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
Loren I. Matilsky, (2022), "Dynamics of Rotation and Magnetism in the Sun's Convection Zone and Tachocline", ProQuest Dissertations Publishing, 29065353: University of Colorado at Boulder, . Cited by:
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:
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:
Featherstone, Nicholas A., Edelmann, Philipp V. F., Gassmoeller, Rene, Matilsky, Loren I., Orvedahl, Ryan J., Wilson, Cian R., (2021), "Rayleigh 1.0.0", Zenodo: Nov, (DOI: 10.5281/zenodo.5683601). Cited by:
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:
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:
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:
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:
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:
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: