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Weather Research and Forecasting Model

The Weather Research and Forecasting (WRF) Model is a next-generation mesoscale system designed for both atmospheric research and operational forecasting, supporting simulations across scales from tens of meters to thousands of kilometers using real or idealized initial conditions. It features the Advanced Research WRF (ARW) core as its primary dynamical core, which emphasizes higher-order accuracy and conservation properties; the Nonhydrostatic Mesoscale Model (NMM) core was previously available but is no longer supported by NCAR—along with a comprehensive suite of physics parameterizations for processes such as microphysics, , and land surface interactions, as well as an integrated system. The latest version, WRF 4.5, was released in 2023, with ongoing updates enhancing its capabilities. Developed collaboratively by the (NCAR), the (NOAA), the U.S. Air Force, the Naval Research Laboratory, the , and the , the model addresses limitations of earlier systems like the Fifth-Generation Mesoscale Model (MM5) and was publicly released in December 2000. WRF's software framework is built for and extensibility, allowing users to customize for diverse applications, including idealized studies, forecasting, regional modeling, and coupled system simulations. The preprocessing system, known as WPS, handles , , and input preparation from various observational and global model , facilitating seamless integration into operational workflows at centers like NOAA's (NCEP). Since its inception in the late , WRF has fostered a large international community, with over 57,000 user registrations from more than 160 countries as of 2021 and more than 12,000 peer-reviewed publications as of 2025, underscoring its role in advancing meteorological science, education, and commercial applications. Ongoing development efforts focus on enhancing physics schemes, leveraging for higher-resolution simulations, and expanding applications to areas like air quality, , and , ensuring WRF remains a cornerstone of modern atmospheric modeling. The model's open-source nature, supported by NCAR through workshops, documentation, and a user forum, promotes continuous community contributions and innovations.

Introduction

Overview and Purpose

The Weather Research and Forecasting (WRF) Model is a next-generation mesoscale (NWP) system designed to support atmospheric simulations across a wide range of scales, from tens of meters to thousands of kilometers. This flexibility enables its application in diverse meteorological contexts, including high-resolution regional forecasts and broader-scale studies. As a community-supported , WRF integrates modular components that allow users to configure simulations for specific research or operational needs. The primary objectives of WRF are to advance atmospheric research through both idealized simulations and real-data case studies, while also facilitating operational forecasting for prediction services worldwide. It serves as a tool for investigating atmospheric processes, testing hypotheses, and improving forecast accuracy in operational environments, such as national centers. By providing open-source access to its , WRF promotes collaboration among scientists and forecasters to refine modeling techniques. Initially released to the public in December 2000 as Version 1.0 through a collaborative effort involving the (NCAR) and partners, WRF has evolved into one of the most widely adopted NWP models globally. As of 2025, it boasts a large user community, with over 39,000 registered users across more than 160 countries, reflecting its broad impact on meteorological science and applications. The model features the Advanced Research WRF (ARW) as its primary dynamical core; the Nonhydrostatic Mesoscale Model (NMM) core was discontinued in version 4.4 (2022).

Development and Community

The development of the Weather Research and Forecasting (WRF) Model was initiated in the late 1990s as a collaborative effort among several key institutions, including the (NCAR), the (NOAA) through its (NCEP) and Earth System Research Laboratory (ESRL), the U.S. Air Force, the Naval Research Laboratory (NRL), the , and the (FAA). This partnership aimed to create a next-generation mesoscale model that could serve both research and operational forecasting needs, building on prior systems like the Penn State/NCAR Mesoscale Model (MM5) and the model. Leadership of the WRF project has been provided by NCAR's Mesoscale and Microscale (MMM) , which coordinates development, maintenance, and community engagement. Key milestones include the release of the first version (Version 1.0) in December 2000, which marked the model's debut as a freely available, open-source tool in the to encourage widespread adoption and contributions. Subsequent enhancements, such as the addition of nesting capabilities in (2004) and a global capability in Version 3.0 (2008), were supported by working groups from the original partners. The current version, 4.7, was released in April 2025. Annual WRF Users' Workshops, organized by NCAR and hosted in , began in 2000 and have continued each year, fostering collaboration and knowledge sharing among developers and users. The WRF community has expanded significantly, with NCAR providing ongoing support through online forums, tutorials, and documentation to assist users in model implementation and customization. As of 2025, the registered user base exceeds 39,000 individuals across more than 160 countries, reflecting its global adoption in academic, governmental, and private sectors. The Developmental Testbed Center (DTC), a joint facility involving NCAR, NOAA, and the U.S. , plays a crucial role in rigorous testing and evaluation of WRF configurations, ensuring reliability for research and operational transitions, such as its integration into NOAA's Rapid Refresh () and High-Resolution Rapid Refresh (HRRR) models.

