The Sun's axisymmetric large-scale flows, differential rotation and meridional circulation, are
thought to be maintained by the influence of rotation on the thermal-convective motions in …

Rossby waves are a pervasive feature of the large-scale motions of the Earth's atmosphere
and oceans. These waves (also known as planetary waves and r-modes) also play an …

The oscillations of a slowly rotating star have long been classified into spheroidal and
toroidal modes. The spheroidal modes include the well-known 5-min acoustic modes used …

Context. Several types of inertial modes have been detected on the Sun. Properties of these
inertial modes have been studied in the linear regime, but have not been studied in …

Context. Several types of global-scale inertial modes of oscillation have been observed on
the Sun. These include the equatorial Rossby modes, critical-latitude modes, and high …

A major outstanding problem in solar physics is the confinement of the solar tachocline, the
thin shear layer that separates nearly solid-body rotation in the radiative interior from strong …

Context. Inertial modes have been observed on the Sun at low longitudinal wavenumbers.
These modes probe the dynamics and structure of the solar convective zone down to the …

Various types of inertial modes have been observed and identified on the Sun, including the
equatorial Rossby modes, critical-latitude modes, and high-latitude modes. Recent …

Can atmospheric waves in planet-hosting solar-like stars substantially resonate to tidal
forcing, perhaps at a level of impacting the space weather or even being dynamo-relevant …

Inertial waves, which are predominantly driven by the Coriolis force, likely play an important
role in solar dynamics, and, additionally, they provide a window into the solar subsurface …