5303Å Coronal Irradiance and Its Relation to the Photospheric Magnetic Activity

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3208

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DC Field	Value	Language
dc.contributor.author	Ramesh, K. B	-
dc.date.accessioned	2008-08-20T10:19:41Z	-
dc.date.available	2008-08-20T10:19:41Z	-
dc.date.issued	1998-12	-
dc.identifier.citation	Solar Physics, Vol. 183, No. 2, pp. 295 - 303	en
dc.identifier.issn	0038 - 0938	-
dc.identifier.uri	http://hdl.handle.net/2248/3208	-
dc.description	Restricted Access	en
dc.description.abstract	The association of Lomnický Štít data of coronal green line irradiance (CI) to photospheric magnetic activity is studied for the years 1975-1994 using the Carrington rotation averaged photospheric magnetic flux data. It is found that the CI correlates well with photospheric magnetic flux of active regions and the total disk-integrated magnetic flux on longer time scales (11-year solar cycle) and fails (about 50% of the time) to show a strong dependence on shorter time scales. A comparison of the association of CI and of the 10.7cm radio flux with the photospheric magnetic flux data indicated that the CI might basically represent the background coronal irradiance.	en
dc.format.extent	92342 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://dx.doi.org/10.1023/A:1005069100527	en
dc.subject	Coronal Green Line Irradiance	en
dc.subject	Photospheric Magnetic Activity	en
dc.title	5303Å Coronal Irradiance and Its Relation to the Photospheric Magnetic Activity	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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