Lab Mission

  1. Develop fast, accurate, and scalable algorithms for modeling the sun’s interior convection.
  2. Develop an unstructured fully compressible MHD model for the Sun’s convection zone.
  3. Train graduate and undergraduate students to become computational scientists and engineers.
  4. Develop fast reduced-order models for predicting solar dynamo and solar cycles.
  5. Develop a cyberinfrastructure, i.e., the CHORUS++ code for the solar physics community.
  6. Improve the CHORUS++ code for unprecedented resolutions in simulating solar convection and dynamo.