T10:51:22Z	-
dc.date.issued	1999-10	-
dc.identifier.citation	Solar Physics, Vol. 189, No. 1, pp. 85 - 93	en
dc.identifier.issn	0038-0938	-
dc.identifier.uri	http://hdl.handle.net/2248/3177	-
dc.description	Restricted Access	en
dc.description.abstract	We report radio observations of enhanced emission associated with the extreme-ultraviolet (EUV) jets from polar coronal hole regions of the Sun, with the Gauribidanur radioheliograph (GRH). We have estimated the brightness temperature, electron density and mass of the ejected material. These jets were not accompanied by nonthermal radio bursts, particularly Type III events.	en
dc.format.extent	782717 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://www.springerlink.com/content/j272r51h30p27717/	en
dc.subject	X-ray jets	en
dc.subject	Radio emmission	en
dc.subject	coronal stremers	en
dc.subject	Telescopes	en
dc.subject	EIT	en
dc.title	Long-Wavelength Observations of Jets from Polar Regions of the Sun	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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