Probability distributions of the induced electric field of the solar wind

Details Probability distributions of the induced electric field of the solar wind Probability distributions of the induced electric field of the solar wind

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003jgra..108.1153b&link_type=abstract

Journal of Geophysical Research (Space Physics), Volume 108, Issue A4, pp. SSH 3-1, CiteID 1153, DOI 10.1029/2002JA009529

Physics

6

Interplanetary Physics: Solar Wind Plasma, Interplanetary Physics: Mhd Waves And Turbulence, Magnetospheric Physics: Mhd Waves And Instabilities, Magnetospheric Physics: Electric Fields (2411)

Scientific paper

The low-frequency induced electric field in the near-Earth interplanetary medium is investigated observationally. These electric field fluctuations are associated with magnetohydrodynamic-scale fluctuations of the magnetic field and plasma velocity. Results of the study, based upon hourly samples with variations computed relative to 4-day means, indicate that the electric field distribution is roughly exponential. More specifically, the electric field distribution is very nearly the one that is obtained from a quasi-normal turbulence model [Milano et al., 2002]. These results may be useful for particle scattering, acceleration, and turbulence.

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