Model Architecture

Dynamical Cores

The Weather Research and Forecasting (WRF) Model employs dynamical cores as the computational solvers responsible for advancing the atmospheric state through the integration of prognostic equations, enabling simulations of nonhydrostatic, compressible flows at various scales. These cores differ in their numerical frameworks, grid structures, and vertical coordinate systems, allowing flexibility for and operational applications. The model originally supported two primary cores: the Advanced Research WRF (ARW) and the Nonhydrostatic Mesoscale Model (NMM). The ARW core, developed by the (NCAR), implements a fully compressible, nonhydrostatic formulation on an Arakawa C-grid, which staggers mass and wind variables for improved and conservation properties. It utilizes a terrain-following, mass-based hybrid sigma-pressure vertical coordinate (default since version 3.9), facilitating high-resolution simulations with support for nested domains at refinement ratios of 3 or 5, two-way interactive nesting, and adaptive time-stepping options. This core's design emphasizes scalar conservation and high-order accuracy, making it suitable for a broad range of applications, including regional and global modeling, idealized cases, and integration with data assimilation systems like WRFDA. In contrast, the NMM core, derived from the Eta model and developed by the National Centers for Environmental Prediction (NCEP) with support from NOAA's Developmental Testbed Center (DTC), employs a nonhydrostatic solver on an Arakawa E-grid with a sigma-pressure hybrid vertical coordinate and rotated latitude-longitude projection. Optimized for operational mesoscale forecasting, it features step-mountain representation for terrain handling and was tailored for efficiency in high-resolution predictions, such as those in the Hurricane Weather Research and Forecasting (HWRF) system, though it offers less flexibility in domain configuration compared to ARW. Following the release of WRF version 4.4 in April 2022, the NMM core was removed from the main WRF distribution by NCAR (initially deprecated in version 4.0 in ), with a separate implementation continuing in specific operational contexts like HWRF; as of version 4.7 (April 2025), ARW is the sole actively maintained dynamical core for the broader WRF community.

Preprocessing and Postprocessing Systems

The Weather Research and Forecasting (WRF) model's preprocessing and postprocessing systems facilitate the preparation of input data and the analysis of simulation outputs, enabling accurate initialization and interpretation of results across various dynamical cores. The WRF Preprocessing System (WPS) serves as the primary tool for real-data simulations, handling the ingestion and interpolation of static and dynamic meteorological data to generate initial and boundary conditions compatible with the model's input requirements. WPS comprises three core programs: , ungrib, and metgrid. defines the model domains by interpolating static geographical , such as , land-use categories, and types, from predefined datasets at resolutions ranging from 30 arc seconds to 10 arc minutes onto user-specified grids. It uses a configuration file to specify domain parameters like , extent, and nesting ratios, producing intermediate files in the WRF I/O format (e.g., ) that include fields like . Ungrib extracts time-varying meteorological fields, such as , humidity, and wind components, from Edition 1 or 2 formatted datasets sourced from global models like GFS or ECMWF, outputting them in an intermediate format (default WPS) after vertical to levels. Metgrid then horizontally interpolates these meteorological fields onto the geogrid-defined domains, combining multiple sources if needed and generating final input files for the WRF real.exe program, with options for boundary-only processing to enhance efficiency. Postprocessing in WRF is exemplified by the ARW postprocessor (ARWpost), which converts model output files into visualization-friendly formats. ARWpost reads WRF-ARW history and restart files, along with WPS-derived and metgrid data, primarily in format, and computes diagnostic variables such as (CAPE) and radar reflectivity. Configured via a namelist.ARWpost file, it produces GrADS-compatible files (.dat and .ctl) for analysis and plotting, with support for GRIB1 inputs though less extensively tested; Vis5D output was discontinued after version 3.0. Data assimilation enhances preprocessing by integrating observational data into the initial conditions, primarily through the WRF Data Assimilation (WRFDA) system. WRFDA supports three-dimensional variational (3D-Var) methods, which minimize a using static background error covariances to assimilate observations like surface and data into a 3D . Four-dimensional variational (4D-Var) extends this by incorporating temporal evolution via the WRF forecast model over an assimilation window, enabling the use of asynchronous observations such as radiances and data. Ensemble-based approaches, including hybrid ensemble-variational techniques like 3DEnVar and 4DEnVar, leverage flow-dependent error statistics from forecasts to improve quality, with preprocessing tools like OBSPROC handling observation formatting in LITTLE_R and BUFR standards. These systems incorporate capabilities to support scalability on platforms. Geogrid and metgrid in WPS utilize (MPI) for distributed-memory parallelism, allowing domain decomposition across multiple processors. WRFDA employs both MPI for inter-processor communication in variational minimizations and for shared-memory threading within nodes, facilitating efficient handling of large datasets and ensemble generations. ARWpost, while primarily serial, can process outputs from parallel WRF runs without additional parallelization. This infrastructure ensures compatibility with the ARW dynamical core by adhering to the WRF I/O standards.

