Rayleigh: Pseudo-spectral MHD
Abstract
The 3-D convection code Rayleigh enables study of dynamo behavior in spherical 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 and has undergone extensive accuracy testing.
- Publication:
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Astrophysics Source Code Library
- Pub Date:
- January 2024
- Bibcode:
- 2024ascl.soft01002F
- Keywords:
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- Software