1. Introduction

The Unified Forecast System (UFS) is a community-based, coupled, comprehensive Earth modeling system. It is designed to be the source system for NOAA’s operational numerical weather prediction applications while enabling research, development, and contribution opportunities for the broader weather enterprise. For more information about the UFS, visit the UFS Portal at https://ufscommunity.org/.

The UFS can be configured for multiple applications (see a complete list at https://ufscommunity.org/science/aboutapps/). The configuration described here is the UFS Short-Range Weather (SRW) Application, which targets predictions of atmospheric behavior on a limited spatial domain and on time scales from less than an hour out to several days. The SRW Application v1.0 release includes a prognostic atmospheric model, pre- and post-processing, and a community workflow for running the system end-to-end, which are documented within the User’s Guide and supported through a community forum. Future work will include expanding the capabilities of the application to include data assimilation (DA) and a verification package (e.g. METplus) as part of the workflow. This documentation provides an overview of the release components, a description of the supported capabilities, a quick start guide for running the application, and information on where to find more information and obtain support.

The SRW App v1.0.1 citation is as follows and should be used when presenting results based on research conducted with the App.

UFS Development Team. (2021, March 4). Unified Forecast System (UFS) Short-Range Weather (SRW) Application (Version v1.0.0). Zenodo. https://doi.org/10.5281/zenodo.4534994

1.1. Pre-processor Utilities and Initial Conditions

The SRW Application includes a number of pre-processing utilities to initialize and prepare the model for integration. For the limited area model (LAM), it is necessary to first generate a regional grid regional_esg_grid/make_hgrid along with orography orog and surface climatology sfc_climo_gen files on that grid. There are additional utilities included to handle the correct number of halo shave points and topography filtering filter_topo. The pre-processing software chgres_cube is used to convert the raw external model data into initial and lateral boundary condition files in netCDF format, needed as input to the FV3-LAM. Additional information about the UFS pre-processor utilities can be found in the UFS_UTILS User’s Guide.

The SRW Application can be initialized from a range of operational initial condition files. It is possible to initialize the model from GFS, NAM, RAP, and HRRR files in Gridded Binary v2 (GRIB2) format and GFS in NEMSIO format for past dates. Please note, for GFS data, dates prior to 1 January 2018 may work but are not guaranteed. Public archives of model data can be accessed through the National Centers for Environmental Information (NCEI) or through the NOAA Operational Model Archive and Distribution System (NOMADS). Raw external model data may be pre-staged on disk by the user.

1.2. Forecast Model

The prognostic atmospheric model in the UFS SRW Application is the Finite-Volume Cubed-Sphere (FV3) dynamical core configured with a Limited Area Model (LAM) capability [BAB+ed]. The dynamical core is the computational part of a model that solves the equations of fluid motion. A User’s Guide for the UFS Weather Model is here.

Supported model resolutions in this release include a 3-, 13-, and 25-km predefined Contiguous U.S. (CONUS) domain, all with 64 vertical levels. Preliminary tools for users to define their own domain are also available in the release with full, formal support of these tools to be provided in future releases. The Extended Schmidt Gnomonic (ESG) grid is used with the FV3-LAM, which features relatively uniform grid cells across the entirety of the domain. Additional information about the FV3 dynamical core can be found here and on the NOAA Geophysical Fluid Dynamics Laboratory website.

Interoperable atmospheric physics, along with the Noah Multi-parameterization (Noah MP) Land Surface Model options, are supported through the Common Community Physics Package (CCPP; described here). Atmospheric physics are a set of numerical methods describing small-scale processes such as clouds, turbulence, radiation, and their interactions. There are two physics options supported for the release. The first is an experimental physics suite being tested for use in the future operational implementation of the Rapid Refresh Forecast System (RRFS) planned for 2023-2024, and the second is an updated version of the physics suite used in the operational Global Forecast System (GFS) v15. A scientific description of the CCPP parameterizations and suites can be found in the CCPP Scientific Documentation, and CCPP technical aspects are described in the CCPP Technical Documentation. The model namelist has many settings beyond the physics options that can optimize various aspects of the model for use with each of the supported suites.

The SRW App supports the use of both GRIB2 and NEMSIO input data. The UFS Weather Model ingests initial and lateral boundary condition files produced by chgres_cube and outputs files in NetCDF format on a specific projection (e.g., Lambert Conformal) in the horizontal and model levels in the vertical.

1.3. Post-processor

The SRW Application is distributed with the Unified Post Processor (UPP) included in the workflow as a way to convert the NetCDF output on the native model grid to GRIB2 format on standard isobaric vertical coordinates. UPP can also be used to compute a variety of useful diagnostic fields, as described in the UPP user’s guide.

Output from UPP can be used with visualization, plotting, and verification packages, or for further downstream post-processing, e.g. statistical post-processing techniques.

1.4. Visualization Example

A Python script is provided to create basic visualization of the model output. The script is designed to output graphics in PNG format for 14 standard meteorological variables when using the pre-defined CONUS domain. In addition, a difference plotting script is included to visually compare two runs for the same domain and resolution. These scripts are provided only as an example for users familiar with Python, and may be used to do a visual check to verify that the application is producing reasonable results.

