Castaing Scaling and Kernels for Theories of the Turbulent Cascade

Details Castaing Scaling and Kernels for Theories of the Turbulent Cascade Castaing Scaling and Kernels for Theories of the Turbulent Cascade

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..550f&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 550-5

Physics

1

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

The Castaing cascade kernel function G(uL,L') relates the pdf of velocity fluctuations on scale L' to those on scale L. The shape of G(uL,L') and how it depends on scale is a measure of intermittency alternative to measures such as the exponent of the structure function or multifractal spectra. This paper provides analytical forms and graphic illustrations of the Castaing kernels corresponding to six models of the turbulent cascade. The popular P-model and Poisson models of turbulence have discrete Castaing kernels, which seems non-physical.

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