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Geophysical & Astrophysical Fluid Dynamics is a peer-reviewed journal published by Taylor & Francis, covering Solar and Space Plasma Dynamics, Geomagnetism and Paleomagnetism Studies, Oceanographic and Atmospheric Processes.
| Publisher | Taylor & Francis |
|---|---|
| Reference style | Author–year (Chicago, T&F) Author–year — (Smith, 2023) in the text Smith, Ada, Ben Jones, and Cara Lee. 2023. "A Representative Article Title." Geophysical & Astrophysical Fluid Dynamics 12 (3): 45–58.
Formats any DOI in Geophysical & Astrophysical Fluid Dynamics style. No sign-up. |
| Publishes research in | Solar and Space Plasma Dynamics Geomagnetism and Paleomagnetism Studies Oceanographic and Atmospheric Processes Fluid Dynamics and Turbulent Flows Geophysics and Gravity Measurements |
| ISSN | 0309-1929 |
| Citation impact (2-yr) | 0.73 |
| h-index | 81 |
| i10-index | 859 |
| Total citations | 36,546 |
| Top institutions publishing here | Newcastle University |
| Journal website | www.tandfonline.com |
| You get | A submission-ready PDF and the editable LaTeX source — ready to submit. |
Citations each year’s papers have accumulated so far — the most recent years are still building up.
Abstract Convection in Earth's fluid core is regarded as a small deviation from a well-mixed adiabatic state of uniform chemical composition. The core is modeled as a binary alloy of iron and some lighter constituent, whose precise chemical composition is unknown but which is here assumed to be FeAd, where Ad = Si, O or…
Abstract The annual mean depth-integrated steric height P and stream function ψ of the world ocean are calculated from a Sverdrup model with Hellerman and Rosenstein's (1983) annual mean wifids. The parameterization of friction is unspecified, but friction is assumed to be important only along western boundaries. A simple rule, based on Sverdrup interior flow…
Abstract The Cauchy-Schwarz inequality is employed to find geometry-independent limits on the magnetic helicity dissipation rate in a resistive plasma. These limits only depend upon the total energy of the plasma, the energy dissipation rate, and a mean diffusion coefficient. For plasmas isolated from external energy sources, limits can also be set on the minimum…
Abstract I examine the geostrophic turbulence field in equilibrium with a horizontally uniform mean zonal flow driven by solar heating. The equilibrium mean vertical shear is highly supercritical, and the turbulence field has its maximum in kinetic energy at wavenumbers smaller than the wavenumbers of fastest growth predicted by linear stability theory. Wavenumber spectra obtained…
Abstract We calculate the trajectories of particles in two-dimensional model flows typifying atmospheric or oceanic eddy motions. Rather than restricting the flows to be weak (but solutions to the relevant dynamics), we have considered motions where the streamfunction is only a kinematic model resembling the actual flows but the amplitude can be large so that…
