Dear WRF solar community
I'm a newbie to WRF solar EPS.
I'm trying to run WRF SOLAR EPS in the reference configuration shown in WRF-Solar® EPS | Research Applications Laboratory. and default STOCHPERT.TBL file.
I successfully ran few cases, But I could not find any output parameters corresponding to EPS.
What I understood that that if you run EPS system with 10ensemble members (nens=10 in namelist), there will be 10 different output variables for solar related parameters, like SWDOWN, SWDDNI etc. Please correct me if I'm wrong.
I can find solar related parameters (SWDOWN, SWDDNI etc from FARMS and Radiation schemes, (I modified registry entries)), but not any parameter specific to EPS.
My question is
1) How the output parameters are formated in WRF SOLAR EPS? Would there be one output parameter for each member ?
2) How can I get or calculate GHI, (SWDOWN) or DNI (SWDDNI) corresponding to different EPS members ?
OR
Am I completely wrong with the sense and if I want 10 ensemble members, do I need conduct 10 model simulations with nens= 10 different values ?
Your help is highly appreciated
Thanks
Vineeth PK
I'm a newbie to WRF solar EPS.
I'm trying to run WRF SOLAR EPS in the reference configuration shown in WRF-Solar® EPS | Research Applications Laboratory. and default STOCHPERT.TBL file.
I successfully ran few cases, But I could not find any output parameters corresponding to EPS.
What I understood that that if you run EPS system with 10ensemble members (nens=10 in namelist), there will be 10 different output variables for solar related parameters, like SWDOWN, SWDDNI etc. Please correct me if I'm wrong.
I can find solar related parameters (SWDOWN, SWDDNI etc from FARMS and Radiation schemes, (I modified registry entries)), but not any parameter specific to EPS.
my namelist parametrs at &stoch section is shown belowI can find variables like PALBEDO(Time, num_stoch_levels, south_north, west_east) , PQVAPOR(Time, num_stoch_levels, south_north, west_east) etc
&stoch
multi_perturb = 1
rand_perturb = 1
spdt = -1.0
pert_farms = .true.
pert_farms_albedo = 1.0
pert_farms_aod = 1.0
pert_farms_angexp = 1.0
pert_farms_aerasy = 1.0
pert_farms_qv = 1.0
pert_farms_qc = 1.0
pert_farms_qs = 1.0
pert_deng = .true.
pert_deng_qv = 1.0
pert_deng_qc = 1.0
pert_deng_t = 1.0
pert_deng_w = 1.0
pert_mynn = .true.
pert_mynn_qv = 1.0
pert_mynn_qc = 1.0
pert_mynn_t = 1.0
pert_mynn_qke = 1.0
pert_noah = .true.
pert_noah_qv = 1.0
pert_noah_t = 1.0
pert_noah_smois = 1.0
pert_noah_tslb = 1.0
pert_thom = .true.
pert_thom_qv = 1.0
pert_thom_qc = 1.0
pert_thom_qi = 1.0
pert_thom_qs = 1.0
pert_thom_ni = 1.0
pert_cld3 = .false.
pert_cld3_qv = 1.0
pert_cld3_t = 1.0
num_pert_3d = 15
perturb_bdy = 0
nens = 10
/
My question is
1) How the output parameters are formated in WRF SOLAR EPS? Would there be one output parameter for each member ?
2) How can I get or calculate GHI, (SWDOWN) or DNI (SWDDNI) corresponding to different EPS members ?
OR
Am I completely wrong with the sense and if I want 10 ensemble members, do I need conduct 10 model simulations with nens= 10 different values ?
Your help is highly appreciated
Thanks
Vineeth PK
Last edited: