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Ion acceleration by Alfven waves on auroral field lines
Rutherford Appleton Lab, England .
Ruhr University of Bochum, Germany .
Institute Super Tecn, Portugal .
Linköping University, Department of Physics, Chemistry and Biology, Theoretical Physics. Linköping University, The Institute of Technology.
2013 (English)In: Physica Scripta, ISSN 0031-8949, E-ISSN 1402-4896, Vol. 87, no 5Article in journal (Refereed) Published
Abstract [en]

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 Alfven waves (KAWs) such that k(A) . v(i) = omega(A), where k(A) is the wave vector, v(i) is the ion resonance velocity and omega(A) is the Alfven wave frequency. The ion resonance velocities are proportional to the Alfven 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 Alfven waves is considered. It may be responsible for large-scale density striations.

Place, publisher, year, edition, pages
Institute of Physics , 2013. Vol. 87, no 5
National Category
Engineering and Technology
URN: urn:nbn:se:liu:diva-93389DOI: 10.1088/0031-8949/87/05/058201ISI: 000318274400032OAI: diva2:624496
Available from: 2013-05-31 Created: 2013-05-31 Last updated: 2013-05-31

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Stenflo, Lennart
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