Geomagnetic field variation during winter storm at localized southern and northern high latitude

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dc.contributor.author Devi, Babita
dc.contributor.author Dubey, Smita
dc.contributor.author Saini, Shailendra
dc.contributor.author Devi, Rajni
dc.contributor.author Wahi, Rashmi
dc.contributor.author Dhar, Ajay
dc.contributor.author Vijay, S.K.
dc.contributor.author Gwal, A.K.
dc.date.accessioned 2015-09-19T07:11:53Z
dc.date.accessioned 2021-02-12T08:52:51Z
dc.date.available 2015-09-19T07:11:53Z
dc.date.available 2021-02-12T08:52:51Z
dc.date.issued 2008
dc.identifier.citation Journal of Astrophysics and Astronomy, v.29, p.275-280, 2008, doi: 10.1007/s12036-008-0036-8 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/432
dc.description.abstract This 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.iso en en_US
dc.subject Geomagnetic field en_US
dc.subject Magnetic field en_US
dc.subject High latitude en_US
dc.subject Geomagnetic storm en_US
dc.subject Dst field en_US
dc.title Geomagnetic field variation during winter storm at localized southern and northern high latitude en_US
dc.type Article en_US
dc.identifier.accession 090931


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