Open mr91i opened 2 years ago
Dear Shoji,
Interesting... Strange indeed! If you do not use mirror symmetry, i.e. just set up a grid that covers both sides of the equatorial plane, does the problem then disappear too?
Do you use second order integration (interpolation-based)? Or just first order (cell based)?
I'd have to look more carefully into this. At the moment I am, however, short on time.
Thanks for reporting this! If I find the origin of the problem, I'll post it here and fix it. Please remind me if I haven't fixed it within a few weeks time.
Best wishes, Kees
Dear Kees,
When I use the grid that covers full theta direction, the velocity asymmetry does not appear.
I have tested only for the first-order integration. I also have tried to use the second order, but the results looks strange: the intensity in the negative velocity completely disappears. This might be related to the issue I have reported originally, but I am not sure at all. Also, this may be due to my lack of understanding of how to use radmc3d, so it may be good to double check. Anyway I hope this also helps our understanding. In case, I attach below the full line of the script.
I know you don't have much time, so please let me know if there is anything I can help.
Best regards, Shoji
problem_setup.py.txt problem_plotexamples.py.txt (Please delete .txt if you use the codes. This is just for a prescription sending python codes in github issue.)
When I was doing synthetic observations of a molecular line for disk-like structure with face-on view, I noticed that the line profile shows asymmetry. I was using the mirror symmetry with a 2d spherical coordinate and a optically thin line, and so the face-on observations should have showed the symmetric line.
I reproduce the issue using a default example file
run_ppdisk_simple_1_line/problem_setup.py
with assuming vtheta = 1 km/s and low molecular abundance:Also, the
plotexample.py
file is like this:The attached figure is the resulting position-velocity diagram. pv.pdf We can see that the intensity for positive velocity is stronger than that for negative velocity.
Actually, when the grid in the θ direction just before the equatorial plane is finer, this symmetry disappear. So, now i am understanding it as the issue on the interpolation at the boundary of mirror symmetry.
Then, I would like to know wether this issue should be addressed on the user side or the code side. Thank you.