Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/36693
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dc.contributor.authorRangarajan, G K-
dc.contributor.authorMurty, A V S-
dc.date.accessioned2016-11-03T06:57:29Z-
dc.date.available2016-11-03T06:57:29Z-
dc.date.issued1984-10-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/36693-
dc.description154-158en_US
dc.description.abstractDay-to-day variability in the ionospheric component of the equatorial electroject strength is not dependent on either the degree of magnetic disturbance or the polarity of interplanetary magnetic field except for the solar maximum year 1969. The time of maximum of equatorial electrojet field shifts to earlier part of the day with enhanced strength. The diurnal variations of the ionospheric component at low and equatorial latitudes are similar in pattern from month to month but the day-to-day variability at individual hours are negatively, though poorly, correlated.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.13(5) [October 1984]en_US
dc.titleVariability of the Ionospheric Component of the Equatorial Geomagnetic Fielden_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.13(5) [October 1984]

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