Not listed WE PROPOSE TO STUDY THE ETECTS OF MAGNETISM ON THE DYNAMICS AND STRUCTURE OF CLOSE IN EXTRASOLAR GIANT PLANETS USING A THREE DIMENSIONAL 3D SPHERICAL MAGNETO HYDRODYNAMIC MHD MODEL WITH SIMPLIFIED RADIATIVE FORCING. THE WORK WILL ADDRESS TWO FUNDAMENTAL ISSUES 1. HOW PLANETARY MAGNETIC ELDS A_ECT THE DYNAMICS ON THESE TIDALLY LOCKED PLANETS AND 2. THE POSITION AND AMPLITUDE OF OHMIC DISSIPATION WITHIN THE PLANETARY ATMOSPHERE. THIS STUDY IS MOTIVATED BY THE GROWING NUMBER OF CLAIMS THAT MAGNETISM COULD CAUSE BOTH THE OBSERVED INATED RADII OF MANY EXTRASOLAR GIANT PLANETS AS WELL AS THE VARIATION IN DAYSIDE NIGHT SIDE TEMPERATURE CONTRAST. PREVIOUS MODELS HAVE BEEN HIGHLY SUGGESTIVE AND ENLIGHTENING YET IT IS CLEAR THAT MORE RIGOROUS INVESTIGATIONS ARE NECESSARY IN ORDER TO UNDERSTAND THE INTERPLAY BETWEEN PLANETARY ATMOSPHERIC DYNAMICS AND MAGNETISM. WE WILL CARRY OUT THE REST SELF CONSISTENT NUMERICAL SIMULATIONS OF THE MHD ON THESE PLANETS IN ORDER TO ASCERTAIN UNDER WHAT CONDITIONS AND WITH WHAT MAGNITUDE PLANETARY MAGNETISM AECTS WINDS AND CONTRIBUTES TO THE THERMAL EVOLUTION OF THE PLANET. ($457) 11/28/18 3 WE PROPOSE TO STUDY THE ETECTS OF MAGNETISM ON THE DYNAMICS AND STRUCTURE OF CLOSE IN EXTRASOLAR GIANT PLANETS USING A THREE DIMENSIONAL 3D, SPHERICAL, MAGNETO HYDRODYNAMIC MHD MODEL WITH SIMPLIFIED RADIATIVE FORCING. THE WORK WILL ADDRESS TWO FUNDAMENTAL ISSUES 1. HOW PLANETARY MAGNETIC ELDS A_ECT THE DYNAMICS ON THESE TIDALLY LOCKED PLANETS AND 2. THE POSITION AND AMPLITUDE OF OHMIC DISSIPATION WITHIN THE PLANETARY ATMOSPHERE. THIS STUDY IS MOTIVATED BY THE GROWING NUMBER OF CLAIMS THAT MAGNETISM COULD CAUSE BOTH THE OBSERVED INATED RADII OF MANY EXTRASOLAR GIANT PLANETS AS WELL AS THE VARIATION IN DAYSIDE NIGHT SIDE TEMPERATURE CONTRAST. PREVIOUS MODELS HAVE BEEN HIGHLY SUGGESTIVE AND ENLIGHTENING, YET IT IS CLEAR THAT MORE RIGOROUS INVESTIGATIONS ARE NECESSARY IN ORDER TO UNDERSTAND THE INTERPLAY BETWEEN PLANETARY ATMOSPHERIC DYNAMICS AND MAGNETISM. WE WILL CARRY OUT THE REST SELF CONSISTENT NUMERICAL SIMULATIONS OF THE MHD ON THESE PLANETS IN ORDER TO ASCERTAIN UNDER WHAT CONDITIONS AND WITH WHAT MAGNITUDE PLANETARY MAGNETISM AECTS WINDS AND CONTRIBUTES TO THE THERMAL EVOLUTION OF THE PLANET. Funding Only Action ($457) 11/28/18 2 WE PROPOSE TO STUDY THE ETECTS OF MAGNETISM ON THE DYNAMICS AND STRUCTURE OF CLOSE