A Radiation Belt Content Index Derived from SAMPEX PET Observations During CME and CIR Driven Geomagnetic Storms

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dc.contributor.authorMurphy, Kyle
dc.date.accessioned2020-02-03T21:19:40Z
dc.date.available2020-02-03T21:19:40Z
dc.date.issued2020
dc.description.abstractThis dataset contains the radiation belt content (RBC) index derived from the Solar Anomalous and Magnetospheric Particle Explorer (SAMPEX) Proton Electron Telescope (PET). The RBC is derived from the 1.5-6 MeV electron flux and is used to study the variation of electrons in the outer radiation belt during 64 CME and CIR driven geomagnetic storms.en_US
dc.identifierhttps://doi.org/10.13016/jew4-fjgm
dc.identifier.urihttp://hdl.handle.net/1903/25485
dc.relation.isAvailableAtDigital Repository at the University of Maryland
dc.relation.isAvailableAtUniversity of Maryland (College Park, Md)
dc.relation.isAvailableAtAstronomy
dc.relation.isAvailableAtCollege of Computer, Mathematical & Natural Sciences
dc.subjectGeomagnetic Stormsen_US
dc.subjectRadiation Belten_US
dc.subjectSAMPEXen_US
dc.titleA Radiation Belt Content Index Derived from SAMPEX PET Observations During CME and CIR Driven Geomagnetic Stormsen_US
dc.typeDataseten_US

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IDL save file of the derived radiation belt content index.
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Storm_list.txt
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List of geomagnetic storms for which the radiation belt content is derived.
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