Influence of Ekman friction on the velocity profile of a coherent vortex in a three-dimensional rotating turbulent flow

VM Parfenyev, SS Vergeles - Physics of Fluids, 2021 - pubs.aip.org
In the presence of strong background rotation, the velocity field tends to become quasi-two-
dimensional, which leads to the inverse energy cascade. If the damping is small enough …

Signature and energetics of internal gravity waves in stratified turbulence

A Maffioli, A Delache, FS Godeferd - Physical Review Fluids, 2020 - APS
Internal gravity waves propagating within homogeneous stratified turbulence are the subject
of the present study. A spatiotemporal analysis is carried out on the results of direct …

effect in three-dimensional vortex of conducting rotating liquid

LL Ogorodnikov, SS Vergeles - Physical Review E, 2024 - APS
We study one-point statistics of helical turbulent pulsations in the background of a three-
dimensional large-scale vortex in a rotating fluid. Assuming that the helical flow is created by …

The spatial segregation of kinetic helicity in geodynamo simulations

A Ranjan, P Davidson - Geophysical Monograph Series, 2024 - Wiley Online Library
Kinetic helicity and its spatial distribution are thought to be important for the maintenance of
a dipolar magnetic field in the geodynamo through the α-effect. Outside the inner core …

The role of slow magnetostrophic waves in the formation of the axial dipole in planetary dynamos

A Varma, B Sreenivasan - Physics of the Earth and Planetary Interiors, 2022 - Elsevier
The preference for the axial dipole in planetary dynamos is investigated through the analysis
of wave motions in spherical dynamo models. Our study focuses on the role of slow …

On the spatial segregation of helicity by inertial waves in dynamo simulations and planetary cores

PA Davidson, A Ranjan - Journal of Fluid Mechanics, 2018 - cambridge.org
The distribution of kinetic helicity in a dipolar planetary dynamo is central to the success of
that dynamo. Motivated by the helicity distributions observed in numerical simulations of the …

Evolution of forced magnetohydrodynamic waves in a stratified fluid

B Sreenivasan, G Maurya - Journal of Fluid Mechanics, 2021 - cambridge.org
The evolution of a buoyancy disturbance in a stratified incompressible fluid permeated by a
uniform vertical magnetic field is investigated. Two regimes are considered in the absence of …

On the generation and segregation of helicity in geodynamo simulations

A Ranjan, PA Davidson… - Geophysical Journal …, 2020 - academic.oup.com
Helicity, the inner product of velocity and vorticity, is considered an important ingredient for
the maintenance of a dipolar magnetic field in the geodynamo. Outside the tangent cylinder …

The connection between the equatorial temperature bias and north–south helicity segregation in numerical simulations of the geodynamo

PA Davidson, A Ranjan - Geophysical Journal International, 2023 - academic.oup.com
In recent numerical simulations of the geodynamo the dynamo action is driven, primarily, by
the effects of helicity, with differential rotation playing only a secondary role. These dynamos …

Are planetary dynamos driven by helical waves?

PA Davidson, A Ranjan - Journal of Plasma Physics, 2018 - cambridge.org
Are planetary dynamos driven by helical waves? Page 1 J. Plasma Phys. (2018), vol. 84,
735840304 c Cambridge University Press 2018 doi:10.1017/S0022377818000466 1 REVIEW …