IN EXTRASOLAR GIANT PLANETS USING A THREE DIMENSIONAL 3D, SPHERICAL, MAGNETO HYDRODYNAMIC MHD MODEL WITH SIMPLIFIED RADIATIVE FORCING. THE WORK WILL ADDRESS TWO FUNDAMENTAL ISSUES 1. HOW PLANETARY MAGNETIC ELDS A_ECT THE DYNAMICS ON THESE TIDALLY LOCKED PLANETS AND 2. THE POSITION AND AMPLITUDE OF OHMIC DISSIPATION WITHIN THE PLANETARY ATMOSPHERE. THIS STUDY IS MOTIVATED BY THE GROWING NUMBER OF CLAIMS THAT MAGNETISM COULD CAUSE BOTH THE OBSERVED INATED RADII OF MANY EXTRASOLAR GIANT PLANETS AS WELL AS THE VARIATION IN DAYSIDE NIGHT SIDE TEMPERATURE CONTRAST. PREVIOUS MODELS HAVE BEEN HIGHLY SUGGESTIVE AND ENLIGHTENING, YET IT IS CLEAR THAT MORE RIGOROUS INVESTIGATIONS ARE NECESSARY IN ORDER TO UNDERSTAND THE INTERPLAY BETWEEN PLANETARY ATMOSPHERIC DYNAMICS AND MAGNETISM. WE WILL CARRY OUT THE REST SELF CONSISTENT NUMERICAL SIMULATIONS OF THE MHD ON THESE PLANETS IN ORDER TO ASCERTAIN UNDER WHAT CONDITIONS AND WITH WHAT MAGNITUDE PLANETARY MAGNETISM AECTS WINDS AND CONTRIBUTES TO THE THERMAL EVOLUTION OF THE PLANET. Other Administrative Action $0 8/1/17 Not listed WE PROPOSE TO STUDY THE ETECTS OF MAGNETISM ON THE DYNAMICS AND STRUCTURE OF CLOSE IN EXTRASOLAR GIANT PLANETS USING A THREE DIMENSIONAL 3D SPHERICAL MAGNETO HYDRODYNAMIC MHD MODEL WITH SIMPLIFIED RADIATIVE FORCING. THE WORK WILL ADDRESS TWO FUNDAMENTAL ISSUES 1. HOW PLANETARY MAGNETIC ELDS A_ECT THE DYNAMICS ON THESE TIDALLY LOCKED PLANETS AND 2. THE POSITION AND AMPLITUDE OF OHMIC DISSIPATION WITHIN THE PLANETARY ATMOSPHERE. THIS STUDY IS MOTIVATED BY THE GROWING NUMBER OF CLAIMS THAT MAGNETISM COULD CAUSE BOTH THE OBSERVED INATED RADII OF MANY EXTRASOLAR GIANT PLANETS AS WELL AS THE VARIATION IN DAYSIDE NIGHT SIDE TEMPERATURE CONTRAST. PREVIOUS MODELS HAVE BEEN HIGHLY SUGGESTIVE AND ENLIGHTENING YET IT IS CLEAR THAT MORE RIGOROUS INVESTIGATIONS ARE NECESSARY IN ORDER TO UNDERSTAND THE INTERPLAY BETWEEN PLANETARY ATMOSPHERIC DYNAMICS AND MAGNETISM. WE WILL CARRY OUT THE REST SELF CONSISTENT NUMERICAL SIMULATIONS OF THE MHD ON THESE PLANETS IN ORDER TO ASCERTAIN UNDER WHAT CONDITIONS AND WITH WHAT MAGNITUDE PLANETARY MAGNETISM AECTS WINDS AND CONTRIBUTES TO THE THERMAL EVOLUTION OF THE PLANET. $0 8/1/17 Not listed WE PROPOSE TO STUDY THE ETECTS OF MAGNETISM ON THE DYNAMICS AND STRUCTURE OF CLOSE IN EXTRASOLAR GIANT PLANETS USING A THREE DIMENSIONAL 3D, SPHERICA $122.8k 8/19/15