Status:
Actively adding features to support improved science or performance by CIG.
Code changes:
Community:
Geodynamics Forum
Bug reports:
Github Issue Tracker
License:
GNU Public License
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 and Chebyshev polynomials in the radial direction. The code has undergone extensive accuracy testing using the Christensen et al. (2001) Boussinesq benchmarks and the Jones et al. (2011) anelastic benchmarks. Rayleigh has been developed with NSF support through the Computational Infrastructure for Geodynamics (CIG).
DOWNLOAD LATEST RELEASE - V1.0.0, *** HERE ***
This release fixes a number of bugs that could cause crashes at output time.
User Manual
The Rayleigh user manual is available online.
Community Wiki
Visit the Rayleigh Wiki page for additional support with building, using, or modifying Rayleigh.
Rayleigh Publications List
Research publications using Rayleigh.
Community Discussion
Browse the CIG Mailing List Archive to find past discussions and previous troubleshooting help, or post to the CIG forum with questions or comments.
Development Version
If you are interested in getting the development version of this code from the CIG repository, use the following git command:
git clone --recursive --branch master https://github.com/geodynamics/rayleigh.git
You can also browse the history of modifications in the Git repository.
Issue/Bug Tracker on Github
Browse and/or submit new issues at our Github Issues Tracker.