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dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-08-20T11:25:14Z
dc.date.accessioned2021-02-12T10:30:53Z-
dc.date.available2015-08-20T11:25:14Z
dc.date.available2021-02-12T10:30:53Z-
dc.date.issued2001
dc.identifier.citationJournal of Atmospheric and Solar-Terrestrial Physics, v.63, p.481-487, 2001, doi: 10.1016/S1364-6826(00)00160-7en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/254-
dc.description.abstractThe presence of an ionospheric-origin anisotropic oxygen ion beam can excite a helicon mode instability in the near-Earth plasma sheet region. The helicon modes can be easily excited under the conditions when the usual long wavelength fire-hose modes are stable. The helicon modes are likely to attain saturation as the typical e-folding time of the instability is about a few minutes in the near-Earth plasma sheet region. Therefore, the instability could significantly affect substorm dynamics and lead to enhanced ionosphere–magnetosphere coupling. Low-frequency turbulence produced by these modes could scatter electrons trapped in the inner central plasma sheer region and help excite the ion tearing modes, leading to substorm onset. As a result, the oxygen ions would be injected into the Earth's nightside magnetosphere. Repeated injections by this process would lead to enhanced oxygen ion fluxes in the storm-time ring current.en_US
dc.language.isoenen_US
dc.subjectHelicon modesen_US
dc.subjectOxygenen_US
dc.subjectRing currenten_US
dc.subjectIonosphere–magnetosphere couplingen_US
dc.subjectMagnetosphereen_US
dc.subjectNear-Earth plasma sheet regionen_US
dc.titleRole of helicon modes in the injection of oxygen ions in the ring currenten_US
dc.typeArticleen_US
dc.identifier.accession090741
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