The Temporal Evolution Of 3 - 9 Mev/nucleon He Flux Trapped In The Magnetosphere

dc.creatorPugacheva G.I.
dc.creatorGusev A.A.
dc.creatorMartin I.M.
dc.creatorSpjeldvik W.N.
dc.creatorKohno T.
dc.date1996
dc.date2015-06-26T17:02:20Z
dc.date2015-11-26T14:18:07Z
dc.date2015-06-26T17:02:20Z
dc.date2015-11-26T14:18:07Z
dc.date.accessioned2018-03-28T21:19:20Z
dc.date.available2018-03-28T21:19:20Z
dc.identifier
dc.identifierGeophysical Research Letters. , v. 23, n. 20, p. 2793 - 2796, 1996.
dc.identifier948276
dc.identifier
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-0030269387&partnerID=40&md5=38dec211e0c55cadb665a67c790e9c0e
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/95396
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/95396
dc.identifier2-s2.0-0030269387
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1243543
dc.descriptionInstitute of Physical and Chemical Research (RIKEN), Saitama, Japan Results of measurements of the absolute values and long term temporal evolution of the spatial distribution of trapped He ion fluxes of 3.2 - 9.2 MeV/nucleon energy at L < 4 obtained by the OHZORA satellite are reported. The annually averaged radial profile exhibits one persistently present peak at L = 1.3 - 1.5 as well as very significant transient trapped fluxes at L = 1.4 - 4.0 during the period 1984-1986. Together the absolute values of the fluxes measured by OHZORA and S72-1, SAMPEX, and CRRES spacecrafts may approximately be described by a power spectrum with index of -8.0±1.0 at L = 1.9-2.3 within the energy range of 3 - 100 MeV/nucleon. Copyright 1996 by the American Geophysical Union.
dc.description23
dc.description20
dc.description2793
dc.description2796
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dc.languageen
dc.publisher
dc.relationGeophysical Research Letters
dc.rightsaberto
dc.sourceScopus
dc.titleThe Temporal Evolution Of 3 - 9 Mev/nucleon He Flux Trapped In The Magnetosphere
dc.typeArtículos de revistas


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