Time-dependent Dispersive Whistlers Close to the Magnetopause

Details Time-dependent Dispersive Whistlers Close to the Magnetopause Time-dependent Dispersive Whistlers Close to the Magnetopause

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsm51b0366s&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SM51B-0366

Physics

7835 Magnetic Reconnection, 7867 Wave/Particle Interactions, 2724 Magnetopause, Cusp, And Boundary Layers, 2772 Plasma Waves And Instabilities

Scientific paper

Whistler waves inside the magnetopause are found to be generated in thin sheets moving with the plasma drift velocity. In the same region we also observe time-dependent dispersive whistler emissions. The duration of each emission is about 1 second and the frequency ranges from 50 to 150 Hz. Using electric and magnetic wave field observations from the four Cluster satellites we estimate the wave length, the direction of propagation and the size and location of the generation region. We also discuss possible generation mechanisms and their relation to the magnetopause.

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