dc.contributor.author |
Devi, Rajni |
|
dc.contributor.author |
Dubey, Smita |
|
dc.contributor.author |
Saini, Shailendra |
|
dc.contributor.author |
Devi, Babita |
|
dc.contributor.author |
Dhar, Ajay |
|
dc.contributor.author |
Vijay, S.K. |
|
dc.contributor.author |
Gwal, A.K. |
|
dc.date.accessioned |
2015-09-19T07:20:41Z |
|
dc.date.accessioned |
2021-02-12T08:52:51Z |
|
dc.date.available |
2015-09-19T07:20:41Z |
|
dc.date.available |
2021-02-12T08:52:51Z |
|
dc.date.issued |
2008 |
|
dc.identifier.citation |
Journal of Astrophysics and Astronomy, v.29/1, pp.281-286, 2008, doi: 10.1007/s12036-008-0037-7 |
en_US |
dc.identifier.uri |
http://localhost:8080/xmlui/handle/123456789/433 |
|
dc.description.abstract |
A 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.iso |
en |
en_US |
dc.subject |
Sudden Storm Commencement (SSC) |
en_US |
dc.subject |
Magnitude of the H component deviation |
en_US |
dc.subject |
Interplanetary magnetic field (IMF) |
en_US |
dc.subject |
Geomagnetic storm |
en_US |
dc.title |
Effect of interplanetary magnetic field and disturb storm time on H component |
en_US |
dc.type |
Article |
en_US |
dc.identifier.accession |
090932 |
|