Physics and Parameterizations

Microphysics and Cumulus Schemes

The Weather Research and Forecasting (WRF) model incorporates microphysics schemes to explicitly resolve and processes within its grid, providing tendencies for heat, moisture, and non-convective rainfall rates. These schemes simulate the evolution of hydrometeors such as , , , , and , often using parameterization approaches that assume predefined size distributions for efficiency. Single-moment schemes predict only the mass mixing ratios of hydrometeor , while double-moment schemes additionally predict number concentrations for improved representation of variability and interactions. Key microphysics options in WRF include the Thompson scheme (mp_physics=8), a double-moment scheme that predicts and number concentrations for ice crystals and raindrops, with an aerosol-aware variant (mp_physics=28) incorporating prognostic effects for better simulation of - interactions in polluted environments. The WSM6 scheme (mp_physics=6) is a single-moment, six-class scheme that predicts mixing ratios for water, rain, , snow, , and vapor, offering computational efficiency suitable for operational forecasts while capturing mixed-phase processes. Another prominent option is the Lin et al. scheme (mp_physics=2), a Kessler-type single-moment scheme derived from the Purdue Lin model, which includes detailed -phase processes and is particularly effective for high-resolution simulations of deep . These microphysics schemes rely on continuity equations for and hydrometeor , typically expressed as \frac{\partial q_v}{\partial t} + \nabla \cdot (q_v \mathbf{v}) = P - L, where q_v is the water vapor mixing ratio, \mathbf{v} is the wind , and P and L represent production and loss terms from phase changes, respectively; advection and terms are handled by the dynamical core. Cumulus parameterization schemes in WRF address subgrid-scale by representing vertical fluxes of , , and that cannot be resolved explicitly, particularly for deep and shallow convective clouds, thereby influencing large-scale circulation and patterns. These schemes employ mass-flux approaches, where updrafts and downdrafts transport air parcels based on (CAPE) triggers. Notable cumulus schemes include the Kain-Fritsch (cu_physics=1), a mass-flux that triggers deep and shallow via removal, incorporates downdraft effects, and offers optional feedback to the cloud radiative for improved diurnal cycle representation. The Grell-Freitas (cu_physics=3) is a multi-scale, scale-aware parameterization designed to smoothly transition from coarse to cloud-resolving resolutions, using multiple closure assumptions to handle both meso- and synoptic-scale without abrupt spin-up issues. The Tiedtke (cu_physics=6) employs a mass-flux framework with -based triggering for deep , includes organized for shallow clouds, and transports momentum to better simulate tropical disturbances. Selection of microphysics and cumulus schemes in WRF is resolution-dependent: cumulus parameterizations are generally required for grid spacings of 10 km or coarser to represent unresolved , but are typically disabled for grids finer than 3–4 km where explicit resolution of clouds is feasible, avoiding double-counting of convective . In the "gray zone" of 3–10 km resolutions, scale-aware schemes like Grell-Freitas or Multi-scale Kain-Fritsch are preferred to mitigate biases in rainfall forecasts. These choices significantly impact rainfall predictions, with double-moment microphysics often improving quantitative forecasts in convective events by better capturing hydrometeor diversity, while cumulus schemes like Kain-Fritsch enhance timing and intensity of organized storms. Microphysics and cumulus schemes interact with parameterizations to modulate vertical mixing of , influencing overall convective initiation.

