From: Bill P. <pa...@ki...> - 2011-06-09 17:31:29
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Hi, Oops -- I lied when I said we didn't have a test suite case showing the new way to do irradiated planets. What a surprise to find that the test called 'irradiated_planet' is actually demonstrating the new way! I answered your earlier email before I'd had a morning cup of coffee -- bad idea. ;-) The irradiated_planet example works in 2 steps. The 1st (inlist1) prepares a model for changing to the constant pressure surface boundary condition, and the 2nd (inlist2) switches to the new BC and evolves the planet with it. -B On Jun 9, 2011, at 8:24 AM, Bill Paxton wrote: > Also, you should know that there is another way > to deal with irradiated planets that uses a constant > pressure surface boundary condition following > Guillot & Havel, A&A 527, A20 (2011). > I haven't added a test_suite case for it yet (I'll do that soon!), > but let me know if you are interested in trying it > and I'll provide some more info for you. |