from mcrt3d.constants.astronomy import M_sun, R_sun, AU from mcrt3d.constants.physics import c from numpy import array, arange, pi, zeros, logspace from time import time # Create a model class. model = MCRT() # Set up the dust. dust = Dust(filename="dustkappa_yso.inp", radmc3d=True) # Set up the star. star = Star(0.0, 0.0, 0.0, M_sun, R_sun, 4000.0) star.set_blackbody_spectrum(dust.nu) # Set up the grid. nx = 10 ny = 10 nz = 10 x = (arange(nx) - (float(nx) - 1) / 2) * AU / 1 y = (arange(ny) - (float(ny) - 1) / 2) * AU / 1 z = (arange(nz) - (float(nz) - 1) / 2) * AU / 1 density = zeros((nx - 1, ny - 1, nz - 1)) + 1.0e-16 model.set_cartesian_grid(x, y, z)
