Ion acceleration by Alfven waves on auroral field lines

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

Observations of ion acceleration along auroral field lines at the boundary of the plasma sheet and tail lobe of the Earth show that the energy of the ions increases with decreasing density. The observations can be explained by ion acceleration through Landau resonance with kinetic Alfvén waves (KAWs) such that k_A.v_i = ω_A, where k_A is the wave vector, v_i is the ion resonance velocity and ω_A is the Alfvén wave frequency. The ion resonance velocities are proportional to the Alfvén velocity which increases with decreasing density. This is in agreement with the data if the process is occurring at the plasma sheet tail lobe boundary. A quasi-linear theory of ion acceleration by KAWs is presented. These ions propagate both down towards and away from the Earth. The paths of the Freja and Polar satellites indicate that the acceleration takes place between the two satellites, between 1Re and 5Re. The downward propagating ions develop a horseshoe-type of distribution which has a positive slope in the perpendicular direction. This type of distribution can produce intense lower hybrid wave activity, which is also observed. Finally, the filamentation of shear Alfvén waves is considered. It may be responsible for large-scale density striations.
LanguageEnglish
Article number058201
Number of pages6
JournalPhysica Scripta
Volume87
Issue number5
DOIs
Publication statusPublished - 2 Apr 2013

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magnetohydrodynamic waves
Line
ions
Tail
Plasma
Kinetics
lobes
Filamentation
Horseshoe
Perpendicular
striation
Slope
kinetics
Directly proportional
Path
slopes
shear
Energy

Keywords

  • plasma
  • alfven waves
  • auroral fieldlines
  • ion acceleration

Cite this

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title = "Ion acceleration by Alfven waves on auroral field lines",
abstract = "Observations of ion acceleration along auroral field lines at the boundary of the plasma sheet and tail lobe of the Earth show that the energy of the ions increases with decreasing density. The observations can be explained by ion acceleration through Landau resonance with kinetic Alfv{\'e}n waves (KAWs) such that k_A.v_i = ω_A, where k_A is the wave vector, v_i is the ion resonance velocity and ω_A is the Alfv{\'e}n wave frequency. The ion resonance velocities are proportional to the Alfv{\'e}n velocity which increases with decreasing density. This is in agreement with the data if the process is occurring at the plasma sheet tail lobe boundary. A quasi-linear theory of ion acceleration by KAWs is presented. These ions propagate both down towards and away from the Earth. The paths of the Freja and Polar satellites indicate that the acceleration takes place between the two satellites, between 1Re and 5Re. The downward propagating ions develop a horseshoe-type of distribution which has a positive slope in the perpendicular direction. This type of distribution can produce intense lower hybrid wave activity, which is also observed. Finally, the filamentation of shear Alfv{\'e}n waves is considered. It may be responsible for large-scale density striations.",
keywords = "plasma, alfven waves, auroral fieldlines, ion acceleration",
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Ion acceleration by Alfven waves on auroral field lines. / Bingham, Robert; Eliasson, Bengt; Mendonca, Jose Tito; Stenflo, Lennart.

In: Physica Scripta, Vol. 87, No. 5, 058201, 02.04.2013.

Research output: Contribution to journalArticle

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AU - Mendonca, Jose Tito

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AB - Observations of ion acceleration along auroral field lines at the boundary of the plasma sheet and tail lobe of the Earth show that the energy of the ions increases with decreasing density. The observations can be explained by ion acceleration through Landau resonance with kinetic Alfvén waves (KAWs) such that k_A.v_i = ω_A, where k_A is the wave vector, v_i is the ion resonance velocity and ω_A is the Alfvén wave frequency. The ion resonance velocities are proportional to the Alfvén velocity which increases with decreasing density. This is in agreement with the data if the process is occurring at the plasma sheet tail lobe boundary. A quasi-linear theory of ion acceleration by KAWs is presented. These ions propagate both down towards and away from the Earth. The paths of the Freja and Polar satellites indicate that the acceleration takes place between the two satellites, between 1Re and 5Re. The downward propagating ions develop a horseshoe-type of distribution which has a positive slope in the perpendicular direction. This type of distribution can produce intense lower hybrid wave activity, which is also observed. Finally, the filamentation of shear Alfvén waves is considered. It may be responsible for large-scale density striations.

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