Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/432
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dc.contributor.authorDevi, Babita
dc.contributor.authorDubey, Smita
dc.contributor.authorSaini, Shailendra
dc.contributor.authorDevi, Rajni
dc.contributor.authorWahi, Rashmi
dc.contributor.authorDhar, Ajay
dc.contributor.authorVijay, S.K.
dc.contributor.authorGwal, A.K.
dc.date.accessioned2015-09-19T07:11:53Z
dc.date.accessioned2021-02-12T08:52:51Z-
dc.date.available2015-09-19T07:11:53Z
dc.date.available2021-02-12T08:52:51Z-
dc.date.issued2008
dc.identifier.citationJournal of Astrophysics and Astronomy, v.29, p.275-280, 2008, doi: 10.1007/s12036-008-0036-8en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/432-
dc.description.abstractThis paper presents the effect of geomagnetic storm on geomagnetic field components at Southern (Maitri) and Northern (Kiruna) Hemispheres. The Indian Antarctic Station Maitri is located at geom. long. 66.03° S; 53.21° E whereas Kiruna is located at geom. long. 67.52° N; 23.38° E. We have studied all the geomagnetic storms that occurred during winter season of the year 2004–2005. We observed that at Southern Hemisphere the variation is large as compared to the Northern Hemisphere. Geomagnetic field components vary when the interplanetary magnetic field is oriented in southward direction. Geomagnetic field components vary in the main phase of the ring current. Due to southward orientation of vertical component of IMF reconnection takes place all across the dayside that transports plasma and magnetic flux which create the geomagnetic field variation.en_US
dc.language.isoenen_US
dc.subjectGeomagnetic fielden_US
dc.subjectMagnetic fielden_US
dc.subjectHigh latitudeen_US
dc.subjectGeomagnetic stormen_US
dc.subjectDst fielden_US
dc.titleGeomagnetic field variation during winter storm at localized southern and northern high latitudeen_US
dc.typeArticleen_US
dc.identifier.accession090931
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