Michael von Papen

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Questions related from Michael von Papen

What controls The Ion Dissipation Range in observations of Solar Wind Turbulence?

I just read an interesting paper by Smith et al. (2012, ApJ), where they describe four characteristic regions in the power spectra of turbulent magnetic field fluctuations: 1. f < 0.5 Hz: Ion...

24 May 2013 8,506 3 View

From frequency to k-space

If a satellite measures magnetic fluctuations, e.g. in the solar wind, taylors frozen in theorem is usually well satisfied (wave speed

07 March 2013 5,838 3 View