HWRF Ferrier-Aligo Microphysics Scheme | This is the CCPP-compliant FER_HIRES driver module |
GFDL In-Core Fast Saturation Adjustment Module | The subroutine 'fv_sat_adj' implements the fast processes in the GFDL Cloud MP. It is part of the GFDL Cloud MP |
▼GFDL Cloud Microphysics Module | This is cloud microphysics package for GFDL global cloud resolving model. The algorithms are originally derived from Lin et al. (1983) [131]. Most of the key elements have been simplified/improved. This code at this stage bears little to no similarity to the original Lin MP. Therefore, it is best to be called GFDL microphysics (GFDL MP) |
GFDL Cloud MP modules | This module contains the column GFDL Cloud microphysics scheme |
▼Morrison-Gettelman MP Driver Module | This subroutine is the Morrison-Gettelman MP driver, which computes grid-scale condensation and evaporation of cloud condensate |
Morrison-Gettelman MP aer_cloud Module | according to the models of Nenes & Seinfeld (2003) [165], Fountoukis and Nenes (2005) [66] and Barahona and Nenes (2008, 2009) [13] [14] . *** Code Developer: Donifan Barahona donif.nosp@m.an.o.nosp@m..bara.nosp@m.hona.nosp@m.@nasa.nosp@m..gov |
Morrison-Gettelman MP cldmacro Module | This module contains MG cloud macrophysics scheme |
Morrison-Gettelman MP cldwat2m_micro Module | This module contains CAM interface for MG microphysics |
Morrison-Gettelman MP version 2.0 | This module includes the MG microphysics version 2.0 - update of MG microphysics with prognostic precipitation |
Morrison-Gettelman MP utils Module | This module contains process rates and utility functions used by the MG microphysics |
Morrison-Gettelman MP wv_saturation Module | This module contain some utility functions for saturation vapor pressure |
▼NSSL MP Module | This module contains the front end to NSSL microphysics scheme |
NSSL 2-moment microphysics modules | This module provides a 1/2/3-moment bulk microphysics scheme based on a combination of Straka and Mansell (2005, JAM) and Zeigler (1985, JAS) and modified/upgraded in in Mansell, Zeigler, and Bruning (2010, JAS). Two-moment adaptive sedimentation follows Mansell (2010, JAS), using parameter infall = 4 |
Aerosol-Aware Thompson MP Module | This module contains the aerosol-aware Thompson microphysics scheme |
GFS gscond Main | This subroutine computes grid-scale condensation and evaporation of cloud condensate |
GFS precpd Main | This subroutine computes the conversion from condensation to precipitation (snow or rain) or evaporation of rain |
▼Grell-Freitas Convection Module | This is the Grell-Freitas scale and aerosol aware scheme |
C3 Deep Convection Module | This is C3 deep convection scheme module |
Grell-Freitas Convection Driver Module | This is Grell-Freitas cumulus scheme driver module |
Grell-Freitas Shallow Convection Module | This module contains Grell-Freitas shallow convection scheme.GF shallow convection as described in Grell and Freitas (2014) [82]. input variables are: |
Chikira-Sugiyama Cumulus Scheme Module | The subroutine contains the main driver for Chikira-Sugiyama convective scheme |
CSAW adjustment Module | This module adjusts surface rainrate for conservation |
▼Grell-Freitas Convection Module | This is the Grell-Freitas scale and aerosol aware scheme |
Grell-Freitas Deep Convection Module | This is Grell-Freitas deep convection scheme module |
Grell-Freitas Convection Driver Module | This is Grell-Freitas cumulus scheme driver module |
Grell-Freitas Shallow Convection Module | This module contains Grell-Freitas shallow convection scheme.GF shallow convection as described in Grell and Freitas (2014) [82]. input variables are: |
Relaxed Arakawa-Schubert Convection Scheme | |
GFS saSAS Deep Convection Module | This subroutine contains the entirety of the SAMF deep convection scheme |
GFS saSAS Shallow Convection Module | This subroutine contains the entirety of the SAMF shallow convection scheme.This routine follows the GFS saSAS Deep Convection Module quite closely, although it can be interpreted as only having the "static" and "feedback" control portions, since the "dynamic" control is not necessary to find the cloud base mass flux. The algorithm is simplified from SAMF deep convection by excluding convective downdrafts and being confined to operate below \(p=0.7p_{sfc}\). Also, entrainment is both simpler and stronger in magnitude compared to the deep scheme |