Boundary Layer and Radiation Parameterizations

The (PBL) parameterizations in the Weather Research and Forecasting (WRF) model simulate vertical mixing processes near the Earth's surface, which are essential for accurately representing , , and fluxes in the atmosphere. These schemes address subgrid-scale that cannot be resolved by the model's dynamical , influencing near-surface winds, profiles, and pollutant . WRF offers several PBL options, each employing distinct approaches to assumptions for turbulent . The (YSU) scheme is a first-order nonlocal closure model that incorporates countergradient transport to account for convective mixing in unstable conditions and explicit processes at the PBL top. It uses a bulk to diagnose the PBL height and applies eddy diffusivities based on a mixing length , making it suitable for a wide range of synoptic conditions, including convective boundary layers. The YSU scheme has been widely adopted for operational forecasting due to its computational efficiency and performance in simulating low-level jets and daytime mixing. In contrast, the Mellor-Yamada-Nakanishi-Niino (MYNN) scheme is a higher-order turbulent (TKE)-based parameterization that predicts TKE evolution and employs an eddy-diffusivity mass-flux approach for both vertical and horizontal mixing. This scheme resolves local gradients more explicitly through level-2.5 closure assumptions, improving simulations of layers and nocturnal compared to simpler nonlocal schemes. MYNN is particularly effective in complex terrain and for coupling with urban canopy models, as it better captures anisotropic structures. The Bougeault-Lacarrère (BouLac) scheme provides a TKE-based local option, emphasizing a mixing length proportional to the distance between surface and inversion layers, which enhances representation of in stably stratified flows. Designed initially for mesoscale applications, it integrates well with building environment parameterization (BEP) for urban simulations, reducing biases in surface and fluxes in built environments. BouLac's formulation avoids excessive vertical mixing in stable conditions, leading to more realistic nocturnal depths. Land surface models in WRF provide the lower boundary conditions by simulating soil-vegetation-atmosphere interactions, including , dynamics, and surface fluxes that feed into PBL schemes. The Noah-Multiparameterization (Noah-MP) model extends the original Noah LSM with multiple options for key processes such as canopy , snow , and , enabling flexible representation of and frozen soil effects. Noah-MP uses four soil layers and incorporates dynamic parameters, improving simulations of seasonal snow cover and fluxes in diverse ecosystems like forests and croplands. Its multi-physics framework allows users to select configurations for specific climates, enhancing accuracy in energy and water budget closure. The Rapid Update Cycle (RUC) land surface model emphasizes high-resolution and temperature predictions with nine vertical layers, including a multilayer scheme for rapid updates in short-range forecasts. RUC accounts for fractional coverage and changes in , which is critical for events involving frozen surfaces, and it couples directly with PBL schemes to provide realistic and moisture fluxes. This model has been refined for operational use in NOAA's Rapid Refresh system, showing reduced biases in near-surface variables over arid and snowy regions. Radiation parameterizations in WRF compute and terrestrial radiative fluxes, influencing the model's budget through , , and processes. The Rapid Radiative Transfer Model for General Circulation Models (RRTMG) employs the correlated-k method to efficiently handle gaseous in both shortwave and longwave spectra, supporting cloud overlap assumptions like maximum-random for realistic . RRTMG includes treatments for aerosols and trace gases, making it robust for and air quality simulations, and it typically calls every few model time steps to balance accuracy and computational cost. Its implementation in WRF has demonstrated superior performance in capturing diurnal temperature cycles and surface insolation compared to older schemes. The radiation scheme, adapted from the CAM3 framework, integrates comprehensive longwave and shortwave parameterizations with diagnostic cloud properties derived from microphysics, emphasizing interactions with greenhouse gases and . uses a two-stream for and supports time-varying profiles, which enhances simulations of stratospheric-tropospheric and regional biases. It is favored for global-scale applications within WRF due to its consistency with broader earth system models. These parameterizations interact through the surface energy balance equation, which equates storage changes to net radiation minus turbulent fluxes and ground heat conduction: S = R - H - LE - G, where S is heat storage, R is net radiation, H is flux, LE is flux, and G is ground heat flux. In Noah-MP and RUC, this balance is solved iteratively to determine , providing boundary conditions for PBL and radiation schemes; a brief coupling with microphysics enables cloud-radiation feedbacks for improved and forecasts. Ongoing updates to WRF physics schemes continue to expand options and refine performance. As of WRF version 4.7 (released April 2025), new microphysics schemes include the UFS Double Moment (UDM; mp_physics=27) for double-moment cloud and rain processes with advected , and RCON (mp_physics=29) for improved warm-rain representation in the . Enhancements also feature updates to the MYNN eddy-diffusivity mass-flux (EDMF) PBL for better efficiency and stability corrections in the k-epsilon PBL option, along with minor fixes to Noah-MP for and mapping.

