The Warm Plasma Composition in the Inner Magnetosphere during 2012–2015

Jahn, J. M.; Goldstein, J.; Reeves, Geoffrey D.; Fernandes, Philip A.; Skoug, Ruth M.; Larsen, Brian Arthur; Spence, H. E.

doi:10.1002/2017JA024183

Title: The Warm Plasma Composition in the Inner Magnetosphere during 2012–2015

Journal Article · 11 September 2017 · Journal of Geophysical Research. Space Physics

DOI: https://doi.org/10.1002/2017JA024183 · OSTI ID:1394981

Jahn, J. M. ^[1]; Goldstein, J. ^[1];

^[2];

^[2]; Skoug, Ruth M. ^[2];

^[2]; Spence, H. E. ^[3]

Southwest Research Inst., San Antonio, TX (United States)
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Univ. of New Hampshire, Durham, NH (United States)

Ionospheric heavy ions play an important role in the dynamics of Earth's magnetosphere. The greater mass and gyro radius of ionospheric oxygen differentiates its behavior from protons at the same energies. Oxygen may have an impact on tail reconnection processes, and it can at least temporarily dominate the energy content of the ring current during geomagnetic storms. At sub-keV energies, multi-species ion populations in the inner magnetosphere form the warm plasma cloak, occupying the energy range between the plasmasphere and the ring current. Lastly, cold lighter ions from the mid-latitude ionosphere create the co-rotating plasmasphere whose outer regions can interact with the plasma cloak, plasma sheet, ring current, and outer electron belt. Here in this paper we present a statistical view of warm, cloak-like ion populations in the inner magnetosphere, contrasting in particular the warm plasma composition during quiet and active times. We study the relative abundances and absolute densities of warm plasma measured by the Van Allen Probes, whose two spacecraft cover the inner magnetosphere from plasmaspheric altitudes close to Earth to just inside geostationary orbit. We observe that warm (>30 eV) oxygen is most abundant closer to the plasmasphere boundary whereas warm hydrogen dominates closer to geostationary orbit. Warm helium is usually a minor constituent, but shows a noticeable enhancement in the near-Earth dusk sector.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: National Aeronautics and Space Administration (NASA); USDOE National Nuclear Security Administration (NNSA)

Grant/Contract Number:: AC52-06NA25396; NAS5-01072

OSTI ID:: 1394981

Report Number(s):: LA-UR-17-24831

Journal Information:: Journal of Geophysical Research. Space Physics, Vol. 122, Issue 11; ISSN 2169-9380

Publisher:: American Geophysical UnionCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 21 works

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