Simplified Arakawa-Schubert Deep Convection | The Simplified Arakawa-Schubert scheme parameterizes the effect of deep convection on the environment (represented by the model state variables) in the following way. First, a simple cloud model is used to determine the change in model state variables due to one entraining/detraining cloud type, per unit cloud-base mass flux. Next, the total change in state variables is retrieved by determining the actual cloud base mass flux using the quasi-equilibrium assumption, whereby convection is assumed to be steady-state. This implies that the generation of the cloud work function (interpreted as entrainment-moderated convective available potential energy (CAPE)) by the large scale dynamics is in balance with the consumption of the cloud work function by the convection |
CIRES UGWP orowam2017 Module | This is the OROGW-solver of WAM2017 |
▼CIRES Unified Gravity Wave Physics v0 Module | @ The subroutine initializes the CIRES UGWP V0 |
GFS UGWP V0 Driver Module | This is the CIRES UGWP V0 driver module |
cires_ugwp_post Module | This module contains code run cires_ugwp afterwards.The subroutine initializes the CIRES UGWP |
GFS Convective Gravity Wave Drag Module | This subroutine is the parameterization of convective gravity wave drag based on the theory given by Chun and Baik (1998) [44] modified for implementation into the GFS/CFS by Ake Johansson(Aug 2005) |
GFS gwdps Module | This subroutine includes orographic gravity wave drag and mountain blocking |
GFS Rayleigh Damping Module | This is the Rayleigh friction calculation with total energy conservation |
ugwpv1_gsldrag Scheme Post | |
GFS Unified Gravity Wave Physics Module | This is the CCPP entry points for unified GWP scheme v0 |
unified_UGWP Scheme Post | The subroutine saves CIRES UGWP diagnostics |
MYNN Surface Layer Module | This scheme (1) performs pre-mynnsfc work, (2) runs the mynn sfc layer scheme, and (3) performs post-mynnsfc work |
GFS sfc_diag module | This module contains the land surface diagose calculation |
GFS sfc_diag_post Module | This module contains code related to the surface diagnostic scheme |
GFS Surface Layer Module | This module calculates surface roughness length.This subroutine includes the surface roughness length formulation based on the surface sublayer scheme in Zeng and Dickinson (1998) [231] |
▼GFS Near-Surface Sea Temperature Module | This module contains the CCPP-compliant GFS near-surface sea temperature scheme.This subroutine calls the Thermal Skin-layer and Diurnal Thermocline models to update the NSST profile |
GFS NSST Diurnal Thermocline Model | This module contains the diurnal thermocline layer model (DTM) of the GFS NSST scheme |
GFS NSST Parameter Module | This module contains constants and parameters used in GFS near surface sea temperature scheme. history: 20210305: X.Li, reduce z_w_max from 30 m to 20 m |
GFS NSST Water Property | This module contains GFS NSST water property subroutines |
GFS Near-Surface Sea Temperature Pre | |
GFS Hybrid Eddy-Diffusivity Mass-Flux (HEDMF) Scheme Module | This subroutine contains all of logic for the Hybrid EDMF PBL scheme except for the calculation of the updraft properties and mass flux |
MYNN-EDMF PBL and Shallow Convection Module | This scheme (1) performs pre-mynnedmf work, (2) runs the mynnedmf, and (3) performs post-mynnedmf work |
GFS Scale-aware TKE-based Moist Eddy-Diffusivity Mass-flux (TKE-EDMF) Scheme Module | This subroutine contains all of the logic for the scale-aware TKE-based moist eddy-diffusion mass-flux (TKE-EDMF) scheme |
GFS TKE-EDMF PBL Module | This file contains the CCPP-compliant SATMEDMF scheme (updated version) which computes subgrid vertical turbulence mixing using scale-aware TKE-based moist eddy-diffusion mass-flux (TKE-EDMF) parameterization (by Jongil Han) |
FV3GFS shinhongvdif_run Main | This subroutine contains all of the logic for the scale-aware Shinhong scheme |
FV3GFS ysuvdif_run Main | This subroutine contains all of the logic for the YSU scheme |
GFS Noah LSM Model | This is Noah LSM driver module, with the functionality of preparing variables to run Noah LSM gfssflx(), calling Noah LSM and post-processing variables for return to the parent model suite including unit conversion, as well as diagnotics calculation |
GFS Surface Perturbation Module | This module contains routines used in the percentile matching algorithm for the albedo and vegetation fraction perturbations |
NoahMP LSM Model | This is the NoahMP LSM driver module, with the functionality of preparing variables to run the NoahMP LSM subroutine noahmp_sflx(), calling NoahMP LSM and post-processing variables for return to the parent model suite including unit conversion, as well as diagnotics calculation |
RUC LSM Model | This module contains the RUC Land Surface Model developed by NOAA/GSL (Smirnova et al. 2016 [204]) |
GFS Simple Ocean Module | This subroutine calculates thermodynamical properties over open water |
