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• W2092374623 abstract "We investigate a class of axisymmetric magnetohydrodynamic turbulence which satisfies the exact relation for third-order Elsässer structure functions. Following the critical balance conjecture, we assume the existence of a power-law relation between correlation length scales along and transverse to the local mean magnetic field direction. The flow direction of the vector third-order moments F± is then along axisymmetric concave/convex surfaces, the axis of symmetry being given by the mean magnetic field. Under this consideration, the vector F± satisfies a simple Kolmogorov law which depends on the anisotropic parameter a±, which measures the concavity of the surfaces. A comparison with recent in situ multispacecraft solar wind observations is made; it is concluded that the underlying turbulence is very likely convex. A discussion is given about the physical meaning of such an anisotropy." @default.
• W2092374623 created "2016-06-24" @default.
• W2092374623 creator A5044640403 @default.
• W2092374623 date "2012-02-06" @default.
• W2092374623 modified "2023-09-27" @default.
• W2092374623 title "KOLMOGOROV VECTORIAL LAW FOR SOLAR WIND TURBULENCE" @default.
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• W2092374623 doi "https://doi.org/10.1088/0004-637x/746/2/184" @default.
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