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

• Main Authors: Devi, Babita, Dubey, Smita, Saini, Shailendra, Devi, Rajni, Wahi, Rashmi, Dhar, Ajay, Vijay, S.K., Gwal, A.K.
• Format: Article in Journal/Newspaper
• Language: English
• Published: 2008
• Subjects: Geomagnetic field; Magnetic field; High latitude; Geomagnetic storm; Dst field; Antarctic; Indian; Kiruna; Maitri; Antarc*
• Online Access: http://14.139.123.141:8080/jspui/handle/123456789/432

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.