Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/14041
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dc.contributor.authorDhanya, R-
dc.contributor.authorGurubaran, S-
dc.contributor.authorSathishkumar, S-
dc.date.accessioned2012-05-02T10:02:36Z-
dc.date.available2012-05-02T10:02:36Z-
dc.date.issued2012-04-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://hdl.handle.net/123456789/14041-
dc.description271-284en_US
dc.description.abstractThe present study investigates the role of planetary-scale waves in the mesosphere-lower thermosphere-ionosphere (MLTI) coupling during the deep solar minimum period of 2005-2008. In the absence of severe magnetic disturbances, it is expected that much of the observed variations in low latitude ionospheric current system, the equatorial electrojet (EEJ), in particular, is expected to be driven by global scale waves propagating from below. The availability of continuous wind data from MF radar at mesospheric heights and geomagnetic field variations, the latter providing a measure of the strength of the ionospheric current system provides a unique opportunity to investigate the role of planetary-scale waves in driving the variabilities in the ionospheric current system during this solar minimum epoch. The study presents interesting findings on the role of planetary waves, especially the 3.5-day ultra-fast Kelvin wave and the 6.5-day wave in the low latitude MLTI coupling.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.relation.ispartof92.60.hb; 92.60.hcen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.41(2) [April 2012]en_US
dc.subjectMesosphere-lower thermosphere-ionosphere (MLTI) couplingen_US
dc.subjectEquatorial electrojet (EEJ), Planetary waveen_US
dc.subjectUltra fast Kelvin waves (UFK)en_US
dc.titlePlanetary wave coupling of the mesosphere-lower thermosphere-ionosphere (MLTI) region during deep solar minimum 2005-2008en_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.41(2) [April 2012]

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