WE WILL DIVIDE THREADS OVER THE THREE YEAR PROJECT PERIOD ALLOWING PROGRESS TO HAPPEN RAPIDLY ON SOME OF THE WORK BUT ALLOWING FLEXIBILITY TO RE-ORDER WORK SHOULD WE ENCOUNTER UNEXPECTED NUMERICAL DIFFICULTIES OR SHOULD COMPUTING TIME NOT BE AVAILABLE IN A LINEAR FASHION. YEAR 1: BEGIN TO PERFORM AND ANALYZE MHD STELLAR WIND MASS LOADING SIMULATIONS ( 2.1); BEGIN TO PERFORM AND JET-INTO-TURBULENCE SIMULATIONS ( 2.2). YEAR 2: BEGIN TO PERFORM AND ANALYZE CLUMP SIMULATIONS ( 2.2); BEGIN TO PERFORM RELATIVISTIC VERIFICATION SIMULATIONS. IMPLEMENT SECULAR MASS LOADING SCHEME INFORMED BY RESULTS FROM YEAR 1. YEAR 3: RUN GLOBAL SIMULATIONS OF IDEALIZED EARLY TYPE GALAXIES WITH RADIO MODE FEEDBACK; RUN SIMULATIONS OF FR I/FR II RADIO GALAXIES; DEVELOP OBSERVATIONAL DIAGNOSTICS AND VISUALIZATION TOOLS; COMPLETE PREVIOUS YEAR S WORK.

University Of Wisconsin System, Madison WI

Investigators