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 2021-05-01 to 2025-05-01.)
ArticleCitations
Can the observable solar activity spectrum be reproduced by a simple dynamo model?15
Introduction8
Rotating convective turbulence in moderate to high Prandtl number fluids8
Formation of small-scale vortices in the core of a large merged vortex8
Rigorous results on conserved and dissipated quantities in ideal MHD turbulence7
Eddy saturation in a reduced two-level model of the atmosphere6
An exact threshold for separator bifurcation5
The inherent instability of axisymmetric magnetostrophic dynamo models5
Weakening the effect of boundaries: “diffusion-free” boundary conditions as a “do least harm” alternative to Neumann5
Angular momentum transfer in direct numerical simulations of a laboratory model of a tropical cyclone5
The Earth's rotational modes revisited5
Magnetoconvection in a rotating spherical shell in the presence of a uniform axial magnetic field4
Astrophysical magnetic fields: from galaxies to the early universe4
On the mother bodies of steady polygonal uniform vortices. Part I: numerical experiments4
Instabilities of low-latitude easterly jets in the presence of moist convection and topography and related cyclogenesis, in a simple atmospheric model4
Self-adjointness of sound-proof models for magnetic buoyancy3
Analysis of mixing structures in the Adriatic Sea using finite-size Lyapunov exponents3
On stratified flow over a topographic ridge in a rotating annulus3
The fastest growing modes in rotating magnetoconvection with anisotropic diffusivities and their links to the Earth's core conditions3
Comments on: nonlinear wind-drift ocean currents in arctic regions3
Geophysical fluid models with simple energy backscatter: explicit flows and unbounded exponential growth3
Generation of azimuthal electromotive forces from azimuthal magnetic fields3
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