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Characteristics of high altitude oxygen ion energization and outflow as observed by Cluster: a statistical study
- 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.
- Subjects :
- Atmospheric Science
Materials science
010504 meteorology & atmospheric sciences
Magnetosphere
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
Champ magnetique
Atmospheric sciences
01 natural sciences
TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY
0103 physical sciences
Earth and Planetary Sciences (miscellaneous)
Oxygen ions
Cluster (physics)
lcsh:Science
010303 astronomy & astrophysics
0105 earth and related environmental sciences
[SDU.OCEAN]Sciences of the Universe [physics]/Ocean, Atmosphere
lcsh:QC801-809
Geology
Astronomy and Astrophysics
Effects of high altitude on humans
lcsh:QC1-999
Solar wind
lcsh:Geophysics. Cosmic physics
13. Climate action
Space and Planetary Science
Magnetopause
Outflow
lcsh:Q
lcsh:Physics
Subjects
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