Grand Prix Super D’ Compositor 1 – Le blog du Cancre

Pommois, P., Veltri, P., and Zimbardo, G., Transport of magnetic field lines in the solar wind magnetic turbulence and influence on particle propagation to high heliographic

of NADW that is pumped up from the deep ocean and driven northward by the wind and converted in the surface layer into less dense water by choosing the outcropping latitude and

Models describing the evolution of long internal waves are proposed that are based on different polynomial approximations of the exact expression for the phase speed of

We demonstrated that even in strongly in- homogeneous temperature fields particles in non-isothermal turbulent fluid flow accumulate at the regions with minimum of mean temperature

board the FAST spacecraft when it was located in the night- side magnetosphere at an invariant latitude of 68 ◦. In this figure we see a large number of negative sloped traces in

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

From a modelling point of view, the conclusion is that a uni-modal approach is not well suited for describing the evo- lution (i.e. generation and propagation) of internal

We performed ecosystem level flux measurements of several VOCs, including some halogenated hydrocarbons, using the REA technique, with the aim to quantify the ecosystem level