Dear Wang,
yes, the differences between absorption models can be large at
individual frequencies, so the value is not impossible. Maybe Alex, here
on Cc, who is working at these frequencies and in this geometry could
also comment?
Best wishes,
Stefan
On 30 Oct 2020, at 8:48, Wenyu Wang
Hi,
Answering your second question, you can add SurfaceDummy to your
iy_surface_agenda. See here:
https://atmtools.github.io/arts-docs-2.4/docserver/methods/SurfaceDummy.html
Cheers,
Oliver
> On 30 Oct 2020, at 08:48, Wenyu Wang wrote:
>
> Dear Everyone,
>
> I had some questions:
>
>
>
Dear Everyone,
I had some questions:
1. When I using line-by-line and MPM93(or PWR98) to calculate the brightness
temperatures, the difference between the results can be more than 20 K at about
50 and 70 GHz in the nadir observation (especially when the reflectivity is
large). Is this