This comprehensive guide details WRF installation, configuration, and execution, utilizing WRF-MOSIT on 64-bit systems,
leveraging ERA5 data and the WRF-GHG user guide for optimal performance and accessibility for all users․
The Weather Research and Forecasting (WRF) Model is a next-generation mesoscale numerical weather prediction system designed to serve both atmospheric research and operational forecasting needs․ Developed jointly by the National Center for Atmospheric Research (NCAR) and NOAA, WRF simulates the atmosphere, offering advanced capabilities for modeling weather phenomena at various scales․

This guide focuses on installing and utilizing WRF, a powerful tool for researchers and professionals alike․ WRF’s flexibility allows for diverse applications, from short-range forecasting to long-term climate studies․ The WRF-MOSIT (Multi-Operating System Install Toolkit) simplifies the installation process across various platforms․ Understanding the core components – WRF itself and the WRF Preprocessing System (WPS) – is crucial for successful implementation․ This guide will navigate you through each step, ensuring a smooth setup and enabling you to harness the full potential of this sophisticated model․ Resources like UCAR/UCP MetEd and the WRF Online Tutorial further enhance learning․
Before embarking on WRF installation, ensuring your system meets the necessary requirements is paramount․ This guide primarily focuses on 64-bit systems, as WRF does not officially support 32-bit architectures․ A robust operating system is essential; compatibility details will be covered in a dedicated section․

Crucially, you’ll need a Fortran compiler – gfortran is a popular and freely available choice․ Additionally, several libraries are required, including those for netCDF, HDF5, and MPI (Message Passing Interface) for parallel processing․ The WRF-MOSIT script streamlines the installation of these dependencies․ Sufficient disk space is also vital, accounting for the WRF source code, WPS, and input data (like ERA5)․ Finally, familiarity with the Linux command line is highly recommended for navigating the installation and compilation processes effectively․
WRF’s hardware demands vary significantly based on the simulation’s scope and complexity․ For smaller test simulations, a modern multi-core processor (Intel or AMD) with at least 8GB of RAM is generally sufficient․ However, realistic regional or global simulations necessitate considerably more powerful hardware․
A high-performance computing (HPC) cluster with numerous cores and substantial memory (64GB or more) is recommended for production runs․ Fast storage, such as an SSD, will significantly reduce I/O bottlenecks during data processing and simulation․ The number of cores directly impacts the simulation’s speed; utilizing MPI for parallelization is crucial on multi-core systems․ Consider a dedicated GPU if you plan to explore advanced WRF configurations or utilize GPU acceleration features․
The Weather Research and Forecasting (WRF) model is primarily designed and supported for 64-bit operating systems․ This is due to the model’s substantial memory requirements and the need to handle large datasets efficiently․ Linux distributions (such as Ubuntu, CentOS, and Red Hat) are the most commonly used and well-supported platforms for WRF installations․
While WRF can be compiled and run on Windows, it typically requires the Windows Subsystem for Linux (WSL) to provide a Linux environment․ macOS compatibility is also possible, but may require more configuration and troubleshooting․ The WRF-MOSIT toolkit specifically targets 64-bit systems, streamlining the installation process across various Linux distributions․ Ensure your system architecture is 64-bit before proceeding with the installation․
Successful WRF compilation and execution necessitate specific compilers and libraries․ A Fortran compiler is crucial; gfortran is a popular and freely available option, often recommended for beginners․ Other compilers like Intel Fortran Compiler can also be used, potentially offering performance benefits․
Essential libraries include the NetCDF library (for handling data files), the MPI library (for parallel processing), and the Jasper library (for PNG support)․ The WRF-MOSIT script automates the installation of these dependencies on many systems․ Ensure these components are correctly installed and configured before initiating the WRF compilation process to avoid errors and ensure a smooth installation experience․
Accessing the WRF source code requires registration as a WRF user․ This is a mandatory step to comply with licensing agreements and ensure authorized access to the model’s latest developments․ Once registered, users can obtain the code through two primary methods: downloading directly from the WRF website or cloning the repository from GitHub․
Downloading provides a stable archive of the code at a specific point in time․ Cloning, however, allows for easy updates and access to the most recent revisions․ The WRF-MOSIT script can often automate the download or cloning process, simplifying the initial setup․ Ensure you download the correct version compatible with your system and desired features․

Before downloading or accessing the WRF source code, mandatory registration is required․ This process ensures compliance with licensing terms and grants access to the latest model updates and support resources․ The registration portal is accessible through the official WRF website, typically involving providing institutional details and agreeing to the usage agreement․
Registration unlocks access to the WRF download area and enables participation in the WRF community forums․ It’s a crucial first step for all new users․ Without registration, obtaining the source code is impossible․ The process is generally straightforward, but allow some time for account verification․ Registered users are then able to proceed with downloading or cloning the WRF source code․
Following successful registration, users can obtain the WRF source code via download or cloning from the official GitHub repository․ Downloading provides a compressed archive of the code, suitable for users unfamiliar with version control systems․ Cloning, utilizing Git, allows for tracking updates and contributing to the WRF development community․

