Magnetic field generation by convective flows in a plane layer: the dependence on the Prandtl numbers

作者：Podvigina O M^*

来源：Geophysical and Astrophysical Fluid Dynamics, 2008, 102(4): 409-433.

DOI：10.1080/03091920701841945

• thermal convection
• bifurcations
• attractors
• magnetic field generation

Investigation of magnetic field generation by convective flows is carried out for three values of kinematic Prandtl number: P = 0.3, 1 and 6.8. We consider Rayleigh-Benard convection in Boussinesq approximation assuming stress-free boundary conditions on horizontal boundaries and periodicity with the same period in the x and y directions. Convective attractors are modelled for increasing Rayleigh numbers for each value of the kinematic Prandtl number. Linear and non-linear dynamo action of these attractors is studied for magnetic Prandtl numbers P(m) <= 100. Flows, which can act as magnetic dynamos, have been found for all the three considered values of P, if the Rayleigh number R is large enough. The minimal R, for which of magnetic field generation occurs, increases with P. The minimum (over R) of critical Pm for magnetic field generation in the kinematic regime is admitted for P = 0.3. Thus, our study indicates that smaller values of P are beneficial for magnetic field generation.

• 出版日期2008