The effect of a uniform straining motion u = (α1x1, α2x2, α3x3), where α1 + α2 + α3 = 0, and α1 > α2 > α3, on what may be called a "blob" of weak magnetic field, that is a magnetic field which is exponentially small outside a certain bounded region, has recently been examined by Pao.(1
We discuss the applicability of the kinematic α-effect formalism at high magnetic Reynolds numbers. ...
In this study, we analysed a three-dimensional Taylor decaying vortex under an applied magnetic fiel...
It is conjectured that transport by parallel mass flow in a braided magnetic field, rather than hype...
Evolution of stochastically homogeneous magnetic field advected by incompressible turbulent flow wit...
Kinematic dynamo in incompressible isotropic turbulent flows with high magnetic Prandtl number is co...
Context. Direct numerical simulations of plasmas have shown that the dynamo effect is efficient eve...
In a recent publication, viz. [Phys. Lett. A 326 (2004) 267], Jovanovic and Shukla (J. and S. in the...
Funding Information: We acknowledge fruitful discussions with A. Brandenburg, I. Rogachevskii, A. Sc...
Small-scale dynamos play important roles in modern astrophysics, especially on Galactic and extragal...
This paper is a detailed report on a programme of simulations used to settle a long-standing issue i...
In a recent paper Nakagawa and Nishida [1989] have suggested that wavy motions of the neutral sheet ...
We investigate the effect of the surface bipolar magnetic regions (BMR) on the large-scale dynamo di...
We analyze the initial, kinematic stage of magnetic field evolution in an isotropic and homogeneous ...
We consider fluctuations of magnetic field excited by external force and advected by isotropic turbu...
We present numerical simulations of driven magnetohydrodynamic (MHD) turbulence with weak/moderate i...
We discuss the applicability of the kinematic α-effect formalism at high magnetic Reynolds numbers. ...
In this study, we analysed a three-dimensional Taylor decaying vortex under an applied magnetic fiel...
It is conjectured that transport by parallel mass flow in a braided magnetic field, rather than hype...
Evolution of stochastically homogeneous magnetic field advected by incompressible turbulent flow wit...
Kinematic dynamo in incompressible isotropic turbulent flows with high magnetic Prandtl number is co...
Context. Direct numerical simulations of plasmas have shown that the dynamo effect is efficient eve...
In a recent publication, viz. [Phys. Lett. A 326 (2004) 267], Jovanovic and Shukla (J. and S. in the...
Funding Information: We acknowledge fruitful discussions with A. Brandenburg, I. Rogachevskii, A. Sc...
Small-scale dynamos play important roles in modern astrophysics, especially on Galactic and extragal...
This paper is a detailed report on a programme of simulations used to settle a long-standing issue i...
In a recent paper Nakagawa and Nishida [1989] have suggested that wavy motions of the neutral sheet ...
We investigate the effect of the surface bipolar magnetic regions (BMR) on the large-scale dynamo di...
We analyze the initial, kinematic stage of magnetic field evolution in an isotropic and homogeneous ...
We consider fluctuations of magnetic field excited by external force and advected by isotropic turbu...
We present numerical simulations of driven magnetohydrodynamic (MHD) turbulence with weak/moderate i...
We discuss the applicability of the kinematic α-effect formalism at high magnetic Reynolds numbers. ...
In this study, we analysed a three-dimensional Taylor decaying vortex under an applied magnetic fiel...
It is conjectured that transport by parallel mass flow in a braided magnetic field, rather than hype...