collaborators

6 papers

physics.flu-dyn2026

Magnetic Dynamo Driven by Inertial Waves

A. Mishra, G. Mamatsashvili, M. Le Bars +2

We demonstrate, by studying precession-driven flows, that inertial wave hydrodynamic turbulence can drive a robust magnetic dynamo action. Motivated by the stronger damping of larg…

astro-ph.SR2026

Tidal triggers and the predictability of solar activity

F. Stefani, G. M. Horstmann, G. Mamatsashvili +1

Magneto-Rossby waves in the solar tachocline are currently considered to be one of the main determinants of solar activity. In particular, they can give rise to the quasi-biennial…

physics.flu-dyn2025

The effect of split endcaps on the flow dynamics in a tall Taylor-Couette setup

A. Mishra, P. Personnettaz, G. Mamatsashvili +2

The effects of axial boundaries, or endcaps are of fundamental interest in many Taylor-Couette (TC) flow experiments. A main challenge in those experiments has been to minimize the…

physics.flu-dyn2025

Strong and weak dynamo regimes in Taylor-Couette flows

A. Mishra, G. Mamatsashvili, F. Stefani

We reveal a nonlinear magnetic dynamo in a Taylor-Couette flow at small magnetic Prandtl numbers , which has been previously believed to exist only at higher $Pm\gtrsim 1…

astro-ph.SR2025

Reappraising the Elatina series: Solar dynamo clocking and inference of orbital periods

F. Stefani, T. Weier, G. M. Horstmann +1

We reconsider the 680 million year old Elatina series of sedimentary laminae from South Australia that show a remarkably stable periodicity with a main period of around 12 years, w…

astro-ph.SR2025

Adding further pieces to the synchronization puzzle: QBO, bimodality, and phase jumps

F. Stefani, G. M. Horstmann, G. Mamatsashvili +1

This work builds on a recently developed self-consistent synchronization model of the solar dynamo which attempts to explain Rieger-type periods, the Schwabe/Hale cycle and the Sue…