astromugs.nautilus.coupling

Functions

av_z(field_radmc3d, lam_mono, R_star, ...)	Compute the vertical visual extinction map using physical vertical coordinates.
avz_disk(field_radmc3d, lam_mono, R_star, ...)	Compute the vertical visual extinction map using scale-height-based vertical coordinates.
dust_density(dtogas, rho_m, sizes, ...)	Interpolate RADMC3D dust density onto the Nautilus chemistry grid.
dust_temperature(temp_radmc3d, rchem, zchem, ...)	Remap multi-species RADMC3D dust temperatures onto the Nautilus grid.
dust_temperature_disk(temp_radmc3d, rchem, ...)	Remap multi-species RADMC3D dust temperatures onto the Nautilus grid using scale heights.
dust_temperature_single(temp_radmc3d, rchem, ...)	Remap single-species RADMC3D dust temperature onto the Nautilus grid.
dust_temperature_single_disk(temp_radmc3d, ...)	Remap single-species RADMC3D dust temperature onto the Nautilus grid using scale heights.
local_field()	Compute the local radiation field (placeholder, not yet implemented).
moving_average(x, w)	Compute a moving average using a uniform convolution kernel.
to_spherical(chemmodel, nr, nt, dist, theta)	Convert a Nautilus chemistry structure from cylindrical to spherical coordinates.