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We thank the Computational Infrastructure for Geodynamics (http://geodynamics.org) which is funded by the National Science Foundation under awards EAR-0949446, EAR-1550901, and EAR-2149126. We use Rayleigh 1.1.0 ( Featherstone and Hindman, 2016; Featherstone et al., 2022) published under the GPL3 license.
Acknowledgement
We thank the Computational Infrastructure for Geodynamics (http://geodynamics.org) which is funded by the National Science Foundation under awards EAR-0949446, EAR-1550901, and EAR-2149126.
Cite Code As
Featherstone, Nicholas A., Edelmann, Philipp V. F., Gassmoeller, Rene, Matilsky, Loren I., Orvedahl, Ryan J., & Wilson, Cian R. (2022). geodynamics/Rayleigh: Rayleigh Version 1.1.0 (v1.1.0). Zenodo. https://doi.org/10.5281/zenodo.6522806
Primary References
Featherstone, N.A.; Hindman, B.W. (2016), The Spectral Amplitude Of Stellar Convection And Its Scaling In The High-Rayleigh-Number Regime, The Astrophysical Journal, 818 (1) , 32, doi: 10.3847/0004-637X/818/1/32, url: http://stacks.iop.org/0004-637X/818/i=1/a=32?key=crossref.a90f82507dd0eeb7a6e7562d1e4b0210
Secondary References
Please also cite:
Matsui, H.; Heien, E.; Aubert, J.; Aurnou, J.M.; Avery, M.; Brown, B.; Buffett, B.A.; Busse, F.; Christensen, U.R.; Davies, C.J.; Featherstone, N.; Gastine, T.; Glatzmaier, G.A.; Gubbins, D.; Guermond, J.-L.; Hayashi, Y.-Y.; Hollerbach, R.; Hwang, L.J.; Jackson, A.; Jones, C.A.; Jiang, W.; Kellogg, L.H.; Kuang, W.; Landeau, M.; Marti, P.H.; Olson, P.; Ribeiro, A.; Sasaki, Y.; Schaeffer, N.; Simitev, R.D.; Sheyko, A.; Silva, L.; Stanley, S.; Takahashi, F.; Takehiro, S.-ichi; Wicht, J.; Willis, A.P. (2016), Performance benchmarks for a next generation numerical dynamo model, Geochemistry, Geophysics, Geosystems, 17 (5) , 1586-1607, doi: 10.1002/2015GC006159, url: http://doi.wiley.com/10.1002/2015GC006159
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