Three-Dimensional Structure of Solar Wind Turbulence
We present a measurement of the scale-dependent, three-dimensional structure of the magnetic field fluctuations in inertial range solar wind turbulence with respect to a local, physically motivated coordinate system. The Alfvenic fluctuations are three-dimensionally anisotropic, with the sense of th...
Hlavní autoři: | Chen, C, Mallet, A, Schekochihin, A, Horbury, T, Wicks, RT, Bale, S |
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Médium: | Journal article |
Vydáno: |
2012
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