This is the final version. Available on open access from Taylor & Francis via the DOI in this recordThe dataset associated with this article is located in ORE at: https://doi.org/10.24378/exe.1603The Archontis dynamo is a rare example of an MHD dynamo within which forcing drives a dynamo where the flow and magnetic fields are almost perfectly aligned and the energies are approximately equal. In this paper, I expand upon our knowledge of the dynamo by showing that the intermediate steady states of the kinetic and magnetic energies observed by Cameron and Galloway are not a necessary feature of aligned dynamos. Furthermore, I show that the steady state into which the flow and magnetic fields eventually evolve is remarkably robu...
We provide a theory of dynamo (α effect) and momentum transport in three-dimensional magnetohydrodyn...
Magnetic fields are ubiquitous in the Universe. The energy density of these fields is typically comp...
This is the final version of the article. Available from OUP via the DOI in this record.The research...
The article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/37966The ...
This paper gives new results concerning magnetic field generation leading to a steady equilibrated s...
Magnetic fields are ubiquitous within astrophysical settings. There is strong evidence to suggest th...
11 pagesInternational audienceA three-dimensional numerical computation of magnetohydrodynamic dynam...
A variational optimization approach is used to optimize kinematic dynamos in a unit sphere and locat...
A three-dimensional numerical computation of magnetohydrodynamic dynamo behavior is described. The d...
The small-scale turbulent dynamo (SSD) is likely to be responsible for the magnetisation of the inte...
Our theoretical and numerical analysis have suggested that for low-mass main sequences stars (of the...
A sphere containing electrically conducting fluid can generate a magnetic field by dynamo action, pr...
4 pages, 4 figuresWe compute numerically the threshold for dynamo action in Taylor-Green swirling fl...
Planetary magnetic fields are generated by the motion of conductive fluid in the planet's interior. ...
Context.We present results from non linear MHD dynamo experiments with a three-dimensional steady an...
We provide a theory of dynamo (α effect) and momentum transport in three-dimensional magnetohydrodyn...
Magnetic fields are ubiquitous in the Universe. The energy density of these fields is typically comp...
This is the final version of the article. Available from OUP via the DOI in this record.The research...
The article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/37966The ...
This paper gives new results concerning magnetic field generation leading to a steady equilibrated s...
Magnetic fields are ubiquitous within astrophysical settings. There is strong evidence to suggest th...
11 pagesInternational audienceA three-dimensional numerical computation of magnetohydrodynamic dynam...
A variational optimization approach is used to optimize kinematic dynamos in a unit sphere and locat...
A three-dimensional numerical computation of magnetohydrodynamic dynamo behavior is described. The d...
The small-scale turbulent dynamo (SSD) is likely to be responsible for the magnetisation of the inte...
Our theoretical and numerical analysis have suggested that for low-mass main sequences stars (of the...
A sphere containing electrically conducting fluid can generate a magnetic field by dynamo action, pr...
4 pages, 4 figuresWe compute numerically the threshold for dynamo action in Taylor-Green swirling fl...
Planetary magnetic fields are generated by the motion of conductive fluid in the planet's interior. ...
Context.We present results from non linear MHD dynamo experiments with a three-dimensional steady an...
We provide a theory of dynamo (α effect) and momentum transport in three-dimensional magnetohydrodyn...
Magnetic fields are ubiquitous in the Universe. The energy density of these fields is typically comp...
This is the final version of the article. Available from OUP via the DOI in this record.The research...