Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95508/1/jgra21877.pd
We discuss properties of large amplitude magnetic field fluctuationsduring fast Alfv ́eenic solar wi...
The solar wind is the Sun's exosphere. As the solar atmosphere expands into interplanetary space, it...
International audienceWe discuss properties of large amplitude magnetic field fluctuations during fa...
This paper analyzes solar wind power spectra of bulk and thermal speed fluctuations that are compute...
The in situ measurements of velocity, magnetic field, density and temperature fluctuations performed...
MHD turbulence is studied by analyzing magnetic field and plasma observations from Helios-1 and -2 a...
International audienceIn this work, we investigate magnetic field fluctuations in three coronal mass...
International audienceIn this work, we investigate magnetic field fluctuations in three coronal mass...
International audienceIn this work, we investigate magnetic field fluctuations in three coronal mass...
A phenomenological theory describes radial evolution of plasma turbulence in the solar wind from 1 t...
The power spectrum of the evolving solar wind shows evidence of a spectral break between an inertial...
A phenomenological theory describes radial evolution of plasma turbulence in the solar wind from 1 t...
This Letter investigates the spectral characteristics of interplanetary magnetic field fluctuations ...
International audienceIn this work, we investigate magnetic field fluctuations in three coronal mass...
International audienceIn this work, we investigate magnetic field fluctuations in three coronal mass...
We discuss properties of large amplitude magnetic field fluctuationsduring fast Alfv ́eenic solar wi...
The solar wind is the Sun's exosphere. As the solar atmosphere expands into interplanetary space, it...
International audienceWe discuss properties of large amplitude magnetic field fluctuations during fa...
This paper analyzes solar wind power spectra of bulk and thermal speed fluctuations that are compute...
The in situ measurements of velocity, magnetic field, density and temperature fluctuations performed...
MHD turbulence is studied by analyzing magnetic field and plasma observations from Helios-1 and -2 a...
International audienceIn this work, we investigate magnetic field fluctuations in three coronal mass...
International audienceIn this work, we investigate magnetic field fluctuations in three coronal mass...
International audienceIn this work, we investigate magnetic field fluctuations in three coronal mass...
A phenomenological theory describes radial evolution of plasma turbulence in the solar wind from 1 t...
The power spectrum of the evolving solar wind shows evidence of a spectral break between an inertial...
A phenomenological theory describes radial evolution of plasma turbulence in the solar wind from 1 t...
This Letter investigates the spectral characteristics of interplanetary magnetic field fluctuations ...
International audienceIn this work, we investigate magnetic field fluctuations in three coronal mass...
International audienceIn this work, we investigate magnetic field fluctuations in three coronal mass...
We discuss properties of large amplitude magnetic field fluctuationsduring fast Alfv ́eenic solar wi...
The solar wind is the Sun's exosphere. As the solar atmosphere expands into interplanetary space, it...
International audienceWe discuss properties of large amplitude magnetic field fluctuations during fa...
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