Early Prediction of Geomagnetic Storms and Space Hazards

Collins, D.; Feynman,  J.

dc.contributor.author	Collins, D.	en_US
dc.contributor.author	Feynman, J.	en_US
dc.date.accessioned	2004-09-23T17:48:54Z
dc.date.available	2004-09-23T17:48:54Z
dc.date.issued	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.identifier.uri	http://hdl.handle.net/2014/14115
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