GFS sfc_sice Module | This is three-layer thermodynomics sea-ice model based on Winton (2000) [219] |
GFS Water Vapor Photochemical Module | This subroutine is NRL H2O physics for stratosphere and mesosphere |
Mersenne Twister Module | Module: mersenne_twister Modern random number generator |
Radiation Aerosols Module | This module contains climatological atmospheric aerosol schemes for radiation computations |
Radiation Astronomy Module | This module sets up astronomical quantities for solar radiation calculations |
Radiation Cloud Overlap Module | This module contains the calculation of cloud overlap parameters for both RRTMG and RRTMGP |
Radiation Clouds Module | This module computes cloud related quantities for radiation computations.Knowledge of cloud properties and their vertical structure is important for meteorological studies due to their impact on both the Earth's radiation budget and adiabatic heating within the atmosphere. Cloud properties in the US National Oceanic and Atmospheric Administration National Centers for Environmental Prediction Global Forecast System (GFS) include (i) cloud liquid/ice water path; (ii) the fraction of clouds; (iii) effective radius of water/ice droplet: |
Radiation Gases Module | This module sets up constant gas profiles, such as co2, ch4, n2o, o2, and those of cfc gases. All data are entered as mixing ratio by volume |
Radiation Surface Module | This module sets up surface albedo for SW radiation and surface emissivity for LW radiation |
GFS RRTMG-LW Main Module | This module includes NCEP's modifications of the RRTMG-LW radiation code from AER.The RRTMG-LW package includes three files: |
GFS RRTMG-SW Main Module | This module includes NCEP's modifications of the RRTMG-SW radiation code from AER |
GFS RRTMG scheme post | This module saves RRTMG-LW fluxes results |
GFS RRTMG-SW scheme post | This module saves two spectral bands' surface downward and upward fluxes for output |
GFS Physics Constants Module | This module contains some of the most frequently used math and physics constants for GCM models |
GFS Physics Function Module | This module provides API for computing basic thermodynamic physics functions |
GFS Convective Cloud Diagnostics Module | This module contains the calculation of fraction of convective cloud, pressure at bottom of convective cloud and at top of convective cloud |
RRTMG dcyc2t3 Module | This module contains the CCPP-compliant dcyc2t3 codes that fits radiative fluxes and heating rates from a coarse radiation calculation time interval into model's more frequent time steps |
GFS Cloud Diagnostics Module | This module contains code to produce the UFS High/Mid/Low cloud-diagnostics. This was bundled together with the prognostic cloud modules within the RRTMG implementation. For the RRTMGP implementation we propose to keep these diagnostics independent |
▼GFS Physics Time Update | This module contains GFS physics time vary subroutines including stratospheric water vapor, aerosol, IN&CCN and surface properties updates |
GFS sfcsub Module | This module contains grib code for each parameter-used in subroutines sfccycle() and setrmsk() |
GFS RRTMG Scheme Post | This module calculate time averaged output quantities (including total-sky and clear-sky SW and LW fluxes at TOA and surface; conventional 3-domain cloud amount, cloud top and base pressure, and cloud top temperature; aerosols AOD, etc.), store computed results in corresponding slots of array fluxr with appropriate time weights |
GFS RRTMG Scheme Pre | This module contains cloud properties calculation for RRTMG |
GFS RRTMG Scheme Setup | This subroutine initializes RRTMG |
GFS surface_generic_post Module | This module contains code related to all GFS surface schemes to be run afterward |
GFS surface_generic_pre module | This module contains code related to running prior to all GFS surface schemes |
GFS_surface_loop_control_part2 Module | This module contains the GFS_surface_loop_control_part2 scheme |
GFS Time Vary Pre Module | This module contains code related to GFS physics suite setup |
sgscloud_radpost_run Module | This interstitial code restores the original resolved-scale clouds (qc and qi) |
sgscloud_radpre_run Module | This interstitial code adds the subgrid clouds to the resolved-scale clouds if there is no resolved-scale clouds in that particular grid box. It can also specify a cloud fraction for resolved-scale clouds as is done currently when using MYNN-EDMF. For clouds coming from the convection schemes (in this case only used by GF scheme), two cloud fraction options are available: Xu-Randall (XR1996) or Chaboureau and Bechtold (CB2005), chosen by the switch "conv_cf_opt" = 0: CB2005, 1: XR1996 |