Numerical Methods

Governing Equations

The Weather Research and Forecasting (WRF) model's Advanced Research WRF (ARW) core solves a set of fully compressible, non-hydrostatic equations that govern atmospheric dynamics. These equations are formulated in a terrain-following coordinate system to accommodate complex topography, using a hybrid sigma-pressure vertical coordinate denoted as η. The η coordinate transitions smoothly from terrain-following levels near the surface to pressure levels aloft, defined as p_d = B(\eta)(p_s - p_t) + [\eta - B(\eta)](p_0 - p_t) + p_t, where p_d is the dry-air pressure perturbation, p_s is surface pressure, p_t is top pressure, p_0 is a reference pressure, and B(\eta) is a monotonic function ensuring the transition. This mass-based coordinate employs \mu_d = \partial p_d / \partial \eta as the prognostic variable for dry-air mass per unit area, enabling flux-form conservation properties. The core prognostic equations are expressed in flux form on an Arakawa C-grid in Cartesian or curvilinear coordinates, incorporating -scale factors m_x and m_y for projections. The prognostic variables are defined as U = \frac{\mu_d u}{m_y} and V = \frac{\mu_d v}{m_x}, where u and v are the components in coordinates (related to physical velocities via by angle \alpha between and grid y-axis). The equations for these variables are: \frac{\partial U}{\partial t} + m_x \left[ \frac{\partial (U u)}{\partial x} + \frac{\partial (V u)}{\partial y} \right] + \frac{\partial (\Omega u)}{\partial \eta} + \frac{m_x}{m_y} \left[ \mu_d \alpha \frac{\partial p}{\partial x} + \frac{\alpha}{\alpha_d} \frac{\partial p}{\partial \eta} \frac{\partial \phi}{\partial x} \right] = F_U \frac{\partial V}{\partial t} + m_y \left[ \frac{\partial (U v)}{\partial x} + \frac{\partial (V v)}{\partial y} \right] + \frac{m_y}{m_x} \frac{\partial (\Omega v)}{\partial \eta} + \frac{m_y}{m_x} \left[ \mu_d \alpha \frac{\partial p}{\partial y} + \frac{\alpha}{\alpha_d} \frac{\partial p}{\partial \eta} \frac{\partial \phi}{\partial y} \right] = F_V Here, \Omega is the vertical velocity in η-coordinates, p is perturbation pressure, \phi = gz is , \alpha = 1/\rho is , \alpha_d is the dry-air specific volume, and F_U, F_V include Coriolis, , and forcing terms. The vertical for the physical vertical velocity W is: \frac{\partial W}{\partial t} + \mathbf{U} \cdot \nabla W = -\frac{\partial \phi}{\partial z} - g \frac{\alpha - \alpha_d}{\alpha_d} + F_W where \mathbf{U} = (u, v, w) is the three-dimensional and F_W encompasses additional terms. The thermodynamic equation advances the moist potential \theta_m: \frac{\partial \Theta_m}{\partial t} + m_x m_y \left[ \frac{\partial (U \theta_m)}{\partial x} + \frac{\partial (V \theta_m)}{\partial y} \right] + m_y \frac{\partial (\Omega \theta_m)}{\partial \eta} = F_{\Theta_m} with \Theta_m = (\mu_d + \mu_w) \theta_m as the flux form, and F_{\Theta_m} representing heating sources. The for total density (dry plus water) is: \frac{\partial \mu_d}{\partial t} + m_x m_y \left[ \frac{\partial U}{\partial x} + \frac{\partial V}{\partial y} \right] + m_y \frac{\partial \Omega}{\partial \eta} = 0 where \mu_w accounts for water mass. For water vapor, the equation for the mixing ratio q_v (or total moisture Q_m) is: \frac{\partial Q_m}{\partial t} + m_x m_y \left[ \frac{\partial (U q_m)}{\partial x} + \frac{\partial (V q_m)}{\partial y} \right] + m_y \frac{\partial (\Omega q_m)}{\partial \eta} = F_{Q_m} with Q_m = (\mu_d + \mu_w) q_m in flux form, and F_{Q_m} including phase change and sources. These equations close with the equation of state for an : p = p_d + p_h = \rho R_d T_v, where T_v is , R_d is the dry-air , and p_h is hydrostatic base-state ; an exner form \Pi = (p / p_0)^\kappa (with \kappa = R_d / c_p) is often used for thermodynamic variables. An optional hydrostatic approximation simplifies the vertical momentum equation by assuming \partial p / \partial z = -\rho g, neglecting vertical acceleration terms, which reduces computational cost for large-scale simulations while maintaining non-hydrostatic horizontal dynamics. This formulation ensures and scalars in flux form, with the full set solved by the ARW dynamical core.

