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

Project Details

Description

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
StatusFinished
Effective start/end date2/1/171/31/18

Funding

  • National Aeronautics and Space Administration

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