Geophysical and Astrophysical Fluid Dynamics

Papers
(The TQCC of Geophysical and Astrophysical Fluid Dynamics is 2. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2022-08-01 to 2026-08-01.)
ArticleCitations
Can the observable solar activity spectrum be reproduced by a simple dynamo model?19
Rotating convective turbulence in moderate to high Prandtl number fluids14
Numerical assessment of advective and diffusive dynamics of interacting and isolated prototypical convectively initiated circulations13
Introduction10
Transmission of three-dimensional anelastic internal gravity wave packets across retrograde jets6
The inherent instability of axisymmetric magnetostrophic dynamo models5
Nonlinear interaction between dynamo-generated magnetic fields, mean flows and internal gravity waves in stellar stably-stratified layers: from 3D to 1D5
A vorticity wavepacket breaking within a rapidly rotating vortex through an off-axis critical layer5
The Earth's rotational modes revisited4
Weakening the effect of boundaries: “diffusion-free” boundary conditions as a “do least harm” alternative to Neumann4
On the mother bodies of steady polygonal uniform vortices. Part I: numerical experiments3
Astrophysical magnetic fields: from galaxies to the early universe3
Magnetoconvection in a rotating spherical shell in the presence of a uniform axial magnetic field3
On stratified flow over a topographic ridge in a rotating annulus3
Ocean neutral transport: sub-Riemannian geometry and hypoelliptic diffusion3
Nonlinear evolution of the global quasi-geostrophic system2
The fastest growing modes in rotating magnetoconvection with anisotropic diffusivities and their links to the Earth's core conditions2
On the Rayleigh–Bénard convection problem for rotating fluids2
Self-adjointness of sound-proof models for magnetic buoyancy2
Spiral wind-up of vortex sheets2
Influence of rotation, stratification, non-hydrostatic and time-dependent mean flow effects on weakly nonlinear gravity waves in shallow-water models: Lagrangian approach2
Spontaneous gravity wave radiation in the Venus atmosphere2
Interaction of a counter-rotating vortex pair with a vortex over bathymetry2
Generation of azimuthal electromotive forces from azimuthal magnetic fields2
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