Add to ORKGWe study the diffusion of helium and other heavy elements in the solar interior by solving exactly t...
Calculation of diffusion and drift velocities in nightime F region, and measurements of ion density ...
International audienceIn this paper we establish links between turbulence dissipation and wave-parti...
The effects of the reduction in the thermal conductivity due to heavy ions on electron temperatures ...
The induced scattering of ion-acoustic waves on ions is considered for preferential preacceleration ...
A comparison of polar solar wind proton flux upper limits derived using a coronal density model, wit...
International audienceThis paper concisely summarizes and critically reviews recent work by the auth...
During the final year of this program we concentrated on understanding the how to constrain the mode...
Magnetic and electric field aligned plasma diffusion in the ionosphere to examine conditions for amb...
A simple model of the lower corona which allows for a possible difference in the electron and proton...
Continuum plasma dynamics, and properties of corona, solar wind, magnetosphere, and transition regio
The outflow of ions at high latitudes is one mechanism thought to populate the magnetosphere with io...
A semiempirical, axisymmetric model of the solar minimum corona is developed by solving the equation...
Aims. Our aim is to investigate and study the de-charging of the elements C, N, O, Mg, Si and S-ions...
International audienceThe solar wind, although predominantly constituted of protons, is also made up...
We study the diffusion of helium and other heavy elements in the solar interior by solving exactly t...
Calculation of diffusion and drift velocities in nightime F region, and measurements of ion density ...
International audienceIn this paper we establish links between turbulence dissipation and wave-parti...
The effects of the reduction in the thermal conductivity due to heavy ions on electron temperatures ...
The induced scattering of ion-acoustic waves on ions is considered for preferential preacceleration ...
A comparison of polar solar wind proton flux upper limits derived using a coronal density model, wit...
International audienceThis paper concisely summarizes and critically reviews recent work by the auth...
During the final year of this program we concentrated on understanding the how to constrain the mode...
Magnetic and electric field aligned plasma diffusion in the ionosphere to examine conditions for amb...
A simple model of the lower corona which allows for a possible difference in the electron and proton...
Continuum plasma dynamics, and properties of corona, solar wind, magnetosphere, and transition regio
The outflow of ions at high latitudes is one mechanism thought to populate the magnetosphere with io...
A semiempirical, axisymmetric model of the solar minimum corona is developed by solving the equation...
Aims. Our aim is to investigate and study the de-charging of the elements C, N, O, Mg, Si and S-ions...
International audienceThe solar wind, although predominantly constituted of protons, is also made up...
We study the diffusion of helium and other heavy elements in the solar interior by solving exactly t...
Calculation of diffusion and drift velocities in nightime F region, and measurements of ion density ...
International audienceIn this paper we establish links between turbulence dissipation and wave-parti...