Flag | Description
|
---|
Write Absorption spectra
|
Write output spectra as binary files
|
Write Brightness Temperature spectra
|
Write Cooling Rate spectra
|
Write spectra with Double Precision
|
Spectral units GHz rather than cm-1.
|
Write Jacobian spectra
|
Jacobian spectra for
tan. pt. perturbations only
|
Intermediate outputs at specified levels
|
Write Pointing Jacobian spectra
|
Open output files as 'NEW'
|
Write Optical Depth spectra
|
Write out internal profile
|
Write Ray Path diagnostics
|
Write Radiance spectra
|
Write Rayleigh-Jeans
Temperature spectra
|
Suppress terminal progress
messages
|
Write tabulated absorption coefficients
|
Write Transmission spectra
|
Write Widemesh diagnostics
|
Flag | Description
|
---|
Use Planck v. optical depth in layers
|
Flux-type calculations (over solid
angle)
|
Use geometric (cf.refracted) ray paths
|
Assume horizontal gradients (2D atmosphere)
|
Perform Homogeneous path calculation
|
Assume hydrostatic eqlbm
to derive CG paths for plane parallel atmosphere
|
Halve the vertical spacing of the user-supplied profile grid
Automatic sub-layering of profiles
|
Assume VMR varies linearly with
altitude
|
Nadir-viewing
|
Specify Observer Location
|
Specify surface characteristics
|
Flux-type calculations without solid-angle
integration
|
Zenith-viewing
|