Scaling exponents of the velocity structure functions in the interplanetary medium

We analyze the scaling exponents of the velocity structure functions, obtained from the velocity fluctuations measured in the interplanetary space plasma. Using the expression for the energy transfer rate which seems the most relevant in describing the evolution of the pseudo-energy densities in the...

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Main Author: V. Carbone
Format: Article
Language:English
Published: Copernicus Publications
Series:Annales Geophysicae
Online Access:http://www.ann-geophys.net/12/585/1994/angeo-12-585-1994.html
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author V. Carbone
author_facet V. Carbone
author_sort V. Carbone
collection DOAJ
description We analyze the scaling exponents of the velocity structure functions, obtained from the velocity fluctuations measured in the interplanetary space plasma. Using the expression for the energy transfer rate which seems the most relevant in describing the evolution of the pseudo-energy densities in the interplanetary medium, we introduce an energy cascade model derived from a simple fragmentation process, which takes into account the intermittency effect. In the absence and in the presence of the large-scale magnetic field decorrelation effect the model reduces to the fluid and the hydromagnetic <i>p</i>-model, respectively. We show that the scaling exponents of the <i>q</i>-th power of the velocity structure functions, as obtained by the model in the absence of the decorrelation effect, furnishes the best-fit to the data analyzed from the Voyager 2 velocity field measurements at 8.5 AU. Our results allow us to hypothesize a new kind of scale-similarity for magnetohydrodynamic turbulence when the decorrelation effect is at work, related to the fourth-order velocity structure function.
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spelling doaj.art-0060c76fcbf34f0f9d730f87b19d75412022-12-21T22:39:01ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-0576127585590Scaling exponents of the velocity structure functions in the interplanetary mediumV. CarboneWe analyze the scaling exponents of the velocity structure functions, obtained from the velocity fluctuations measured in the interplanetary space plasma. Using the expression for the energy transfer rate which seems the most relevant in describing the evolution of the pseudo-energy densities in the interplanetary medium, we introduce an energy cascade model derived from a simple fragmentation process, which takes into account the intermittency effect. In the absence and in the presence of the large-scale magnetic field decorrelation effect the model reduces to the fluid and the hydromagnetic <i>p</i>-model, respectively. We show that the scaling exponents of the <i>q</i>-th power of the velocity structure functions, as obtained by the model in the absence of the decorrelation effect, furnishes the best-fit to the data analyzed from the Voyager 2 velocity field measurements at 8.5 AU. Our results allow us to hypothesize a new kind of scale-similarity for magnetohydrodynamic turbulence when the decorrelation effect is at work, related to the fourth-order velocity structure function.http://www.ann-geophys.net/12/585/1994/angeo-12-585-1994.html
spellingShingle V. Carbone
Scaling exponents of the velocity structure functions in the interplanetary medium
Annales Geophysicae
title Scaling exponents of the velocity structure functions in the interplanetary medium
title_full Scaling exponents of the velocity structure functions in the interplanetary medium
title_fullStr Scaling exponents of the velocity structure functions in the interplanetary medium
title_full_unstemmed Scaling exponents of the velocity structure functions in the interplanetary medium
title_short Scaling exponents of the velocity structure functions in the interplanetary medium
title_sort scaling exponents of the velocity structure functions in the interplanetary medium
url http://www.ann-geophys.net/12/585/1994/angeo-12-585-1994.html
work_keys_str_mv AT vcarbone scalingexponentsofthevelocitystructurefunctionsintheinterplanetarymedium