JPL Technical Report Server

Proton Fluence Prediction Models

Show simple item record

dc.contributor.author Feynman, Joan en_US
dc.date.accessioned 2004-09-30T05:14:03Z
dc.date.available 2004-09-30T05:14:03Z
dc.date.issued 1996 en_US
dc.identifier.clearanceno 96-0633 en_US
dc.identifier.uri http://hdl.handle.net/2014/25009
dc.description.abstract Many spacecraft anomalies are caused by positively charged high energy particles impinging on the vehicle and its component parts. Here we review the current knowledge of the interplanetary particle environment in the energy ranges that are most important for these effects, 10 to 100 MeV/amu. The emphasis is on the particle environment at 1 AU. State-of-the-art engineering models are briefly described along with comments on the future work required in this field. en_US
dc.format.extent 1270652 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Proton Fluence Prediction Models spacecraft anomalies high energy particles en_US
dc.title Proton Fluence Prediction Models en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account