Modeling of short scale turbulence in the solar wind

This experience covers indeed the modelling of the NWM oceanic circulation at regional scale, several studies of the coastal dynamics of the shelf of the Gulf of Lion, and

In particular, the derived thermal velocity is strongly dominated by perturbations of the magnetic field (and not parallel and/or perpendicular proton temperatures) and therefore

While many of the measured properties are shared with measurements nearer 1 au, signi fi cant differences include increased power levels ( by more than two orders of magnitude

Although those results are original and constitute a real leap forward in studies of solar wind turbulence, ( i ) C09 remains a heuristic model ( i.e., not derived analytically as

The analysis shows that while resonant triad interactions survive the highly nonlinear bath of ion-cyclotron fluctuations at large scales for which the degree of nonlinearity is low

The workshop participants felt that DEMs are not presently able to satisfy the two-pronged criteria—both advanced enough and affordable—required to replace the continuum models

The present article aims primarily at presenting the experiment, the properties of the investigated turbulence (injection and dissipation scales, isotropy, Reynolds number, etc.)

Our first aim is to provide the reader with an elementary proof of a global well-posedness result for small data with critical Sobolev regularity, in the spirit of Fujita-Kato’s