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Observations of multiharmonic ion-cyclotron waves due to inverse ion-cyclotron damping in the northern magnetospheric cusp
Luleå University of Technology, Department of Computer Science, Electrical and Space Engineering, Space Technology.ORCID iD: 0000-0002-2347-1871
Belgian Institute for Space Aeronomy, Avenue Circulaire, Brussels.
Department of Physics, Umeå University.
Number of Authors: 3
2017 (English)In: Geophysical Research Letters, ISSN 0094-8276, E-ISSN 1944-8007, Vol. 44, no 1, 22-29 p.Article in journal (Refereed) Published
Abstract [en]

We present a case study of inverse ion-cyclotron damping taking place in the northern terrestrial magnetospheric cusp, exciting waves at the ion-cyclotron frequency and its harmonics. The ion-cyclotron waves are primarily seen as peaks in the magnetic-field spectral densities. The corresponding peaks in the electric-field spectral densities are not as profound, suggesting a background electric field noise or other processes of wave generation causing the electric spectral densities to smoothen out more compared to the magnetic counterpart. The required condition for inverse ion-cyclotron damping is a velocity shear in the magnetic field-aligned ion-bulk flow, and this condition is often naturally met for magnetosheath influx in the northern magnetospheric cusp, just as in the presented case. We note that some ion-cyclotron wave activity is present in a few similar shear events in the southern cusp, which indicates that other mechanisms generating ion-cyclotron waves may also be present during such conditions.

Place, publisher, year, edition, pages
2017. Vol. 44, no 1, 22-29 p.
National Category
Aerospace Engineering
Research subject
Atmospheric science
Identifiers
URN: urn:nbn:se:ltu:diva-61214DOI: 10.1002/2016GL071680ISI: 000393954900003Scopus ID: 2-s2.0-85010604932OAI: oai:DiVA.org:ltu-61214DiVA: diva2:1058998
Note

Validerad; 2017; Nivå 2; 2017-02-10 (andbra)

Available from: 2016-12-22 Created: 2016-12-22 Last updated: 2017-10-19Bibliographically approved

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