The scripts are available in the regional_workflow repository under ush/Python. Usage information and instructions are described in Chapter 10 and are also included at the top of the script.

1.5. Build System and Workflow

The SRW Application has a portable build system and a user-friendly, modular, and expandable workflow framework.

An umbrella CMake-based build system is used for building the components necessary for running the end-to-end SRW Application: the UFS Weather Model and the pre- and post-processing software. Additional libraries (NCEPLIBS-external and NCEPLIBS) necessary for the application are not included in the SRW Application build system, but are available pre-built on pre-configured platforms. There is a small set of system libraries and utilities that are assumed to be present on the target computer: the CMake build software, a Fortran, C, and C++ compiler, and MPI library.

Once built, the provided experiment generator script can be used to create a Rocoto-based workflow file that will run each task in the system (see Rocoto documentation) in the proper sequence. If Rocoto and/or a batch system is not present on the available platform, the individual components can be run in a stand-alone, command line fashion with provided run scripts. The generated namelist for the atmospheric model can be modified in order to vary settings such as forecast starting and ending dates, forecast length hours, the CCPP physics suite, integration time step, history file output frequency, and more. It also allows for configuration of other elements of the workflow; for example, whether to run some or all of the pre-processing, forecast model, and post-processing steps.

This SRW Application release has been tested on a variety of platforms widely used by researchers, such as the NOAA Research and Development High-Performance Computing Systems (RDHPCS), including Hera, Orion, and Jet; NOAA’s Weather and Climate Operational Supercomputing System (WCOSS); the National Center for Atmospheric Research (NCAR) Cheyenne system; NSSL’s HPC machine, Odin; the National Science Foundation Stampede2 system; and generic Linux and macOS systems using Intel and GNU compilers. Four levels of support have been defined for the SRW Application, including pre-configured (level 1), configurable (level 2), limited test platforms (level 3), and build only platforms (level 4). Each level is further described below.

For the selected computational platforms that have been pre-configured (level 1), all the required libraries for building the SRW Application are available in a central place. That means bundled libraries (NCEPLIBS) and third-party libraries (NCEPLIBS-external) have both been built. The SRW Application is expected to build and run out of the box on these pre-configured platforms and users can proceed directly to the using the workflow, as described in the Quick Start (Chapter 2).

A few additional computational platforms are considered configurable for the SRW Application release. Configurable platforms (level 2) are platforms where all of the required libraries for building the SRW Application are expected to install successfully, but are not available in a central place. Applications and models are expected to build and run once the required bundled libraries (NCEPLIBS) and third-party libraries (NCEPLIBS-external) are built.

Limited-Test (level 3) and Build-Only (level 4) computational platforms are those in which the developers have built the code but little or no pre-release testing has been conducted, respectively. A complete description of the levels of support, along with a list of preconfigured and configurable platforms can be found in the SRW Application wiki page.

1.6. User Support, Documentation, and Contributing Development

A forum-based, online support system with topical sections provides a centralized location for UFS users and developers to post questions and exchange information. The forum complements the formal, written documentation, summarized here for ease of use.

A list of available documentation is shown in Table 1.1.

Table 1.1 Centralized list of documentation



UFS SRW Application v1.0 User’s Guide


UFS_UTILS v2.0 User’s Guide


UFS Weather Model v2.0 User’s Guide


NCEPLIBS Documentation


NCEPLIBS-external Documentation


FV3 Documentation


CCPP Scientific Documentation


CCPP Technical Documentation


ESMF manual


Unified Post Processor


The UFS community is encouraged to contribute to the development effort of all related utilities, model code, and infrastructure. Issues can be posted in the GitHub repository for the SRW Application or the relevant subcomponent to report bugs or to announce upcoming contributions to the code base. For code to be accepted in the authoritative repositories, the code management rules of each component (described in the User’s Guides listed in Table 1.1 need to be followed.

1.7. Future Direction

Users can expect to see incremental improvements and additional capabilities in upcoming releases of the SRW Application to enhance research opportunities and support operational forecast implementations. Planned advancements include:

  • A more extensive set of supported developmental physics suites.

  • A larger number of pre-defined domains/resolutions and a fully supported capability to create a user-defined domain.

  • Inclusion of data assimilation, cycling, and ensemble capabilities.

  • A verification package (i.e., METplus) integrated into the workflow.

  • Inclusion of stochastic perturbation techniques.

In addition to the above list, other improvements will be addressed in future releases.

1.8. How to Use This Document

This guide instructs both novice and experienced users on downloading, building and running the SRW Application. Please post questions in the UFS forum at https://forums.ufscommunity.org/.

Throughout the guide, this presentation style indicates shell
commands and options, code examples, etc.


Variables presented as AaBbCc123 in this document typically refer to variables in scripts, names of files and directories.


T.L. Black, J.A. Abeles, B.T. Blake, D. Jovic, E. Rogers, X. Zhang, E.A. Aligo, L.C. Dawson, Y. Lin, E. Strobach, P.C. Shafran, and J.R. Carley. A limited area modeling capability for the finite-volume cubed-sphere (fv3) dynamical core. Monthly Weather Review, Submitted.