UPP  11.0.0
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CALRAD_WCLOUD_newcrtm.f File Reference

Subroutine that computes model derived brightness temperature. More...

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Functions/Subroutines

subroutine calrad_wcloud
 
REAL function effr (pmid, t, q, qqw, qqi, qqr, f_rimef, nlice, nrain, qqs, qqg, qqnr, qqni, qqnw, mp_opt, species)
 
REAL function gammln (XX)
 
REAL function wgamma (y)
 

Detailed Description

Subroutine that computes model derived brightness temperature.

This routine computes model derived brightness temperature using CRTM. It is patterned after GSI setuprad with Treadon's help.

Program history log:

Date Programmer Comments
2007-01-17 H Chuang Initial
2011-02-06 Jun Wang add grib2 option
2014-12-09 WM Lewis added function EFFR to compute effective particle radii channel selection using LVLS from WRF_CNTRL.PARM
2019-04-01 Sharon Nebuda Added output option for GOES-16 & GOES-17 ABI IR Channels 7-16
2020-04-09 Tracy Hertneky Added Himawari-8 AHI CH7-CH16
2021-01-10 Wen Meng Added checking points for skiping grids with filling value spval
2021-03-11 Bo Cui improve local arrays memory
2021-08-31 Lin Zhu added ssmis-f17 channels 15-18 grib2 output
2021-09-02 Bo Cui Decompose UPP in X direction
2022-05-26 WM Lewis added support for GOES-18 ABI IR Channels 7-16
2022-09-12 Wen Meng Added cloud fraction changes for crtm/2.4.0
2023-03-22 WM Lewis Added support for using effective radius arrays from RRFS
Author
Chuang
Date
2007-01-17

Definition in file CALRAD_WCLOUD_newcrtm.f.