Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/19340
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dc.contributor.authorKane, R P-
dc.date.accessioned2013-06-24T09:39:31Z-
dc.date.available2013-06-24T09:39:31Z-
dc.date.issued2004-12-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://hdl.handle.net/123456789/19340-
dc.description358-366en_US
dc.description.abstractComparison of the evolutions of daily and monthly values of several solar indices during 1999-2002 indicated that the daily values had large day-to-day fluctuations with peak spacings differing considerably from the 27-day solar rotation period. Plots of the percentage increases (trough-to-peak) versus temperature of the source regions of the various indices indicated a double-humped structure. The monthly values showed many peaks. The average spacing was -3.5 months (-100 days). The 12-month moving averages showed considerable differences. Some indices reached a maximum near March 2000. Some of these decreased since then and continue to decrease at present; but some reached a minimum near January 2001 and remained steady there, or started increasing again to reach a probable maximum near June 2002. Some indices did not have a maximum in March 2000 and continued to increase till June 2002. Thus, the evolutions of the various solar indices during the sunspot maximum of cycle 23 (1999-2002) are substantially different from each other. Obviously, the dynamical upheavals in the photosphere reach upper levels of the solar atmosphere with varying intensities.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.relation.ispartof96.60 Qc; 96.60 Tf; 94.20 Vven_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.33(6) [December 2004]en_US
dc.subjectSolar indicesen_US
dc.subjectSunspot maximumen_US
dc.subjectSolar cycle 23en_US
dc.titleVariations of solar indices during the sunspot maximum years (1999-2002) of cycle 23en_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.33(6) [December 2004]

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