Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456798/351
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dc.contributor.authorLakhina, G.S.-
dc.contributor.authorAlex, S.-
dc.contributor.authorTsurutani, B.T.-
dc.contributor.authorGonzalez, W.D.-
dc.date.accessioned2022-09-12T10:20:01Z-
dc.date.available2022-09-12T10:20:01Z-
dc.date.issued2012-
dc.identifier.citationExtreme Events and Natural Hazards: The Complexity Perspective, Geophysical Monograph Series 196, 10.1029/2011GM001073en_US
dc.identifier.urihttp://library.iigm.res.in:8080/xmlui/handle/123456798/351-
dc.description.abstractMagnetic storms are an important component of space weather effects on Earth. Superintense magnetic storms (defined here as those with Dst < 500 nT, where Dst stands for the disturbance storm time index that measures the strength of the magnetic storm), although relatively rare, can be hazardous to technological systems in space as well as on the ground. Such storms can cause life-threatening power outages, satellite damage, communication failures, and navigational problems. The data for such magnetic storms during the last 50 years is rather scarce. Research on historical geomagnetic storms can help to create a good database for intense and superintense magnetic storms. The superintense storm of 1–2 September 1859 is analyzed in the light of new knowledge of interplanetary and solar causes of storms gained from the space-age observations. We will discuss the results in the context of some recent intense storms and also the occurrence probability of such superstorms.en_US
dc.language.isoenen_US
dc.subjectSupermagnetic stormsen_US
dc.subjectMagnetic stormsen_US
dc.subjectCMEen_US
dc.titleSupermagnetic storms: hazard to societyen_US
dc.typeBook chapteren_US
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