Extended or generalized similarity is a ubiquitous but not well understood feature of turbulence that is realized over a finite range of scales. The ULYSSES spacecraft solar polar passes at solar minimum provide in situ observations of evolving anisotropic magnetohydrodynamic turbulence in the solar wind under ideal conditions of fast quiet flow. We find a single generalized scaling function characterizes this finite range turbulence and is insensitive to plasma conditions. The recent unusually inactive solar minimum-with turbulent fluctuations down by a factor of similar to 2 in power-provides a test of this invariance
A major development underlying much of hydrodynamic turbulence theory is the similarity decay hypoth...
International audienceThe solar wind is a highly turbulent and intermittent medium at frequencies be...
Previous theoretical treatments of fluid-scale turbulence in the solar wind have concentrated on des...
We perform statistical analysis of the fluctuating magnetic field observed in-situ by the Ulysses sp...
This review highlights recent examples of generic statistical scaling as departures from ideal Kolmo...
Solar wind fluctuations, such as magnetic field or velocity, show power-law power spectra suggestive...
International audienceIn this paper we review some of the work done in investigating the scaling pro...
Incompressible magnetohydrodynamics is often assumed to describe solar wind turbulence. We use exten...
Using high-speed solar wind data recorded by the Ulysses spacecraft, we investigate and estimate the...
The solar wind provides a natural laboratory for observations of MHD turbulence over extended tempor...
We investigate the intermittency of anisotropic magnetohydrodynamic (MHD) turbulence in high-speed s...
International audienceThe first two orbits of Parker Solar Probe have provided us with the closest e...
International audienceThe anisotropic nature of the scaling properties of solar wind magnetic turbul...
International audienceTurbulent spectrum of magnetic fluctuations in the solar wind nearly follows K...
While the details of the origin of the solar wind in the lower corona remain a puzzle, the supersoni...
A major development underlying much of hydrodynamic turbulence theory is the similarity decay hypoth...
International audienceThe solar wind is a highly turbulent and intermittent medium at frequencies be...
Previous theoretical treatments of fluid-scale turbulence in the solar wind have concentrated on des...
We perform statistical analysis of the fluctuating magnetic field observed in-situ by the Ulysses sp...
This review highlights recent examples of generic statistical scaling as departures from ideal Kolmo...
Solar wind fluctuations, such as magnetic field or velocity, show power-law power spectra suggestive...
International audienceIn this paper we review some of the work done in investigating the scaling pro...
Incompressible magnetohydrodynamics is often assumed to describe solar wind turbulence. We use exten...
Using high-speed solar wind data recorded by the Ulysses spacecraft, we investigate and estimate the...
The solar wind provides a natural laboratory for observations of MHD turbulence over extended tempor...
We investigate the intermittency of anisotropic magnetohydrodynamic (MHD) turbulence in high-speed s...
International audienceThe first two orbits of Parker Solar Probe have provided us with the closest e...
International audienceThe anisotropic nature of the scaling properties of solar wind magnetic turbul...
International audienceTurbulent spectrum of magnetic fluctuations in the solar wind nearly follows K...
While the details of the origin of the solar wind in the lower corona remain a puzzle, the supersoni...
A major development underlying much of hydrodynamic turbulence theory is the similarity decay hypoth...
International audienceThe solar wind is a highly turbulent and intermittent medium at frequencies be...
Previous theoretical treatments of fluid-scale turbulence in the solar wind have concentrated on des...