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...
| Váldodahkkit: | , , , , , |
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| Materiálatiipa: | Journal article |
| Almmustuhtton: |
2012
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