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
Frontiers in Planetary and Stellar Magnetism Through High Performance Computing
The data generated for this project was part of the Frontiers in Planetary and Stellar Magnetism Through High Performance Computing project as part of the Geodynamo Working Group Computational time on Mira and support was provided through the DOE INCITE project. The data consists of two (2) targets the: 1. Geodynamo and 2. Jovian atmosphere. For more information about this data set see: https://incite.geodynamics.org/
More information about this project can be found on the project page. The data for these magnetohydorodynamics (MHD) simulations were generated by the 3-D pseudospectral convection code Rayleigh.