This review highlights recent examples of generic statistical scaling as departures from ideal Kolmogorov fluid turbulence as seen in the solar wind. Similarity analysis is first reviewed to set turbulence in the context of the wider class of observed phenomenology that show statistical scaling. Examples are provided that are characteristic of finite range MHD turbulent phenomenology-anisotropy, and generalized similarity as a finite range effect. This motivates the question as to whether the observed phenomonology are universal
Incompressible magnetohydrodynamics is often assumed to describe solar wind turbulence. We use exten...
Graduation date: 1994The statistics describing variations of turbulent motions within the so called\...
We apply the finite size scaling technique to quantify the statistical properties of fluctuations in...
Extended or generalized similarity is a ubiquitous but not well understood feature of turbulence tha...
We apply the finite size scaling technique to quantify the statistical properties of fluctuations in...
The solar wind provides a natural laboratory for observations of MHD turbulence over extended tempor...
We apply the finite size scaling technique to quantify the statistical properties of fluctuations in...
International audienceIn this paper we review some of the work done in investigating the scaling pro...
We perform statistical analysis of the fluctuating magnetic field observed in-situ by the Ulysses sp...
International audienceThis paper gives a review of some recent work on intermittency, non-Gaussian s...
[1] Statistical properties of the interplanetary magnetic field fluctuations can provide an importan...
The solar wind provides a natural laboratory for observations of magnetohydrodynamic (MHD) turbulenc...
Solar wind fluctuations, such as magnetic field or velocity, show power-law power spectra suggestive...
The solar wind plasma is a natural laboratory for studies of plasma turbulence. Long, evenly sampled...
Statistical properties of the interplanetary magnetic field fluctuations can provide an important in...
Incompressible magnetohydrodynamics is often assumed to describe solar wind turbulence. We use exten...
Graduation date: 1994The statistics describing variations of turbulent motions within the so called\...
We apply the finite size scaling technique to quantify the statistical properties of fluctuations in...
Extended or generalized similarity is a ubiquitous but not well understood feature of turbulence tha...
We apply the finite size scaling technique to quantify the statistical properties of fluctuations in...
The solar wind provides a natural laboratory for observations of MHD turbulence over extended tempor...
We apply the finite size scaling technique to quantify the statistical properties of fluctuations in...
International audienceIn this paper we review some of the work done in investigating the scaling pro...
We perform statistical analysis of the fluctuating magnetic field observed in-situ by the Ulysses sp...
International audienceThis paper gives a review of some recent work on intermittency, non-Gaussian s...
[1] Statistical properties of the interplanetary magnetic field fluctuations can provide an importan...
The solar wind provides a natural laboratory for observations of magnetohydrodynamic (MHD) turbulenc...
Solar wind fluctuations, such as magnetic field or velocity, show power-law power spectra suggestive...
The solar wind plasma is a natural laboratory for studies of plasma turbulence. Long, evenly sampled...
Statistical properties of the interplanetary magnetic field fluctuations can provide an important in...
Incompressible magnetohydrodynamics is often assumed to describe solar wind turbulence. We use exten...
Graduation date: 1994The statistics describing variations of turbulent motions within the so called\...
We apply the finite size scaling technique to quantify the statistical properties of fluctuations in...