Turbulent Convection and Dynamos in Stars
Andrea Malagoli, University of Chicago

Scientific Grand Challenge:
To simulate the solar interior at a fidelity sufficient to understand penetrative convection.

* PPMC - finite volume convection code
** MPS - spectral MHD code
*** HPS - spectral finite difference convection code

ESS Contact Scientists:
- Anil Deane/University of Maryland
- Bruce Fryxell/Drexel University

Table of Contents | Section Contents -- Applications | Subsection Contents -- Science Team II