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dc.contributor.authorLakhina, G.S.
dc.contributor.authorAlex, S.
dc.contributor.authorMukherjee, S.
dc.contributor.authorVichare, Geeta
dc.date.accessioned2015-09-07T10:37:11Z
dc.date.accessioned2021-02-12T09:27:57Z-
dc.date.available2015-09-07T10:37:11Z
dc.date.available2021-02-12T09:27:57Z-
dc.date.issued2006
dc.identifier.citationILWS Workshop 2006, GOA, 2006en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/342-
dc.description.abstractMagnetospheric substorms and storms are indicators of geomagnetic activity. Whereas the geomagnetic index AE (auroral electrojet) is used to study substorms, it is common to characterize the magnetic storms by the Dst (disturbance storm time) index of geomagnetic activity. This talk discusses briefly the storm substorms relationship, and highlights some of the characteristics of intense magnetic storms, including the events of 29-31 October and 20-21 November 2003. The adverse effects of these intense geomagnetic storms on telecommunication, navigation, and on spacecraft functioning will be discussed.en_US
dc.language.isoenen_US
dc.subjectGeomagnetic activityen_US
dc.subjectGeomagnetic stormsen_US
dc.subjectSpace weatheren_US
dc.subjectSubstormsen_US
dc.titleOn magnetic storms and substormsen_US
dc.typeArticleen_US
dc.identifier.accession090835
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