Comparison of the Magnetic Turbulence in the Solar Wind and in the Earth's Plasma Sheet - Case Studies

Details Comparison of the Magnetic Turbulence in the Solar Wind and in the Earth's Plasma Sheet - Case Studies Comparison of the Magnetic Turbulence in the Solar Wind and in the Earth's Plasma Sheet - Case Studies

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...3e..64d&link_type=abstract

Solar Active Regions and 3D Magnetic Structure, 26th meeting of the IAU, Joint Discussion 3, 16-17 August, 2006, Prague, Czech R

Statistics

Scientific paper

Recently it was demonstrated that turbulence in the solar wind and the intermittent properties of magnetic fluctuations in the Earth's plasma sheet can be studied using the statistical approach (Dorotovič and Vörös, 2004). Comparison of higher order moments (skewness and kurtosis) for selected events from the years 1996-2002 (Dorotovič and Vörös, 2005), however, provided no straightforward clues how the turbulence statistics in the solar wind and in the Earth's plasma sheet can be physically interconnected. In this paper we investigate cases when peculiarities of specific conditions in both regions can be considered and their influence on turbulence statistics can be recognized.

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