ULF Waves in the Terrestrial Magnetosphere: First CLUSTER FGM Results

Details ULF Waves in the Terrestrial Magnetosphere: First CLUSTER FGM Results ULF Waves in the Terrestrial Magnetosphere: First CLUSTER FGM Results

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsm22a0831f&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SM22A-0831

Physics

2731 Magnetosphere: Outer, 2752 Mhd Waves And Instabilities, 2772 Plasma Waves And Instabilities

Scientific paper

ULF waves are one of the prominent dynamical features of the terrestrial magnetosphere. Generated by external and internal plasma instabilities as well as wave activity in the solar wind and magnetosheath they represent an attractive object of scientific analysis using CLUSTER magnetic field observations. Having available four closely spaced spacecraft enables us to study in detail their spatial and temporal characteristics in an as yet unprecedented accuracy. We shall present examples of ULF waves resembling field line resonances and surface waves as well as propagating and standing wave structures. Emphasize is especially paid on propagation properties and spatial extent of the wave fields.

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