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Oxygen ion energization observed at high altitudes
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Swedish Institute of Space Physics, Uppsala Division.
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2010 (English)In: Annales Geophysicae, ISSN 0992-7689, E-ISSN 1432-0576, Vol. 28, no 4, 907-916 p.Article in journal (Refereed) Published
Abstract [en]

We present a case study of significant heating (up to 8 keV) perpendicular to the geomagnetic field of outflowing oxygen ions at high altitude (12 R-E) above the polar cap. The shape of the distribution functions indicates that most of the heating occurs locally (within 0.2-0.4 R-E in altitude). This is a clear example of local ion energization at much higher altitude than usually reported. In contrast to many events at lower altitudes, it is not likely that the locally observed wave fields can cause the observed ion energization. Also, it is not likely that the ions have drifted from some nearby energization region to the point of observation. This suggests that additional fundamentally different ion energization mechanisms are present at high altitudes. One possibility is that the magnetic moment of the ions is not conserved, resulting in slower outflow velocities and longer time for ion energization.

Place, publisher, year, edition, pages
2010. Vol. 28, no 4, 907-916 p.
Keyword [en]
Magnetospheric physics, Magnetosphere-ionosphere interactions
National Category
Physical Sciences
URN: urn:nbn:se:uu:diva-147426DOI: 10.5194/angeo-28-907-2010ISI: 000277243500003OAI: oai:DiVA.org:uu-147426DiVA: diva2:400448
Available from: 2011-02-25 Created: 2011-02-25 Last updated: 2011-02-25Bibliographically approved

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