The strong magnetic field of neutron stars is intimately coupled to the observed temperature
and spectral properties, as well as to the observed timing properties (distribution of spin …

In 1995, two groups [Kageyama et al., 1995; Glatzmaier and Roberts, 1995a, 1995b]
reported results of numerical integrations of fully three‐dimensional, fully nonlinear …

Speculation about its possible super-rotation has drawn the attention of many geophysical
researchers to the Earth's inner core. An issue of special interest for geodynamo modelling …

Magnetism is one of the most pervasive features of the Universe, with planets, stars and
entire galaxies all having associated magnetic fields. All of these fields are generated by the …

Equations arising in general relativity are usually too complicated to be solved analytically
and one must rely on numerical methods to solve sets of coupled partial differential …

Although the origin of Earth's and other celestial bodies' magnetic fields remains unknown,
we do know that the motion of electrically conducting fluids generates and maintains these …

Numerical simulations of the geodynamo have successfully represented many observable
characteristics of the geomagnetic field, yielding insight into the fundamental processes that …

There has been significant progress in the development of numerical geodynamo models
over the last five years. Advances in computer technology have made it possible to perform …

▪ Abstract The past seven years have seen significant advances in computational
simulations of convection and magnetic field generation in the Earth's core. Although …

In this work the authors draw upon their expertise in geophysical and astrophysical MHD to
explore the motion of electrically conducting fluids, the so-called dynamo effect, and …