Dear all,
Hello! I met a problem when I was using ARTS's scattering database.
I used a matlab program named demo_ssp4arts.m in DataInterfaces to convert the
scattering data of LargePlateAggregate_Id20 particles in the database from nc
format to the format used internally by ARTS. The results of
Hello,
I would like to do some radiative transfer modeling for Venus. I want to
see about what percentage of photons emitted from the surface of Venus get
scattered/absorbed at various altitudes. The wavelengths I'm interested in
are NIR, 0.7-1.5 microns.
Would ART provide reasonable estimates at t
Dear Song shuhua,
You have discovered one of the reasons why we created the standard
habits. It is difficult to run DDA on the large particles at high
frequencies, and we had a limit at size parameter = 10. This means that
the highest frequencies not are present for all particles.
In the sta