Discretization and Time Integration

The Weather Research and Forecasting (WRF) Model employs distinct numerical methods for discretizing its governing equations on a computational and advancing the in time, tailored to its dynamical cores. In the Advanced Research WRF (ARW) core, horizontal discretization utilizes an Arakawa C- staggering, where prognostic variables such as velocity components (u and v) are positioned at the faces of cells, while scalar variables like potential temperature and are centered within the cells. This staggered arrangement enhances the representation of divergent flows and reduces computational modes, with finite-difference approximations applied using 2nd- to 6th-order schemes for terms. The Nonhydrostatic Mesoscale Model (NMM) core (deprecated in WRF v4.4, 2022), in contrast, adopted an E- structure with co-located variables, which favored the simulation of rotational modes but required adjustments for divergent physics. Vertically, the ARW core implements a terrain-following hybrid sigma-pressure coordinate system, denoted as η, which transitions smoothly from sigma levels near the surface to pressure levels aloft, with the model top fixed at a constant pressure surface. This coordinate follows the terrain to resolve boundary layer processes accurately while minimizing distortions in the free atmosphere; however, to mitigate numerical errors from steeply sloping surfaces—such as Gibbs oscillations or artificial vertical velocities—smoothing techniques are applied during coordinate definition and grid generation. Vertical discretization uses finite differences on mass points, supporting stretched grids for enhanced resolution near the surface. As of WRF v4.4 (2022), the NMM core was removed, with ongoing developments enhancing the ARW core's numerical methods for higher resolutions and efficiency. Time integration in the ARW core relies on a third-order Runge-Kutta scheme, which advances prognostic variables in three sub-steps per large time step, providing low numerical damping for meteorological modes while treating acoustic waves semi-implicitly. This approach splits the integration into smaller time steps for fast-propagating acoustic and gravity waves, using a forward-backward method horizontally and an implicit scheme vertically to maintain stability. The NMM core (deprecated since 2022) employed a leapfrog scheme with a Robert-Asselin time filter to suppress computational modes, combined with second-order Adams-Bashforth steps for horizontal advection and Crank-Nicolson for vertical terms, though without explicit splitting for gravity waves. Diffusion and slower advection terms are integrated over the larger time step in the ARW core to balance computational efficiency and accuracy. Model stability is enforced through the Courant-Friedrichs-Lewy (CFL) condition, which restricts the time step to satisfy < / |u|{max} for horizontal advection, where is the grid spacing and |u|{max} is the maximum , ensuring that information does not propagate across more than one per step. For acoustic modes in the ARW, a stricter acoustic CFL applies to the small time step < / (2 c_s), with c_s the , typically limiting to around 17 seconds for a 10 km grid. Adaptive time-stepping options adjust dynamically based on domain-wide CFL criteria, preventing instabilities from evolving winds or vertical motions.

