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A low altitude trapped proton model for solar minimum conditions based on SAMPEX/PET data

dc.contributor.authorHeynderickx, D.
dc.contributor.authorKruglanski, M.
dc.contributor.authorPierrard, V.
dc.contributor.authorLemaire, J.
dc.contributor.authorLooper, M.D.
dc.contributor.authorBlake, J.B.
dc.date1999
dc.date.accessioned2017-05-09T11:58:42Z
dc.date.available2017-05-09T11:58:42Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5365
dc.descriptionWe present a low altitude (below about 600 km) trapped proton model for solar minimum conditions (1994-1995), based on measurements made by the Proton/Electron Telescope onboard the SAMPEX satellite. Substantial differences are found with the low altitude part of the AP-8 MIN model: !ow energy fluxes appear to be overestimated by AP-8 MIN, while the new model predicts higher fluxes than AP-8 MIN for energies above about 30MeV.
dc.languageeng
dc.titleA low altitude trapped proton model for solar minimum conditions based on SAMPEX/PET data
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeProton electron telescope
dc.subject.freeTrapped proton
dc.subject.freeElectrons
dc.subject.freeGeomagnetism
dc.subject.freeMathematical models
dc.subject.freeProtons
dc.subject.freeRadiation damage
dc.subject.freeSatellites
dc.subject.freeTelescopes
dc.subject.freeRadiation belts
dc.source.titleIEEE Transactions on Nuclear Science
dc.source.volume46
dc.source.issue6
dc.source.page1475-1480
Orfeo.peerreviewedYes
dc.identifier.doi10.1109/23.819110
dc.identifier.scopus2-s2.0-0033314068


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