On magnetic storms and substorms

dc.contributor.author	Lakhina, G.S.
dc.contributor.author	Alex, S.
dc.contributor.author	Mukherjee, S.
dc.contributor.author	Vichare, Geeta
dc.date.accessioned	2015-09-07T10:37:11Z
dc.date.accessioned	2021-02-12T09:27:57Z
dc.date.available	2015-09-07T10:37:11Z
dc.date.available	2021-02-12T09:27:57Z
dc.date.issued	2006
dc.identifier.citation	ILWS Workshop 2006, GOA, 2006	en_US
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/342
dc.description.abstract	Magnetospheric 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.iso	en	en_US
dc.subject	Geomagnetic activity	en_US
dc.subject	Geomagnetic storms	en_US
dc.subject	Space weather	en_US
dc.subject	Substorms	en_US
dc.title	On magnetic storms and substorms	en_US
dc.type	Article	en_US
dc.identifier.accession	090835