Convection in Low-Mass Stars

Jane Pratt, Georgia State University

Usage Details

In order to produce new and improved models for stellar evolution, this team uses the Multi-dimensional Stellar Implicit Code (MUSIC) to study realistic nonlinear fluid dynamics in the interior of a young solar-like star. The models produced from this work will allow to better interpret data from space missions and observatories, including data on topics like stellar winds and space weather, and the environmental conditions of extra-solar planets.