Dear WRF Community,
I have a question on substitution of ALB/LAI/GVF in WRF V4.0. As for these three, I can replace the equivalent fields through usemonalb = true, rdlai2d = true, and sst_update=1 in namelist.input.
Question 01: if sst_update = 0, usemonalb = false, rdlai2d = false in namelist.input, then:
we are using albedo from TBL, lai from TBL, but GVF (VEGFRAC) from monthly MODIS. This is verified from wrfout* files. Is there a control/switch for GVF (VEGFRAC) from TBL?
Question 02: if I wish to substitute additional fields, such as emissivity, what should I do? The wrflowinp.d0*.nc files do not contain corresponding field.
Question 03: Noah-Unified is used as Land Surface Model. Hence, relative modules to digest these fields are in /phys/module_sf_noahdrv.F?
Thanks in advance.
I have a question on substitution of ALB/LAI/GVF in WRF V4.0. As for these three, I can replace the equivalent fields through usemonalb = true, rdlai2d = true, and sst_update=1 in namelist.input.
Question 01: if sst_update = 0, usemonalb = false, rdlai2d = false in namelist.input, then:
we are using albedo from TBL, lai from TBL, but GVF (VEGFRAC) from monthly MODIS. This is verified from wrfout* files. Is there a control/switch for GVF (VEGFRAC) from TBL?
Question 02: if I wish to substitute additional fields, such as emissivity, what should I do? The wrflowinp.d0*.nc files do not contain corresponding field.
Question 03: Noah-Unified is used as Land Surface Model. Hence, relative modules to digest these fields are in /phys/module_sf_noahdrv.F?
Thanks in advance.