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Hybrid simulation of foreshock waves and ion spectra and their linkage to cusp energetic ions


Metadata FieldValueLanguage
dc.creatorWang, X.Y.
dc.creatorLin, Y.
dc.creatorChang, S.W.
dc.date.accessioned2022-10-25T14:15:33Z
dc.date.available2022-10-25T14:15:33Z
dc.date.created2009
dc.identifier10.1029/2008JA013745en_US
dc.identifier.urihttps://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2008JA013745en_US
dc.identifier.urihttps://aurora.auburn.edu/handle/11200/50417
dc.identifier.urihttp://dx.doi.org/10.35099/aurora-485
dc.description.abstractA three-dimensional global hybrid simulation is carried out to investigate energetic ions and electromagnetic waves in the quasi-parallel (Q-∥) bow shock and cusp for a typical interplanetary magnetic field configuration during the cusp energetic particle events. The bow shock, magnetosheath, and dayside magnetosphere form by interaction between the solar wind and geomagnetic dipole field. Ions of solar wind characteristics injected into the system evolve along with electromagnetic waves in a self-consistent manner. Several important features are yielded from the simulation. Solar wind ions are accelerated by the waves and turbulence at the bow shock and foreshock as indicated by the ion distribution. The shock-accelerated ions possess an exponential energy spectrum with their differential flux scaled by the field-aligned distance to the bow shock, consistent with satellite observations. Second, the compressive and transversal waves in the foreshock are strongly correlated with the diffuse ion dynamics. Third, energetic ions in the magnetosheath and cusp downstream from the Q-∥ shock also exhibit a spectrum similar to those at the shock. By tracing trajectories of cusp energetic ions in the simulation, the origin of these ions is revealed. Their source is predominantly associated with the Fermi acceleration at the Q-∥ shock and foreshock. Waves in the magnetosheath and cusp, as well as magnetic reconnection at the high-latitude magnetopause, are relatively insignificant in accelerating cusp energetic particles.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 2009. 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: Lin, Y., Lee, L. C., & Yan, M. (1996). Generation of dynamic pressure pulses downstream of the bow shock by variations in the interplanetary magnetic field orientation. Journal of Geophysical Research: Space Physics, 101(A1), 479-493.en_US
dc.titleHybrid simulation of foreshock waves and ion spectra and their linkage to cusp energetic ionsen_US
dc.typeTexten_US
dc.type.genreJournal Article, Academic Journalen_US
dc.citation.volume114en_US
dc.citation.issueA6en_US
dc.citation.spageA06203en_US
dc.description.statusPublisheden_US
dc.description.peerreviewYesen_US

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