Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/37609
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dc.contributor.authorRao, S P Manohar-
dc.contributor.authorRao, B Ramachandra-
dc.date.accessioned2016-11-25T09:25:21Z-
dc.date.available2016-11-25T09:25:21Z-
dc.date.issued1976-09-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/37609-
dc.description261-263en_US
dc.description.abstractThe results of the variation of the peak occurrence (evaluated as percentage) of sporadic-E during an ascending half-solar cycle with geomagnetic latitude are reported. It is seen that Es occurrence is maximum in low sunspot period for low and middle latitudes, and vice versa for equatorial and high latitudes. The southern latitudes, in particular, show a systematic decrease in E, occurrence with increase in geomagnetic latitude for all limiting frequencies of Es (fEs). An attempt is made to explain the above results on the basis of the Sq current system.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.05(3) [September 1976]en_US
dc.titleLatitude Variation of Peak E, Occurrences during a Half-Solar Cycleen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.05(3) [September 1976]

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