Structure function measurements of the intermittent MHD turbulent cascade

The intertmittent nature of turbulence within solar wind plasma has been demonstrated by several studies of spacecraft data. Using magnetic field data taken in high speed flows at high heliographic latitudes by the Ulysses probe, the character of fluctuations within the inertia] range is discussed....

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Main Authors: T. S. Horbury, A. Balogh
Format: Article
Language:English
Published: Copernicus Publications 1997-01-01
Series:Nonlinear Processes in Geophysics
Online Access:http://www.nonlin-processes-geophys.net/4/185/1997/npg-4-185-1997.pdf
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author T. S. Horbury
A. Balogh
author_facet T. S. Horbury
A. Balogh
author_sort T. S. Horbury
collection DOAJ
description The intertmittent nature of turbulence within solar wind plasma has been demonstrated by several studies of spacecraft data. Using magnetic field data taken in high speed flows at high heliographic latitudes by the Ulysses probe, the character of fluctuations within the inertia] range is discussed. Structure functions are used extensively. A simple consideration of errors associated with calculations of high moment structure functions is shown to be useful as a practical estimate of the reliability of such calculations. For data sets of around 300 000 points, structure functions of moments above 5 are rarely reliable on the basis of this test, highlighting the importance of considering uncertainties in such calculations. When unreliable results are excluded, it is shown that inertial range polar fluctuations are well described by a multifractal model of turbulent energy transfer. Detailed consideration of the scaling of high order structure functions suggests energy transfer consistent with a "Kolmogorov" cascade.
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spelling doaj.art-d52363f6d19b4eb2a950b65592809e412022-12-22T02:36:09ZengCopernicus PublicationsNonlinear Processes in Geophysics1023-58091607-79461997-01-0143185199Structure function measurements of the intermittent MHD turbulent cascadeT. S. HorburyA. BaloghThe intertmittent nature of turbulence within solar wind plasma has been demonstrated by several studies of spacecraft data. Using magnetic field data taken in high speed flows at high heliographic latitudes by the Ulysses probe, the character of fluctuations within the inertia] range is discussed. Structure functions are used extensively. A simple consideration of errors associated with calculations of high moment structure functions is shown to be useful as a practical estimate of the reliability of such calculations. For data sets of around 300 000 points, structure functions of moments above 5 are rarely reliable on the basis of this test, highlighting the importance of considering uncertainties in such calculations. When unreliable results are excluded, it is shown that inertial range polar fluctuations are well described by a multifractal model of turbulent energy transfer. Detailed consideration of the scaling of high order structure functions suggests energy transfer consistent with a "Kolmogorov" cascade.http://www.nonlin-processes-geophys.net/4/185/1997/npg-4-185-1997.pdf
spellingShingle T. S. Horbury
A. Balogh
Structure function measurements of the intermittent MHD turbulent cascade
Nonlinear Processes in Geophysics
title Structure function measurements of the intermittent MHD turbulent cascade
title_full Structure function measurements of the intermittent MHD turbulent cascade
title_fullStr Structure function measurements of the intermittent MHD turbulent cascade
title_full_unstemmed Structure function measurements of the intermittent MHD turbulent cascade
title_short Structure function measurements of the intermittent MHD turbulent cascade
title_sort structure function measurements of the intermittent mhd turbulent cascade
url http://www.nonlin-processes-geophys.net/4/185/1997/npg-4-185-1997.pdf
work_keys_str_mv AT tshorbury structurefunctionmeasurementsoftheintermittentmhdturbulentcascade
AT abalogh structurefunctionmeasurementsoftheintermittentmhdturbulentcascade