UPP
11.0.0
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Subroutine that computes model derived brightness temperature. More...
Go to the source code of this file.
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.
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 |
Definition in file CALRAD_WCLOUD_newcrtm.f.