The internal angular momentum distribution of a star is the key to determining its evolution.
Fortunately, stellar internal rotation can be probed through studies of rotationally split …

Our understanding of the dynamics of the Earth's core can be advanced by a combination of
observation, experiments, and simulations. A crucial aspect of the core is the interplay …

Motivated by planetary-driven applications and experiments in non-spherical geometries,
we study compressible fluid modes in rotating rigid ellipsoids. Such modes are also required …

The acoustic spectrum of a gas-filled resonating cavity can be used to indirectly probe its
internal velocity field. This unconventional velocimetry method is particularly interesting for …

The acoustic modes of a rotating fluid-filled cavity can be used to determine the effective
rotation rate of a fluid (since the resonant frequencies are modified by the flows). To be …

Les modes acoustiques sont couramment utilisés pour déterminer les propriétés physiques
de l'intérieur des planètes et des étoiles. La méthode d'imagerie par vélocimétrie acoustique …

Strongly nonlinear fluid flows germane to the planetary cores are possible in laboratory
settings. Both measures of nonlinearity, Reynolds and magnetic Reynolds number, can be …

Many common techniques for flow measurement, such as Particle Image Velocimetry (PIV)
or Ultrasonic Doppler Velocimetry (UDV), rely on the presence of reflectors in the fluid …

We present a new laboratory experiment built to study zonal flows induced by thermal
convection, called ZoRo (Zonal flows in Rotating fluids, TuDy ANR). ZoRo is a rapidly …

Fluid eigenmodes are often used to passively infer physical properties of the interiors of
rotating planets and stars [1]. A similar method has been also introduced in fluid dynamics …