Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/37714
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dc.contributor.authorSastri, J. Hanumath-
dc.date.accessioned2016-11-28T06:51:08Z-
dc.date.available2016-11-28T06:51:08Z-
dc.date.issued1975-09-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/37714-
dc.description225-227en_US
dc.description.abstractEvidence is presented from normal run magnetogram data of Huancayo, Kodaikanal and Kakioka to show that geomagnetic solar flare effect (SFE or Crochet, occurs not only in the sunlit hemisphere but also in dark hemisphe reo Using a selected sample of five events observed over the period 1969-71, it is noticed that discrepancy exists between the observed characteristics of nighttime geomagnetic SFE and those expected from the interpretation that the nighttime geomagnetic SFE is due to induced currents that are forced to flow into the ,dark. hemisphere owing to the sudden increase in electrical conductivity of the sunlit hemisphere. This discrepancy may be due to some of the inherent assumptions of the theoretical model used .for calculating the characteristics of induced currents in the dark hemisphere.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.04(3) [September 1975]en_US
dc.titleGeomagnetic Solar Flare Effect in the Dark Hemisphereen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.04(3) [September 1975]

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