Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/37977
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSrivastava, B. J.-
dc.contributor.authorAbbas, Habiba-
dc.date.accessioned2016-12-01T07:06:22Z-
dc.date.available2016-12-01T07:06:22Z-
dc.date.issued1973-09-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/37977-
dc.description177-179en_US
dc.description.abstractThe rise-times of SSCs are found to range from 1 to 8 min and the amplitudes from 5 to 100 γ. An inverse relationship (negative correlation) has been obtained between the rise-time and the amplitude of SSCS at Hyderabad, similar to Alibag and Hermanus, but quite different from that observed for Budkov where a direct relationship (positive correlation) has been reported. SSC* events which are very rare at Hyderabad, are observed only during daytime and correspond to prominent events in the equatorial electrojet region. At high-latitude stations like Hartland, Eskdalemuir and Lerwick, SSC*s are observed both during day and night hours. The implications of these observations are examined. The observed association of micro-pulsations with SSCs and SSC*s is also discussed.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.02(3) [September 1973]en_US
dc.titleSome Aspects of SSCs Observed at Hyderabad during 1965-72en_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.02(3) [September 1973]

Files in This Item:
File Description SizeFormat 
IJRSP 2(3) 177-179.pdf292.67 kBAdobe PDFView/Open


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