OOIR: Observatory of International Research

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 2021-04-01 to 2025-04-01.)

Article	Citations
A study of global magnetic helicity in self-consistent spherical dynamos	14
Stability of upper-tropospheric flows and the chaotic oscillation regime	8
Multiple jets in a rotating annulus model with an imposed azimuthal magnetic field	7
The time evolution of the mother body of a planar uniform vortex moving in an inviscid fluid	7
Rotating convective turbulence in moderate to high Prandtl number fluids	6
Solitary wave scattering by segmented arc-shaped breakwater	5
Magnetoconvection in a rotating spherical shell in the presence of a uniform axial magnetic field	5
Instabilities of low-latitude easterly jets in the presence of moist convection and topography and related cyclogenesis, in a simple atmospheric model	5
Astrophysical magnetic fields: from galaxies to the early universe	5
Can the observable solar activity spectrum be reproduced by a simple dynamo model?	5
Zonostrophic instabilities in magnetohydrodynamic Kolmogorov flow	5
Dynamics of the coherent structure for incompressible fluid flow in turbulent boundary layers	4
Formation of small-scale vortices in the core of a large merged vortex	4
Introduction	4
On the mother bodies of steady polygonal uniform vortices. Part I: numerical experiments	3
Multiplicity in an optimised kinematic dynamo	3
Axial flow in an eroding Euler hairpin in ℝ ³ : does it prevent blow-up?	3
On the role of helicity inversions in reversals and excursions of the geodynamo	3
Smoothed particle hydrodynamics approach for modelling submerged granular flows and the induced water wave generation	3
Hydrodynamicα-effect in a rotating stratified moist atmosphere driven by small-scale non-helical force	3
Eddy saturation in a reduced two-level model of the atmosphere	3