A statistical study of wave Poynting vectors measured during long-period magnetospheric pulsations at geostationary orbit

Physics

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Electric Fields, Geomagnetism, Geosynchronous Orbits, Magnetospheric Instability, Poynting Theorem, Statistical Analysis, Geos 2 Satellite, Magnetohydrodynamic Waves

Scientific paper

From electric and magnetic field data measured at geostationary orbit, 3580 wave Poynting vectors for long-period magnetospheric pulsations were computed. Typical vector magnitudes were in the range 10 to the -9th to -7th W/sq m. During the winter season, the field-aligned component of the majority of the vectors was directed to the Northern Hemisphere, where the ionospheric conductivity was lower than in the opposite hemisphere. For most Poynting vector events, the E/b(E) ratio was well above the local Alfven speed, and generally increased with increasing wave frequency of the pulsations. Most long-period wave Poynting vectors had an inward component and pointed toward the nose of the magnetosphere. These results are in good agreement with the interpretation of the vector events as fundamental mode eigenoscillations of geomagnetic field lines which are caused by solar wind driven surface waves on the outer boundaries of the magnetosphere.

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