22 Oct 2021 | | Contributor(s):: Nicholas Featherstone (primary-developer), Philip Edelmann (primary-developer), Rene Gassmoeller (primary-developer), Loren Matilsky (primary-developer), Ryan Orvedahl (primary-developer), Cian Wilson (primary-developer)
Rayleigh is a 3-D convection code designed for the study of dynamo behavior in spherical shell geometry. It evolves the incompressible and anelastic MHD equations in spherical geometry using a pseudo-spectral approach. Rayleigh employs spherical harmonics in the horizontal direction...
22 Oct 2021 | | Contributor(s):: Hiroaki Matsui (primary-developer)
Calypso is a set of codes for magnetohydrodynamics (MHD) dynamo simulation in a rotating spherical shell using spherical harmonics expansion methods. Solve MHD equations in a rotating spherical shell Treat conductive fluid with Boussinesq approximation Inner core can have...
21 Oct 2021 | | Contributor(s):: Gary Glatzmaier (primary-developer), Uli Christensen (primary-developer), Peter Olsen (primary-developer)
MAG is a serial version of a rotating spherical convection/magnetoconvection/dynamo code, developed by Gary Glatzmaier and modified by Uli Christensen and Peter Olson.