Applications

Operational Forecasting

The Weather Research and Forecasting (WRF) Model forms the foundation for several operational numerical weather prediction systems at the National Oceanic and Atmospheric Administration's (NOAA) National Centers for Environmental Prediction (NCEP), enabling routine high-resolution forecasts to support weather services across North America. These systems leverage WRF's flexibility in data assimilation and physics parameterizations to produce timely guidance for severe weather, aviation, and public safety applications. The Rapid Refresh (RAP) model, operational since May 2012, utilizes the WRF Advanced Research core (WRF-ARW) at a 13 km horizontal resolution over the North American domain, with hourly updates to provide short-range forecasts out to 18 hours. It incorporates frequent assimilation of and surface observations to initialize cycles, enhancing predictions of rapidly evolving weather patterns such as thunderstorms and fronts. Building on the RAP framework, the High-Resolution Rapid Refresh (HRRR) model operates at 3 km resolution since September 2014, delivering convection-allowing forecasts over the with hourly cycling and sub-hourly updates every 15 minutes. The HRRR, also based on WRF-ARW, excels in resolving mesoscale features like supercells and heavy , supporting nowcasting and short-term outlooks up to . The North American Mesoscale (NAM) Forecast System employs the WRF nonhydrostatic mesoscale core at 12 km resolution, with nested 3 km grids for high-resolution regional domains, and runs four times daily for forecasts extending to 84 hours. Operational as a key component of NCEP's suite, the NAM provides detailed guidance for mid-latitude weather systems, including winter storms and temperature extremes. In tropical cyclone forecasting, the Hurricane Weather Research and Forecasting (HWRF) model was operational at NCEP from the 2007 Atlantic hurricane season until October 2025, using a WRF-based configuration to predict storm tracks and intensity up to 126 hours in advance. The HWRF integrated vortex initialization and ensemble capabilities to improve accuracy for wind speeds, rainfall, and surge hazards associated with hurricanes. It was replaced by the Hurricane Analysis and Forecast System (HAFS), which uses the FV3 dynamical core. These WRF-driven operational models demand substantial computing power and are executed on NOAA's supercomputer, which provides over 55,000 CPU cores for of high-resolution grids and cycles. To address uncertainty, configurations are routinely generated, such as the NSSL-WRF with multiple members run on Jet, yielding probabilistic forecasts that quantify spread in track and intensity predictions. The WRF Preprocessing System (WPS) facilitates real-time ingestion of meteorological data for initializing these production runs.

Research and Specialized Simulations

The Weather Research and Forecasting (WRF) model is extensively utilized in idealized simulations to investigate fundamental atmospheric processes without reliance on real observational , enabling controlled experiments on phenomena such as -induced flows, hurricane , and initiation. For instance, idealized simulations, including wave cases, allow researchers to examine orographic influences on and using analytically defined initial conditions and terrain-following coordinates. Similarly, idealized setups simulate hurricane vortex evolution and intensification, often incorporating or gravity current initializations to study asymmetric and eyewall . initiation studies employ or test cases to explore organized development, with grid spacings as fine as 100 meters for large-eddy simulations () to resolve turbulent structures. These configurations, supported by the WRF's nonhydrostatic and hydrostatic balance options, facilitate sensitivity analyses of physics parameterizations in isolated environments. In real-data research, WRF drives investigations into complex environmental interactions, such as events, air quality dynamics, and , leveraging its high-resolution capabilities and integration with observational datasets. studies often focus on thunderstorms or extreme cases, where WRF assimilates data to model convective evolution and validate microphysics schemes during events like the 2016 UAE . Air quality research employs WRF to simulate pollutant transport and dispersion, particularly through scalar for chemistry constituents, as seen in multi-year simulations assessing urban emissions under varying meteorological conditions. applications use WRF to refine global model outputs for regional scales, such as over the , where nested grids improve forecasts by incorporating terrain and land-use effects from datasets like the (NCEP). These efforts highlight WRF's role in bridging coarse-resolution projections with localized impacts, emphasizing dynamical processes over statistical methods. WRF supports specialized field campaigns by integrating model outputs with in-situ and observations, enhancing process-level understanding of targeted weather phenomena. A prominent example is the Investigation of Microphysics and Precipitation for Atlantic Coast-Threatening Snowstorms (IMPACTS) campaign, conducted from 2020 to 2023, which used WRF to simulate East Coast winter cyclones and snowbands, assimilating , , and data to study snowstorm microphysics and dynamics during events like the February 7, 2020, New York snowstorm. This integration allows for high-resolution hindcasts that validate model physics against multi-scale observations, improving representations of structures in mid-latitude storms. Beyond operational contexts, WRF serves as a for academic and non-operational research, with thousands of peer-reviewed publications demonstrating its versatility as a tool for testing and parameterization development. Researchers frequently employ WRF for experiments on physics options, such as varying cumulus or schemes to assess their impacts on simulated or , often in idealized or real-case frameworks to isolate scheme interactions. Community workshops facilitate the dissemination of these findings, promoting collaborative advancements in model applications.

