We demonstrate that the critical magnetic Reynolds number Rm c for a turbulent nonhelical dynamo in the limit of low magnetic Prandtl number Pm (i.e. Pm=Rm/Re ≪ 1) can be significantly reduced if the flow is subjected to global rotation. Even for moderate rotation rates the required energy injection rate can be reduced by a factor of more than 10 3 . This strong decrease in the onset is attributed to the transfer of energy to the large scales, forming a large-scale condensate, and the reduction in the turbulent fluctuations that cause the flow to have a much larger cutoff length scale than in a non-rotating flow of the same Reynolds number. The dynamo thus behaves as if it is driven just by the large scales that act as a laminar flow (i.e....
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...
We demonstrate that the critical magnetic Reynolds number Rm c for a turbulent nonhelical dynamo in...
Planetary and stellar dynamos likely result from turbulent motions in magnetofluids with kinematic v...
Context. Direct numerical simulations of plasmas have shown that the dynamo effect is efficient eve...
This paper is a detailed report on a programme of direct numerical simulations of incompressible non...
This paper is a detailed report on a programme of simulations used to settle a long-standing issue i...
We study numerically the dependence of the critical magnetic Reynolds number Rmc for the turbulent s...
We study numerically the dependence of the critical magnetic Reynolds number Rmc for the turbulent s...
International audienceWhile the saturated magnetic energy is independent of viscosity in dynamo expe...
International audienceWhile the saturated magnetic energy is independent of viscosity in dynamo expe...
doi:10.1088/1367-2630/9/8/300 Abstract. This paper is a detailed report on a programme of direct num...
We study numerically the dependence of the critical magnetic Reynolds number Rmc for the turbulent s...
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...
We demonstrate that the critical magnetic Reynolds number Rm c for a turbulent nonhelical dynamo in...
Planetary and stellar dynamos likely result from turbulent motions in magnetofluids with kinematic v...
Context. Direct numerical simulations of plasmas have shown that the dynamo effect is efficient eve...
This paper is a detailed report on a programme of direct numerical simulations of incompressible non...
This paper is a detailed report on a programme of simulations used to settle a long-standing issue i...
We study numerically the dependence of the critical magnetic Reynolds number Rmc for the turbulent s...
We study numerically the dependence of the critical magnetic Reynolds number Rmc for the turbulent s...
International audienceWhile the saturated magnetic energy is independent of viscosity in dynamo expe...
International audienceWhile the saturated magnetic energy is independent of viscosity in dynamo expe...
doi:10.1088/1367-2630/9/8/300 Abstract. This paper is a detailed report on a programme of direct num...
We study numerically the dependence of the critical magnetic Reynolds number Rmc for the turbulent s...
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...
4 pagesInternational audienceWe present a three-pronged numerical approach to the dynamo problem at ...