Geophysical and Astrophysical Fluid Dynamics

Papers
(The TQCC of Geophysical and Astrophysical Fluid Dynamics is 3. 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 2021-11-01 to 2025-11-01.)
ArticleCitations
Formation of small-scale vortices in the core of a large merged vortex20
Can the observable solar activity spectrum be reproduced by a simple dynamo model?12
Rotating convective turbulence in moderate to high Prandtl number fluids11
Eddy saturation in a reduced two-level model of the atmosphere8
Rigorous results on conserved and dissipated quantities in ideal MHD turbulence8
A vorticity wavepacket breaking within a rapidly rotating vortex through an off-axis critical layer8
Introduction8
The Earth's rotational modes revisited7
Angular momentum transfer in direct numerical simulations of a laboratory model of a tropical cyclone7
The inherent instability of axisymmetric magnetostrophic dynamo models7
An exact threshold for separator bifurcation6
Weakening the effect of boundaries: “diffusion-free” boundary conditions as a “do least harm” alternative to Neumann5
Astrophysical magnetic fields: from galaxies to the early universe5
Magnetoconvection in a rotating spherical shell in the presence of a uniform axial magnetic field4
On the mother bodies of steady polygonal uniform vortices. Part I: numerical experiments3
Self-adjointness of sound-proof models for magnetic buoyancy3
Generation of azimuthal electromotive forces from azimuthal magnetic fields3
Influence of rotation, stratification, non-hydrostatic and time-dependent mean flow effects on weakly nonlinear gravity waves in shallow-water models: Lagrangian approach3
On stratified flow over a topographic ridge in a rotating annulus3
Comments on: nonlinear wind-drift ocean currents in arctic regions3
Spiral wind-up of vortex sheets3
Geophysical fluid models with simple energy backscatter: explicit flows and unbounded exponential growth3
The fastest growing modes in rotating magnetoconvection with anisotropic diffusivities and their links to the Earth's core conditions3
Solitary wave scattering by segmented arc-shaped breakwater3
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