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 …

Rossby modes are the oscillations in a rotating fluid, whose restoring force is the Coriolis
force. They provide an additional diagnostic to understand the rotation of stars, which …

Powerful 'space weather'events caused by solar activity pose serious risks to human health,
safety, economic activity and national security. Spikes in deaths due to heart attacks, strokes …

Rossby waves are a type of global-scale wave that develops in planetary atmospheres,
driven by the planet's rotation. They propagate westward owing to the Coriolis force, and …

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 …

Rossby waves arise in thin layers within fluid regions of stars and planets. These global
wave‐like patterns occur due to the variation in Coriolis forces with latitude. In the past …

The influence of a toroidal magnetic field on the dynamics of shallow water waves in the
solar tachocline is studied. A sub-adiabatic temperature gradient in the upper overshoot …

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 …

Global solar activity variation mainly occurs over about an 11 yr cycle. However, both longer
and shorter periodicities than the solar cycle are also present in many different solar activity …

We present a nonlinear magnetohydrodynamic shallow-water model for the solar tachocline
(MHD-SWT) that generates quasi-periodic tachocline nonlinear oscillations (TNOs) that can …