3 papers
astro-ph.SR2026
Solar differential rotation driven by baroclinic forcing
L. S. Menicucci, G. Guerrero, M. Dikpati +3
A combination of recent observations and numerical simulations has called into question whether Sun's interior is characterized by strong turbulent convection, a problem known as c…
astro-ph.SR2025
Simulations of the onset and dynamical evolution of inertial waves in solar/stellar interior
Mariane D. Souza-Gomes, Conrado S. Finotti, Gustavo Guerrero +4
Inertial modes have been recently detected in the Sun via helioseismology, yet their origin, evolution, and role in the dynamics of the solar plasma and magnetic field remain poorl…
astro-ph.SR2023
Dynamics of the tachocline
Antoine Strugarek, Bernadett Belucz, Allan Sacha Brun +2
The solar tachocline is an internal region of the Sun possessing strong radial and latitudinal shears straddling the base of the convective envelope. Based on helioseismic inversio…