Physics – Plasma Physics
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsm51c1843p&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #SM51C-1843
Physics
Plasma Physics
[2730] Magnetospheric Physics / Magnetosphere: Inner, [7863] Space Plasma Physics / Turbulence
Scientific paper
Turbulent fluctuations of the geomagnetic field have been studied using the data of the THEMIS satellite mission and and ground magnetometer data from auroral and sub-auroral station including of the SAMBA magnetometer chain, located in Chile and in the Antarctic peninsula. It was found that turbulent spectra obtained at the same geomagnetic field line on the ground level in both hemispheres and near the equatorial plane are generally similar. Using the Local Intermittency Measure technique it was also established that the observed turbulence has an intermittent behavior. The MLT and longitudinal dependence were found to be stronger near midnight inside the auroral zone, which corresponds to the satellite location at 12-18 Earth radii to the tail.
Antonova Elizabeth E.
Pinto V. A.
Stepanova M. V.
Valdivia Juan A.
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