from mcrt3d.grid import CartesianGrid from mcrt3d.dust import Dust from mcrt3d.sources import Star from mcrt3d.camera import Image, Spectrum 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
dpc=1, code="radmc3d", camera_scatsrc_allfreq=True, \
verbose=False)
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#
# Run the model with MCRT3D
#
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# Create a model class.
model = MCRT()
# Set up the dust.
dust = Dust(filename="../examples/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
