Body Text
We thank the Computational Infrastructure for Geodynamics (http://geodynamics.org) which is funded by the National Science Foundation under awards EAR-0949446 and EAR-1550901.We use Rayleigh 1.0.0 ( Featherstone and Hindman, 2016; Featherstone et al., 2021) 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 and EAR-1550901.
Cite Code As
Featherstone, Nicholas A., Edelmann, Philipp V. F., Gassmoeller, Rene, Matilsky, Loren I., Orvedahl, Ryan J., & Wilson, Cian R. (2021). geodynamics/Rayleigh: Rayleigh Version 1.0.0 (v1.0.0). Zenodo. https://doi.org/10.5281/zenodo.5683601
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
CITE PREVIOUS VERSIONS
For previous versions, please substitute the appropriate version number, year, and DOI below. See also: https://doi.org/10.5281/zenodo.1158289
Body Text
We use Rayleigh 0.9.0 ( Featherstone and Hindman, 2016; Featherstone, 2018) 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 and EAR-1550901.
Cite Code As
Featherstone, N. (2018), Rayleigh Version 0.9.0, Computational Infrastructure for Geodynamics, doi: 10.5281/zenodo.1158290, url: https://doi.org/10.5281/zenodo.1158290
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