Alfven vortices: magnetosheath Cluster observations and compressible MHD simulations

Physics – Geophysics

Scientific paper

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2728 Magnetosheath, 2752 Mhd Waves And Instabilities (2149, 6050, 7836), 4400 Nonlinear Geophysics (3200, 6944, 7839), 4490 Turbulence (3379, 4568, 7863)

Scientific paper

Magnetic field fluctuations in the frequency range [0.02-12.5] Hz are studied with the four Cluster satellites in the Earth magnetosheath downstream of a quasi-per\-pen\-di\-cu\-lar bow-shock. The turbulent spectrum presents a spectral break accompanied by a broad maximum usually interpreted as due to Alfvén Ion Cyclotron waves. We establish that this spectral knee corresponds to space-localized coherent magnetic structures in the form of Alfvén vortices. The Alfvén vortex is a non-linear cylindrical Alfvén wave, quasi-parallel to the mean magnetic field B0 and propagating in a plane perpendicular to B_0. The frequent observations of such structures indicate their stability in the plasma. To verify the vortex stability, two-dimensional compressible MHD simulations are performed.

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