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dc.contributor.authorSugiyama, Hajime
dc.contributor.authorSingh, S.V.
dc.contributor.authorOmura, Yoshiharu
dc.contributor.authorShoj, Masafumi
dc.contributor.authorNunn, David
dc.contributor.authorSummers, Danny
dc.date.accessioned2017-10-26T05:49:52Z
dc.date.accessioned2021-02-12T09:46:29Z-
dc.date.available2017-10-26T05:49:52Z
dc.date.available2021-02-12T09:46:29Z-
dc.date.issued2015
dc.identifier.citationJGR, 120, p. 8426–8439, doi: 10.1002/2015JA021346en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/992-
dc.description.abstractA theoretical model to study electromagnetic ion cyclotron (EMIC) waves in kappa-Maxwellian plasma is developed. The plasma is assumed to have five components, i.e., electrons, cool and hot protons, and singly charged helium and oxygen ions. The kappa-Maxwellian anisotropic particle distribution function is assumed for the hot protons. We use the Kyoto University Plasma Dispersion Analysis Package, a full dispersion solver developed at Kyoto University, to obtain the numerical results and delineate the oxygen, helium, and proton bands. Higher harmonics of the EMIC waves are also studied, and the effects of the kappa distribution on the growth of these waves are clearly demonstrated. Our results are applied to Cluster spacecraft observations of EMIC waves in the inner magnetosphere.en_US
dc.language.isoenen_US
dc.subjectCyclotron wavesen_US
dc.subjectElectromagnetic ion cyclotronen_US
dc.subjectKappa-Maxwellian particleen_US
dc.subjectEMIC wave instabilitiesen_US
dc.subjectMagnetosphereen_US
dc.titleElectromagnetic ion cyclotron waves in the Earth’s magnetosphere with a kappa-Maxwellian particle distributionen_US
dc.typeArticleen_US
dc.identifier.accession091534
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