The GitHub repository offers the most current version of WRF․ Cloning is recommended for experienced users, enabling easy synchronization with future releases․ Download links are also provided for convenience․ Ensure sufficient disk space is available before initiating the download or clone process․ Both methods provide access to the complete WRF source code, ready for compilation and customization․
WRF-MOSIT is a complete BASH script installation package designed for universal compatibility across any 64-bit system․ This toolkit streamlines the installation process for the Weather Research & Forecasting (WRF) model and related packages․ It simplifies the often-complex steps involved in setting up WRF, making it accessible to a wider range of users, regardless of their operating system or technical expertise․
WRF-MOSIT automates the download and compilation of necessary components, including WRF itself and the WPS preprocessing system․ It offers options for selecting compilers and libraries, tailoring the installation to specific hardware and software configurations․ This toolkit significantly reduces the potential for errors and ensures a consistent installation environment․
The WRF-MOSIT BASH script functions as a centralized control panel for installing WRF and its dependencies․ Upon execution, the script presents a menu-driven interface, guiding the user through the installation process․ This interface allows for customization, including the selection of desired WRF packages and compilation options․ The script handles downloading the necessary source code, configuring compilation settings, and initiating the build process․
Key features include automated dependency resolution, compiler selection (like gfortran), and options for parallel compilation (dmpar)․ It simplifies complex tasks like setting environment variables and linking libraries․ The script’s modular design allows for updates and additions, ensuring compatibility with newer WRF versions and operating systems․ It’s designed for ease of use, even for those unfamiliar with command-line interfaces․
To initiate the WRF installation, navigate to the directory containing the WRF-MOSIT BASH script within your terminal․ Ensure the script possesses executable permissions; if not, use the command chmod +x wrf-mosit․sh․ Execute the script by typing ․/wrf-mosit․sh and pressing Enter․ The script will then present an interactive menu, prompting you to select installation options․
Carefully review each prompt, choosing the appropriate settings for your system and desired WRF configuration․ The script will automatically download required components and manage the installation process․ Monitor the output for any errors or warnings․ Successful completion will result in a configured WRF environment, ready for compilation․ Detailed logging is provided for troubleshooting purposes․
Following the installation script, navigate to the WRF directory – typically /WRF․ Compilation is initiated using the ․/configure command․ This script detects your system’s configuration and creates a configure․wrf file․ Subsequently, use ․/compile em_real for a standard build, or ․/compile dmpar for a distributed-memory parallel build․
The compilation process can take considerable time, depending on your hardware․ Monitor the output for errors․ Common issues involve missing compilers or libraries․ If errors occur, consult the troubleshooting documentation or online forums․ A successful compilation generates executable files within the main and dmpar directories, signifying a ready-to-run WRF model․
The configure․wrf file, generated by the ․/configure script, dictates compilation settings․ Key options include the compiler (gfortran is common), and parallelization method (dmpar for distributed memory)․ Carefully review this file before compiling․ For dmpar builds, ensure MPI libraries are correctly installed and linked․
Adjusting compiler flags can optimize performance for specific hardware․ The configure script attempts to auto-detect optimal settings, but manual adjustments may be necessary․ Consider options like optimization levels (e․g․, -O3) and vectorization flags․ Incorrect configurations can lead to compilation errors or suboptimal model performance, so thorough testing is crucial․
After configuring, use ․/compile em_real to initiate compilation․ This process can take considerable time, depending on your system’s resources․ Monitor the output for errors․ Common issues include missing libraries, incorrect compiler settings, or insufficient memory․
If errors occur, carefully examine the error messages; Often, they indicate missing dependencies or configuration problems․ Re-run ․/configure with appropriate adjustments․ Consult the WRF documentation and online forums for solutions to common errors․ Ensure your environment is correctly set up with necessary paths and variables․ Successful compilation results in executable files within the main and share directories․
The WRF Preprocessing System (WPS) prepares meteorological data for WRF․ Download WPS from the WRF website and extract the archive․ Navigate to the WPS directory and run ․/configure, ensuring it’s compatible with your WRF build․ Then, execute make to compile WPS․
Proper configuration of WPS is crucial․ The geogrid․conf file defines the domain and resolution․ ungrib converts raw data into WPS-compatible format, and metgrid interpolates data onto the WRF grid․ Thoroughly review the WPS documentation for detailed instructions and troubleshooting tips․ Successful WPS setup is essential for accurate WRF simulations․

