Volume 25 Issue 5
Sep.  2005
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J. Du, C. Wang, X.X. Zhang, N.N. Shevyre, G.N. Zastenker. Magnetic Field Fluctuations in the Solar Wind, Foreshock and Magnetosheath: Cluster Data Analysis[J]. Journal of Space Science, 2005, 25(5): 368-373. doi: 10.11728/cjss2005.05.368
Citation: J. Du, C. Wang, X.X. Zhang, N.N. Shevyre, G.N. Zastenker. Magnetic Field Fluctuations in the Solar Wind, Foreshock and Magnetosheath: Cluster Data Analysis[J]. Journal of Space Science, 2005, 25(5): 368-373. doi: 10.11728/cjss2005.05.368

Magnetic Field Fluctuations in the Solar Wind, Foreshock and Magnetosheath: Cluster Data Analysis

doi: 10.11728/cjss2005.05.368
  • Received Date: 1900-01-01
  • Rev Recd Date: 1900-01-01
  • Publish Date: 2005-09-15
  • 46 magnetosheath crossing events from the two years (2001.2-2003.1) of Cluster magnetic field measurements are identified and used to investigate the characters of the magnetic field fluctuations in the regions of undisturbed solar wind, foreshock, magnetosheath. The preliminary results indicate the properties of the plasma turbulence in the magnetosheath are strongly controlled by IMF orientation with respect to the bow shock normal. The amplitude of the magnetic field magnitude and direction variations behind quasiparallel bow shock are larger than those behind quasi-perpendicular bow shock. Almost purely compressional waves are found in quasi-perpendicular magnetosheath.

     

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