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Aagaard, B., (2015), "SpatialData v1.9.5 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2014), "SpatialData v1.9.3 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2014), "SpatialData v1.9.4 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2013), "SpatialData v1.9.1 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2012), "SpatialData v1.8.1 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2012), "SpatialData v1.8.2 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2012), "SpatialData v1.9.0 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2011), "SpatialData v0.6.0 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2011), "SpatialData v1.8.0 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2009), "SpatialData v0.5.2 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2008), "SpatialData v0.3.0 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2008), "SpatialData v0.3.1 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagaard, B., (2008), "SpatialData v0.4.0 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagard, B., (2013), "SpatialData v1.9.2 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagard, B., (2011), "SpatialData v0.7.0 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagard, B., (2011), "SpatialData v1.7.1 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aagard, B., (2009), "SpatialData v0.5.1 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Oliva, A., Pinard, F., Tromey, T., (2013), "Nemesis v1.1.0 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Oliva, A., Pinard, F., Tromey, T., (2011), "Nemesis v1.0.2 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Oliva, A., Pinard, F., Tromey, T., (2009), "Nemesis v1.0.1 [software]", : (DOI: NoDOI). Cited by:
Oliva, A., Pinard, F., Tromey, T., (2007), "Nemesis v1.0 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aivazis, M., (2016), "Pythia v0.8.1.17 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aivazis, M., (2013), "Pythia v0.8.1.16 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aivazis, M., (2012), "Pythia v0.8.1.14 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aivazis, M., (2012), "Pythia v0.8.1.15 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aivazis, M., (2011), "Pythia v0.8.1.12 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aivazis, M., (2011), "Pythia v0.8.1.13 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aivazis, M., (2009), "Pythia v0.8.1.8 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aivazis, M., (2009), "Pythia v0.8.1.9 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aivazis, M., (2008), "Pythia v0.8.1.7 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Aivazis, M., (2006), "Pythia v0.8 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Armendariz, L., Kientz, S., (2007), "CIGMA v0.9 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Armendariz, L., Kientz, S., Sunil, A., Mount, D., (2009), "CIGMA v1.0.0 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Armendariz, L., Kientz, S., (2008), "Cigma User Manual", Computational Infrastructure of Geodynamics, Pasadena, CA: . Cited by:
Strand, L., Bothner, P., Oliva, A., Tan, E., (2009), "Exchanger v1.0.1 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
Strand, L., Bothner, P., Oliva, A., Tan, E., (2007), "Exchanger v1.0.0 [software]", Computational Infrastructure for Geodynamics: (DOI: NoDOI). Cited by:
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:
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:
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:
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:
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:
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:
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:
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:
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:
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:
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:
Liu, L., Olson, P., (2009), "Geomagnetic dipole moment collapse by convective mixing in the core", Geophysical Research Letters, 36, 10: pg: L10305, (DOI: 10.1029/2009GL038130). Cited by:
Olson, P., Deguen, R., (2012), "Eccentricity of the geomagnetic dipole caused by lopsided inner core growth", Nature Geoscience, 5, 8: pg: 565--569, (DOI: 10.1038/ngeo1506). Cited by:
Olson, P., Deguen, R., Hinnov, L. A., Zhong, S., (2013), "Controls on geomagnetic reversals and core evolution by mantle convection in the Phanerozoic", Physics of the Earth and Planetary Interiors, 214: pg: 87--103, (DOI: 10.1016/j.pepi.2012.10.003). Cited by:
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