Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/11192
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dc.contributor.authorKane, R P-
dc.date.accessioned2011-03-14T06:13:05Z-
dc.date.available2011-03-14T06:13:05Z-
dc.date.issued2011-02-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://hdl.handle.net/123456789/11192-
dc.description7-10en_US
dc.description.abstractDuring the sunspot minimum years 2007-2009 of solar cycle 23, the sunspot number, Rz, declined from January 2007 till the end of 2007 and further till September 2009. But in between, there were sporadic increases during January, June, December 2007; March 2008; and September 2009. These were reflected very well in timing in the 2800 MHz solar radio emission flux F-10, X-ray background, and the occurrence frequency of coronal mass ejections (CME). Thus, all these have a major origin in the same active regions.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.relation.ispartof96.60.ph; 96.60.qden_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.40(1) [February 2011]en_US
dc.subjectSolar activityen_US
dc.subjectSunspot numberen_US
dc.subjectSolar radio emission fluxen_US
dc.subjectCoronal mass ejection (CME)en_US
dc.titleSolar activity during sunspot minimumen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.40(1) [February 2011]

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