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dc.contributor.authorDevi, Rajni
dc.contributor.authorDubey, Smita
dc.contributor.authorSaini, Shailendra
dc.contributor.authorDevi, Babita
dc.contributor.authorDhar, Ajay
dc.contributor.authorVijay, S.K.
dc.contributor.authorGwal, A.K.
dc.date.accessioned2015-09-19T07:20:41Z
dc.date.accessioned2021-02-12T08:52:51Z-
dc.date.available2015-09-19T07:20:41Z
dc.date.available2021-02-12T08:52:51Z-
dc.date.issued2008
dc.identifier.citationJournal of Astrophysics and Astronomy, v.29/1, pp.281-286, 2008, doi: 10.1007/s12036-008-0037-7en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/433-
dc.description.abstractA fluxgate digital magnetometer is used to study the variation of magnitude of H component during geomagnetic storm events of April, July and November 2004 at southern subauroral localized region at “MAITRI” (geom. lat. 62°S, long. 52.8°E). We also study the effect of vertical component of interplanetary magnetic field (IMF) on the variation of the magnitude of H component during storm time of April, July and November 2004. Results show that before sudden storm commencement (SSC) time magnitude of H component and IMF show smooth variation but after SSC of first storm of 22 July 2004, the magnitude of the H component shows fluctuations and at 09:00 UT it increases, but during second storm of 24 July 2004, the magnitude of H component indicates large fluctuations and it increases rapidly at 04:00 UT.en_US
dc.language.isoenen_US
dc.subjectSudden Storm Commencement (SSC)en_US
dc.subjectMagnitude of the H component deviationen_US
dc.subjectInterplanetary magnetic field (IMF)en_US
dc.subjectGeomagnetic stormen_US
dc.titleEffect of interplanetary magnetic field and disturb storm time on H componenten_US
dc.typeArticleen_US
dc.identifier.accession090932
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