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Coronal holes and flare index: A Correlation Study

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dc.contributor.author Joshi, A.
dc.date.accessioned 2009-08-19T10:21:05Z
dc.date.available 2009-08-19T10:21:05Z
dc.date.issued 2000
dc.identifier.uri http://hdl.handle.net/123456789/284
dc.description.abstract The correlation between the presence of coronal holes and flare indices has been inves- tigated for the period from 1976 to 1995. The analysis shows that in the cases of 227 Carrington rotations (CRs) backward time lags yield the highest correlation between the coronal holes and flare indices. The maximum correlations were found at time lags of 222 and 142 CRs for polar and equatorial coronal holes, respectively. The period of study covers the past two solar cycles (21 and 22). Correlation analysis of both solar cycles has also been studied individually. The correlation analysis reveals that there is in general a forward shift in the maximum correlation for polar coronal holes, but it cannot be recommended to use polar coronal hole numbers for forecasting the next solar cycle. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries sp198-149
dc.subject Coronal holes, Flare, en_US
dc.title Coronal holes and flare index: A Correlation Study en_US
dc.type Article en_US


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