JPL Technical Report Server

Early Prediction of Geomagnetic Storms and Space Hazards

Show simple item record

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


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account