Spectral signatures of jumps and turbulence in interplanetary speed and magnetic field data

Physics

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Interplanetary Magnetic Fields, Plasma Turbulence, Solar Wind Velocity, Spectral Signatures, Fourier Analysis, Random Walk, Time Series Analysis

Scientific paper

It is shown here that, consistent with a suggestion of Burlaga and Mish (1987), the f exp -2 spectra in the magnitudes of the magnetic and velocity fields in the solar wind result from jumps due to various rapid changes in the time series for these quantities. If these jumps are removed from the data, the spectra of the resulting 'difference' time series have the f exp -5/3 form. It is concluded that f exp -2 spectra in these magnitudes arise from phase coherent structures that can be distinguished clearly from incoherent turbulent fluctuations.

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