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Phase coherence of foreshock MHD waves: wavelet analysis

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Abstract

The earth's foreshock is a region where particularly large amplitude MHD waves are commonly observed. They exhibit various waveforms, suggesting that nonlinear interaction between the waves is in progress. In a previous paper (Hada et al., 2003) we have introduced a method to quantitatively evaluate the strength of phase coherence among the waves from a given time series data. Here we further develop our method by applying wavelet filtering technique. From the analysis it was found that, although the turbulence is consisted of waves with a wide range of plasma rest frame frequencies, only those frequencies lower than the ion gyrofrequency are responsible for generating the phase coherence.

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References

  • Hada, T., Koga, D. and Yamamoto, E.: 2003, ‘Phase Coherence of MHD Waves in the Solar Wind’, Space Sci.Rev. this issue.

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Koga, D., Hada, T. Phase coherence of foreshock MHD waves: wavelet analysis. Space Science Reviews 107, 495–498 (2003). https://doi.org/10.1023/A:1025510225311

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  • DOI: https://doi.org/10.1023/A:1025510225311

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