Obtain the WPS source code after registering as a WRF user․ Download the appropriate WPS version corresponding to your WRF build․ Extract the downloaded archive to your desired installation directory․ Navigate into the WPS directory using your terminal․
Initiate the compilation process by running the ․/configure script․ This script checks your system for necessary dependencies and prepares the build environment․ Following configuration, execute make to compile the WPS code․ Monitor the compilation output for any errors․ Successful compilation results in executable files within the WPS directory, ready for use in preprocessing meteorological data for WRF simulations․
The geogrid․exe program, part of the WPS, defines the model domain’s static geographical information․ Before execution, modify the namelist․wps file to specify the desired domain size, resolution, and projection parameters․ Crucially, define the start and end longitude/latitude coordinates, along with the grid spacing․
Run geogrid․exe to generate static grid files․ These files contain elevation data, landuse categories, and other geographical features․ Ensure the WPS correctly locates necessary data, such as static data from the USGS․ Proper geogrid configuration is fundamental for accurate WRF simulations, establishing the foundation for subsequent WPS steps and the WRF model itself․
WRF requires meteorological data for initial and boundary conditions, typically obtained from global datasets like Copernicus ERA5․ Access ERA5 data through the Copernicus Climate Data Store (CDS), requiring registration and understanding of data access policies․ Download necessary variables – temperature, wind, humidity, and geopotential height – in the appropriate format (e․g․, NetCDF)․
Preprocessing involves converting the downloaded data into WPS-compatible formats using WPS utilities․ This includes extracting relevant variables, regridding to the WRF domain, and ensuring data consistency․ Careful data acquisition and preparation are vital for accurate WRF simulations, directly impacting forecast quality and reliability․

Copernicus ERA5 provides comprehensive atmospheric data ideal for WRF initialization and boundary conditions․ However, successful integration requires a specific workflow․ Users often encounter challenges downloading and processing ERA5 data from the Copernicus Climate Data Store (CDS)․ A step-by-step guide is crucial for navigating the CDS interface, selecting appropriate variables, and defining the desired temporal resolution․
Post-download, data must be converted into a format compatible with the WRF Preprocessing System (WPS)․ This involves utilizing WPS tools to re-grid the ERA5 data onto the WRF model domain, ensuring spatial consistency․ Proper implementation of this process is essential for accurate and reliable WRF simulations․
Accessing ERA5 data begins with registering for a free account on the Copernicus Climate Data Store (CDS) website․ Once registered, navigate to the ERA5 dataset and carefully define your download parameters․ Key considerations include selecting the appropriate variables (temperature, wind, humidity, etc․) relevant to your WRF simulation․
Specify the desired time period, spatial resolution, and data format․ The CDS offers various formats; netCDF is commonly used with WRF․ Pay close attention to the data volume, as large downloads can take considerable time․ Utilize the CDS API for automated downloads, especially for frequent updates or extensive datasets․
After successful compilation of WRF and WPS, a test simulation validates the installation and configuration․ Begin by configuring the input files: namelist․wps controls WPS preprocessing, defining the domain and resolution, while namelist․input governs the WRF model itself, specifying physics options and simulation duration․

Submit the WRF job to your computing environment (local machine, cluster, or cloud)․ Monitor the job’s progress, checking for errors in the output logs․ A successful run produces WRF output files containing meteorological data․ Visualize the results using tools like NCL or GrADS to confirm the simulation’s functionality and identify any potential issues․

Proper configuration of namelist․wps and namelist․input is crucial for a successful WRF simulation․ namelist․wps defines the domain, resolution, and data sources for WPS preprocessing․ Key parameters include the start and end dates, map projection, and grid spacing․ Careful attention to these settings ensures accurate data preparation․
namelist․input controls the WRF model’s behavior․ This file specifies physics schemes (microphysics, cumulus, boundary layer), time step, and output frequency․ Experimentation with these parameters allows tailoring the simulation to specific research questions․ Thoroughly review each option to understand its impact on the results․
Once input files are configured, submitting the WRF job to a computing cluster is the next step․ This typically involves using a job scheduler (e․g․, PBS, Slurm) and a submission script specifying resource requirements like CPU cores, memory, and wall time․ Accurate resource allocation prevents job failures due to insufficient resources․
Monitoring the job’s progress is essential․ Check the scheduler’s queue to confirm the job has started and is running․ Examine output files for error messages or warnings․ Regularly reviewing logs helps identify and resolve issues promptly, ensuring a smooth and efficient simulation run․ Successful completion generates WRF output files for analysis․
The WRF-GHG community benefits from a dedicated user guide, accessible via DOI link, offering comprehensive documentation․ This resource, hosted by BIRA-IASB, details utilizing the WRF model with greenhouse gas considerations, crucial for climate change research and accurate atmospheric modeling․
Additional resources include UCAR/UCP MetEd’s NWP training courses, providing foundational knowledge; Tutorial presentations – both recorded and in ․pdf format – supplement learning․ The WRF Online Tutorial offers further guidance․ Engaging with the WRF community forum fosters collaborative problem-solving and knowledge sharing, ensuring users can maximize the model’s capabilities and stay updated on best practices․