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The Comprehensive Inner Magnetosphere-Ionosphere Model


Metadata FieldValueLanguage
dc.creatorFok, M
dc.creatorBuzulukova, N
dc.creatorChen, S
dc.creatorGlocer, A
dc.creatorNagai, T
dc.creatorValek, P
dc.creatorPerez, J
dc.date.accessioned2023-01-31T20:40:13Z
dc.date.available2023-01-31T20:40:13Z
dc.date.created2014
dc.identifier10.1002/2014JA020239en_US
dc.identifier.urihttps://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2014JA020239en_US
dc.identifier.urihttps://aurora.auburn.edu/handle/11200/50502
dc.identifier.urihttp://dx.doi.org/10.35099/aurora-570
dc.description.abstractSimulation studies of the Earth's radiation belts and ring current are very useful in understanding the acceleration, transport, and loss of energetic particles. Recently, the Comprehensive Ring Current Model (CRCM) and the Radiation Belt Environment (RBE) model were merged to form a Comprehensive Inner Magnetosphere-Ionosphere (CIMI) model. CIMI solves for many essential quantities in the inner magnetosphere, including ion and electron distributions in the ring current and radiation belts, plasmaspheric density, Region 2 currents, convection potential, and precipitation in the ionosphere. It incorporates whistler mode chorus and hiss wave diffusion of energetic electrons in energy, pitch angle, and cross terms. CIMI thus represents a comprehensive model that considers the effects of the ring current and plasmasphere on the radiation belts. We have performed a CIMI simulation for the storm on 5-9 April 2010 and then compared our results with data from the Two Wide-angle Imaging Neutral-atom Spectrometers and Akebono satellites. We identify the dominant energization and loss processes for the ring current and radiation belts. We find that the interactions with the whistler mode chorus waves are the main cause of the flux increase of MeV electrons during the recovery phase of this particular storm. When a self-consistent electric field from the CRCM is used, the enhancement of MeV electrons is higher than when an empirical convection model is applied. We also demonstrate how CIMI can be a powerful tool for analyzing and interpreting data from the new Van Allen Probes mission.en_US
dc.formatPDFen_US
dc.publisherAmerican Geophysical Unionen_US
dc.relation.ispartofJOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICSen_US
dc.relation.ispartofseries2169-9380en_US
dc.rights©American Geophysical Union 2014. This is this the version of record co-published by the American Geophysical Union and John Wiley & Sons, Inc. It is made available under the CC-BY-NC-ND 4.0 license. Item should be cited as: Fok, M. C., Buzulukova, N. Y., Chen, S. H., Glocer, A., Nagai, T., Valek, P., & Perez, J. D. (2014). The comprehensive inner magnetosphere‐ionosphere model. Journal of Geophysical Research: Space Physics, 119(9), 7522-7540.en_US
dc.titleThe Comprehensive Inner Magnetosphere-Ionosphere Modelen_US
dc.typeTexten_US
dc.type.genreJournal Article, Academic Journalen_US
dc.citation.volume119en_US
dc.citation.issue9en_US
dc.description.statusPublisheden_US
dc.description.peerreviewYesen_US
dc.creator.orcid0000-0001-9500-866Xen_US
dc.creator.orcid0000-0001-9843-9094en_US
dc.creator.orcid0000-0002-2318-8750en_US

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