Turbulence in Solar Wind Plasma (IMAGE)

Max-Planck-Institut für Plasmaphysik (IPP)

Turbulence in Solar Wind Plasma

Caption

Turbulence in solar wind plasma. The simulation - an example for the results of the successful Max-Planck-Princeton partnership -- shows the magnetic field fluctuations due to turbulence. Their spatial and temporal structures can be compared with space probe measurements.

Credit

Graphic: IPP, Daniel Told

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