Rayleigh

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.

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contributed at 2019-07-02

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Application-focused categoriesNatural-perspectiveSolid-earth regions

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English {{currentDetailLanguage}} English

Quoted from: https://geodynamics.org/cig/software/rayleigh/ 

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).

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How to Cite

Yue Songshan (2019). Rayleigh, Model Item, OpenGMS, https://geomodeling.njnu.edu.cn/modelItem/5b2d9222-2d58-40a5-a27d-c198a9ffea03
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Initial contribute: 2019-07-02

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