One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …

We observe the emergence of strong vertical drafts in direct numerical simulations of the
Boussinesq equations in a range of parameters of geophysical interest. These structures …

We present a novel machine learning approach to reduce the dimensionality of state
variables in stratified turbulent flows governed by the Navier–Stokes equations in the …

Turbulence in stratified and rotating turbulent flows is characterized by an interplay between
waves and eddies, resulting in continuous exchanges between potential and kinetic energy …

We use multi‐year observations of cross‐track winds (u) from the CHAllenging Minisatellite
Payload (CHAMP) and the Gravity Field and Steady State Ocean Circulation Explorer …

In recent years, multistatic specular meteor radars (SMRs) have been introduced to study the
Mesosphere and Lower Thermosphere (MLT) dynamics with increasing spatial and …

A virtual meteor radar system based on the upper‐atmosphere extension of the high‐
resolution ICOsahedral Non‐hydrostatic general circulation model is constructed to validate …

Nonlinear phenomena and turbulence are central to our understanding and modeling of the
dynamics of fluids and plasmas, and yet they still resist analytical resolution in many …

Turbulent flows in three dimensions are characterized by the transport of energy from large
to small scales through the energy cascade. Since the small scales are the result of the …

In recent years, multistatic specular meteor radars (SMRs) have been introduced to study the
Mesosphere and Lower Thermosphere (MLT) dynamics with increasing spatial and …