Stirring of water by mesoscale currents (“eddies”) leads to large-scale transport many important oceanic properties (“tracers”). These eddy-induced transports can be related the tracer gradients, using concept turbulent diffusion. The is widely used describe these in real ocean and represent them climate models. This study focuses on inherent complexity corresponding coefficient tensor (“K-tens...

Abstract

Compensation of the poleward eddy heat transport by the heat transport of an eddy-induced mean meridional overturning cell is a common feature in many eddyresolving ocean models. It has been ,argued that this is the result of the weak thermal driving of the ocean. As the actual air/sea coupling is scale dependent, it might be questioned whether the approximation of weak thermal driving is relev...

In this paper thermal conductivity and thermal diffusivity of a two layer system is examined from the theoretical point of view. We use the one dimensional heat diffusion equation with the appropriate solution in each layer and boundary conditions at the interfaces to calculate the heat transport in this bounded system. We also consider the heat flux at the surface of the samle as boundary cond...

The quasi-geostrophic global stratospheric model at MIT developed by is used to study the zonal and time-averaged transport of potential temperature and ozone by the planetary zonal wavenumbers 1-6. Several types of covariances between the winds, geopotential, and the tracers are calculated in order to evaluate the directions and strength of the fluxes and the winds causing the fluxes. The eddy...

This paper considers a linear one dimensional inverse heat conduction problem with non constant thermal diffusivity and two unknown terms in a heated bar with unit length. By using the WKB method, the heat flux at the end of boundary and initial temperature will be approximated, numerically. By choosing a suitable parameter in WKB method the ill-posedness of solution will be improved. Finally, ...

Convection of an electrically conducting fluid in a rotating system represents a basic dynamical process in planetary interiors and in stars. Astrophysicists and geophysicists have long been interested in the mechanisms that govern the convective heat transport and the generation of magnetic fields by convection in those systems. The availability in recent years of large scale computer capaciti...