Turbulent Electric Field and Magnetic Field in the Tail: THEMIS High-Resolution Observations

Details Turbulent Electric Field and Magnetic Field in the Tail: THEMIS High-Resolution Observations Turbulent Electric Field and Magnetic Field in the Tail: THEMIS High-Resolution Observations

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsm53a..04t&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SM53A-04

Physics

[2712] Magnetospheric Physics / Electric Fields, [2744] Magnetospheric Physics / Magnetotail

Scientific paper

Turbulent electric field and magnetic field are examined with THEMIS high-resolution observations in the magnetotail. The distribution of de-trended Poynting flux shows a clear asymmetric feature with earthward flux prevailing in the range from ~8 Re to ~15 Re, and an approximately symmetric feature beyond 15 Re. The power spectra of E and B are computed in the frequency range 0.008-3 kHz, which is extended beyond the MHD range compared with the ion gyrofrequency (> 0.1 Hz). In general, the spectra of B fields show similar features with previous studies while the spectra of E fields show features completely different from B fields.

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