Radiative MHD Simulation of a Solar Active Region from Flux Emergence to Coronal Mass Ejections.
Matthias Rempel (NCAR/HAO)
Feng Chen (NCAR/HAO, University of Colorado/LASP)
John Clyne and Matt Rehme (NCAR/CISL)
This work was supported by the National Science Foundation and NCAR’s Advanced Scientific Discovery project.
NASA imagery courtesy of NASA/SDO and the AIA, EVE, and HMI science teams. http://sdo.gsfc.nasa.gov/
The National Center for Atmospheric Research is sponsored by the National Science Foundation. Any opinions, findings and conclusions or recommendations expressed in this material do not necessarily reflect the views of the National Science Foundation.
