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The biases of radiative fluxes, cloud cover, and surface temperature in GFSv17 are relatively large.
By modifying the Thompson microphysics scheme and its related part in the RRTMG(P) pre interstitial code, it can reduce the biases.
The text was updated successfully, but these errors were encountered:
Fixed in #19
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Description
The biases of radiative fluxes, cloud cover, and surface temperature in GFSv17 are relatively large.
Solution
By modifying the Thompson microphysics scheme and its related part in the RRTMG(P) pre interstitial code, it can reduce the biases.
The text was updated successfully, but these errors were encountered: