THE GOAL FOR THIS PROJECT IS TO DEVELOP A NEW COMPUTATIONAL MODEL OF THE INTERNAL DYNAMICS, TURBULENT ENERGY AND MOMENTUM TRANSPORT, AND MAGNETIC FIELD GENERATION INSIDE THE SUN AND SOLAR-TYPE STARS. THE METHODOLOGY WILL BE BASED ON PERFORMING HIGH-RESOLU
|Effective start/end date
|2/1/17 → 1/31/18
- National Aeronautics and Space Administration
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