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Characteristics of high altitude oxygen ion energization and outflow as observed by Cluster: a statistical study

Authors :
H. Nilsson
M. Waara
S. Arvelius
O. Marghitu
M. Bouhram
Y. Hobara
M. Yamauchi
R. Lundin
H. Rème
J.-A. Sauvaud
I. Dandouras
A. Balogh
L. M. Kistler
B. Klecker
C. W. Carlson
M. B. Bavassano-Cattaneo
A. Korth
Swedish Institute of Space Physics [Kiruna] (IRF)
Max-Planck-Institut für Extraterrestrische Physik (MPE)
Institute of Space Science [Bucharest-Măgurele] (ISS)
Centre d'étude spatiale des rayonnements (CESR)
Observatoire Midi-Pyrénées (OMP)
Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3)
Université Fédérale Toulouse Midi-Pyrénées
Imperial College of Science
University of New Hampshire (UNH)
Space Sciences Laboratory [Berkeley] (SSL)
University of California [Berkeley]
University of California-University of California
Istituto di Fisica dello Spazio Interplanetario (IFSI)
Consiglio Nazionale delle Ricerche (CNR)
Max-Planck-Institut für Sonnensystemforschung (MPS)
Max-Planck-Gesellschaft
Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
University of California [Berkeley] (UC Berkeley)
University of California (UC)-University of California (UC)
National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR)
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS)
Source :
Annales Geophysicae, Annales Geophysicae, European Geosciences Union, 2006, 24 (3), pp.1099-1112, Scopus-Elsevier, Annales Geophysicae, 2006, 24 (3), pp.1099-1112, Annales Geophysicae, Vol 24, Pp 1099-1112 (2006), Annales Geophysicae, Vol 24, Iss 3, Pp 1099-1112 (2006)
Publication Year :
2018

Abstract

The results of a statistical study of oxygen ion outflow using Cluster data obtained at high altitude above the polar cap is reported. Moment data for both hydrogen ions (H+) and oxygen ions (O+) from 3 years (2001-2003) of spring orbits (January to May) have been used. The altitudes covered were mainly in the range 5–12 RE geocentric distance. It was found that O+ is significantly transversely energized at high altitudes, indicated both by high perpendicular temperatures for low magnetic field values as well as by a tendency towards higher perpendicular than parallel temperature distributions for the highest observed temperatures. The O+ parallel bulk velocity increases with altitude in particular for the lowest observed altitude intervals. O+ parallel bulk velocities in excess of 60 km s-1 were found mainly at higher altitudes corresponding to magnetic field strengths of less than 100 nT. For the highest observed parallel bulk velocities of O+ the thermal velocity exceeds the bulk velocity, indicating that the beam-like character of the distribution is lost. The parallel bulk velocity of the H+ and O+ was found to typically be close to the same throughout the observation interval when the H+ bulk velocity was calculated for all pitch-angles. When the H+ bulk velocity was calculated for upward moving particles only the H+ parallel bulk velocity was typically higher than that of O+. The parallel bulk velocity is close to the same for a wide range of relative abundance of the two ion species, including when the O+ ions dominates. The thermal velocity of O+ was always well below that of H+. Thus perpendicular energization that is more effective for O+ takes place, but this is not enough to explain the close to similar parallel velocities. Further parallel acceleration must occur. The results presented constrain the models of perpendicular heating and parallel acceleration. In particular centrifugal acceleration of the outflowing ions, which may provide the same parallel velocity increase to the two ion species and a two-stream interaction are discussed in the context of the measurements.

Details

Language :
English
ISSN :
14320576 and 09927689
Database :
OpenAIRE
Journal :
Annales Geophysicae, Annales Geophysicae, European Geosciences Union, 2006, 24 (3), pp.1099-1112, Scopus-Elsevier, Annales Geophysicae, 2006, 24 (3), pp.1099-1112, Annales Geophysicae, Vol 24, Pp 1099-1112 (2006), Annales Geophysicae, Vol 24, Iss 3, Pp 1099-1112 (2006)
Accession number :
edsair.doi.dedup.....dd973bedb221041cd515a877129dd3d1