Module source

Functions

source_fn_cont

source_fn_line

source_fn_polarized

stokes_angles 🔒

This function rotates the B-field vector from the model frame to the observer frame, then calculates and returns some useful values which will in function source_fn_polarized() make it easy to obtain the Stokes parameters of polarized submillimetre dust emission. (For an explanation of the reasons for choosing the particular quantities we do, see the comment in that function.)