Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/3923
Full metadata record
DC FieldValueLanguage
dc.contributor.authorGupta, Meera-
dc.contributor.authorMishra, V K-
dc.contributor.authorTiwari, D P-
dc.contributor.authorMishra, A P-
dc.date.accessioned2009-04-21T03:49:59Z-
dc.date.available2009-04-21T03:49:59Z-
dc.date.issued2006-10-
dc.identifier.issn0367-8393-
dc.identifier.urihttp://hdl.handle.net/123456789/3923-
dc.description324-326en_US
dc.description.abstractA minimum between solar cycle 22 and 23 has been defined earlier on the basis of type-I radio burst only. In the present paper a re-visit to the occurrence of type-I radio bursts in relation to general level of solar activity (sunspot number) is made covering the minima of cycle 21 to complete cycles 22-23. The study shows that, it is not appropriate to speculate solar cycle minima on the basis of type-I radio burst only.en_US
dc.language.isoen_USen_US
dc.publisherCSIRen_US
dc.sourceIJRSP Vol.35(5) [October 2006]en_US
dc.subjectType-I radio bursten_US
dc.subjectSolar cycleen_US
dc.subjectSolar activityen_US
dc.subjectSunspot numberen_US
dc.titleOccurrence of type-I radio bursts and their association with solar cycleen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.35(5) [October 2006]

Files in This Item:
File Description SizeFormat 
IJRSP 35(5) 324-326.pdf85.03 kBAdobe PDFView/Open


Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.