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Early Prediction of Geomagnetic Storms and Space Hazards

Show simple item record Collins, D. en_US Feynman, J. en_US 2004-09-23T17:48:54Z 2004-09-23T17:48:54Z 2000-03 en_US
dc.identifier.citation Chapman Conference on Space Weather en_US
dc.identifier.citation Clearwater, FL, USA en_US
dc.identifier.clearanceno 00-0517 en_US
dc.description.abstract Solar coronal mass ejections (CMEs) can cause hazadous high-energy particles and geomagnetic storms that, in the more serious instances, can disrupt Earth power grids, communications, and satellites. en_US
dc.format.extent 519794 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other space weather space physics solar physics microspacecraft geomagnetic storm en_US
dc.title Early Prediction of Geomagnetic Storms and Space Hazards en_US

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