diff --git a/doc/UsersGuide/source/InputsOutputs.rst b/doc/UsersGuide/source/InputsOutputs.rst index b03e29f8c9..5ec4e46c53 100644 --- a/doc/UsersGuide/source/InputsOutputs.rst +++ b/doc/UsersGuide/source/InputsOutputs.rst @@ -422,7 +422,7 @@ https://dtcenter.org/GMTB/UFS/sci_doc/CCPPsuite_nml_desp.html The following link describes the stochastic physics namelist records -https://stochastic-physics.readthedocs.io/en/ufs_public_release/namelist_options.html +https://stochastic-physics.readthedocs.io/en/ufs-v1.0.0/namelist_options.html The following link describes some of the other namelist records (dynamics, grid, etc): diff --git a/doc/UsersGuide/source/Introduction.rst b/doc/UsersGuide/source/Introduction.rst index f9045f3bda..d968ec6b1a 100644 --- a/doc/UsersGuide/source/Introduction.rst +++ b/doc/UsersGuide/source/Introduction.rst @@ -27,7 +27,7 @@ for those elements, are listed below: - The stochastic physics capability, including the Stochastic Kinetic Backscatter Scheme (SKEBS), the Stochastically Perturbed Parameterization Tendencies (SPPT) scheme, the perturbed boundary layer humidity (SHUM) scheme, and the cellular automata method - (https://stochastic-physics.readthedocs.io/en/ufs_public_release/). + (https://stochastic-physics.readthedocs.io/en/ufs-v1.0.0/). - The NOAA Environmental Modeling System (:term:`NEMS`) model driver used to create the main program (https://noaa-emc.github.io/NEMS_doc/index.html). diff --git a/doc/UsersGuide/source/RegTests.rst b/doc/UsersGuide/source/RegTests.rst index 6f607abb1d..889c34a83a 100644 --- a/doc/UsersGuide/source/RegTests.rst +++ b/doc/UsersGuide/source/RegTests.rst @@ -242,4 +242,4 @@ Compatibility between the Code Base, the SDF, and the Namelist in the UFS Atmosp The variable ``suite_name`` within the ``namelist.input`` file used in the UFS Atmosphere determines which suite will be employed at run time (e.g., ``suite_name=FV3_GFS_v15``). It is the user’s responsibility to ascertain that the other variables in ``namelist.input`` are compatible with the chosen suite. When runs are executed using the RT framework described in the preceding sections, compatibility is assured. For new experiments, users are responsible for modifying the two files (``SDF`` and ``namelist.input``) consistently, since limited checks are in place. -Information about the UFS Atmosphere physics namelist can be found with the CCPP Scientific Documentation at https://dtcenter.org/GMTB/v3.0/sci_doc/. +Information about the UFS Atmosphere physics namelist can be found with the CCPP Scientific Documentation at https://dtcenter.org/GMTB/v4.0/sci_doc/.