Dear all,
I stumbled accross this interesting paper on an open C library for particularly
efficient MC calculations. Could this be the basis of ARTS 3D MC flux and
heating rate calculations? Using MC sampling also for the spectral dimension,
to be efficient, as in the second paper, which is
Leo,
If you want to know the complete path through the atmosphere, you can do
as you outline. If you only are interested in where you end up at the
surface, you can use the geo_pos mechanism. You need to set geo_pos by
adding the WSM: geo_posEndOfPpath
Exactly how geo_pos is handled has
Hi Richard,
many thanks for your answer. I try to answer to your questions.
I am using ARTS 2.5.0
My entry point is 'yCalc', you are correct. I have some Python script
which call ARTS commands, so I would say that I run ARTS via custom
language interface.
Currently, I am getting and saving
