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Rayleigh

By Nicholas Featherstone (primary-developer)1, Philip Edelmann (primary-developer)2, Rene Gassmoeller (primary-developer)3, Loren Matilsky (primary-developer)4, Ryan Orvedahl (primary-developer)5, Cian Wilson (primary-developer)6

1. Southwest Research Institute 2. Los Alamos National Lab 3. University of Florida 4. University of Colorado Boulder 5. University of California Davis 6. Carnegie DTM

Citations Non-affiliated (12) | Affiliated (2)

Non-affiliated authors

  • Orvedahl, R. J., Featherstone, N. A., Calkins, M. A., (2021), "Large-scale magnetic field saturation and the Elsasser number in rotating spherical dynamo models", Monthly Notices of the Royal Astronomical Society: Letters, 507, 1: pg: 67, (DOI: 10.1093/mnrasl/slab097). Cited by:

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  • Orvedahl, R. J., (2021), "Numerical Simulations of Convection and Convection-Driven Dynamos in Spherical Shells", ProQuest Dissertations and Theses: University of Colorado at Boulder, . Cited by:

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  • Calkins, M. A., Orvedahl, R. J., Featherstone, N. A., (2021), "Large-scale balances and asymptotic scaling behaviour in spherical dynamos", Geophysical Journal International, 227, 2: pg: 1228--1245, (DOI: 10.1093/gji/ggab274). Cited by:

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  • 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", Zenodo: Nov, (DOI: 10.5281/zenodo.5683601). Cited by:

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  • Orvedahl, R. J., Calkins, M. A., Featherstone, N. A., Hindman, B. W., (2018), "Prandtl-number Effects in High-Rayleigh-number Spherical Convection", The Astrophysical Journal, 856, 1: pg: 13, (DOI: 10.3847/1538-4357/aaaeb5). Cited by:

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  • Miquel, B., Xie, J-H, Featherstone, N., Julien, K., Knobloch, E., (2018), "Equatorially trapped convection in a rapidly rotating shallow shell", Physical Review Fluids, 3, 5: (DOI: 10.1103/PhysRevFluids.3.053801). Cited by:

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  • Karak, B. B., Miesch, M., Bekki, Y., (2018), "Consequences of high effective Prandtl number on solar differential rotation and convective velocity", Physics of Fluids, 30, 4: pg: 046602, (DOI: 10.1063/1.5022034). Cited by:

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  • Driscoll, P. E., Wilson, C., (2018), "Paleomagnetic Biases Inferred From Numerical Dynamos and the Search for Geodynamo Evolution", Frontiers in Earth Science, 6: pg: 113, (DOI: 10.3389/feart.2018.00113). Cited by:

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  • Featherstone, N., (2018), "Rayleigh 0.9.1", : (DOI: 10.5281/zenodo.1236565). Cited by:

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  • O'Mara, B., Miesch, M. S., Featherstone, N. A., Augustson, K. C., (2016), "Velocity amplitudes in global convection simulations: The role of the Prandtl number and near-surface driving", Advances in Space Research, 58, 8: pg: 1475--1489, (DOI: 10.1016/j.asr.2016.03.038). Cited by:

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  • 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: pg: 32, (DOI: 10.3847/0004-637X/818/1/32). Cited by:

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  • Featherstone, N. A., Hindman, B. W., (2016), "The Emergence Of Solar Supergranulation As A Natural Consequence Of Rotationally Constrained Interior Convection", The Astrophysical Journal, 830, 1: pg: L15, (DOI: 10.3847/2041-8205/830/1/L15). Cited by:

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Affiliated authors

  • Buffett, B., Matsui, H., (2019), "Equatorially trapped waves in Earth's core", Geophysical Journal International, 218, 2: pg: 1210--1225, (DOI: 10.1093/gji/ggz233). Cited by:

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  • Featherstone, N., (2018), "Rayleigh Version 0.9.0", Computational Infrastructure for Geodynamics, Davis, CA: (DOI: 10.5281/zenodo.1158290). Cited by:

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