Variants and Extensions

Hurricane and Polar Variants

The Hurricane Weather Research and Forecasting (HWRF) model, a specialized variant of the WRF, was developed by NOAA's Atlantic Oceanographic and Meteorological Laboratory and became operational at the in 2007. It builds on the Advanced Research WRF (ARW) dynamical core with targeted adaptations for simulation. Key features include vortex initialization to accurately represent the initial storm structure using observational and storm-following moving nests that dynamically track the hurricane's path while maintaining high resolution in the inner core. These nests enable a multi-level grid system, with configurations evolving from outer domains of 18-27 km to 13.5 km resolution and inner nests refining to 2 km or finer, reaching 1.5 km by 2019, allowing detailed capture of eyewall dynamics and processes. HWRF has been used operationally by the for track and intensity forecasts extending up to 126 hours, supporting real-time guidance during the Atlantic and eastern Pacific hurricane seasons until its retirement in 2022 in favor of the Hurricane Analysis and Forecast System. The Polar WRF variant, released in 2009 by the Polar Meteorology Group at Ohio State University's Byrd Polar and Climate Research Center (with initial public availability in 2008), addresses the unique challenges of high-latitude environments through modifications to the standard WRF framework. Based on WRF version 3.1.1, it incorporates polar-optimized parameterizations, including enhancements to the land surface model for improved treatment of thermodynamics, such as variable fraction, thickness, snow depth, and to better simulate surface energy balance and heat transfer over ice-covered regions. Radiation schemes are adapted for the and conditions, with adjustments to longwave and shortwave processes to handle extreme solar angles and persistent low temperatures. These changes enhance model stability in cold climates by reducing common cold biases in near-surface temperatures and improving simulations of processes over and ice sheets. Polar WRF has been widely applied in and , powering systems like the Antarctic Mesoscale for daily forecasts at resolutions from 30 km down to sub-kilometer scales, with ongoing updates including version 4.5.1 released in September 2023. Both variants leverage WRF's flexible nesting capabilities for high-resolution enhancements, such as inner nests at 1-2 km to resolve fine-scale features like hurricane eyewalls or polar cyclones, which improve the representation of convective structures without excessive computational cost. In terms of performance, HWRF demonstrated notable improvements in the , achieving average track error reductions of about 20% compared to predecessor models like GFDL at various lead times, particularly through better vortex initialization and nest motion.

Coupled Model Systems

The Weather Research and Forecasting (WRF) model supports coupled systems that integrate atmospheric dynamics with other physical processes, enabling multi-physics simulations for enhanced forecasting of interconnected environmental phenomena. These couplings allow for two-way interactions, where meteorological fields influence and are influenced by additional components such as , , and surface processes. This modularity facilitates applications in air quality, water , and , with ongoing developments improving computational efficiency and process representation. WRF-Chem represents a key coupled system that integrates WRF's meteorological framework with modules to simulate air quality and transport. It enables online, two-way interactions between and , including effects on budgets and -cloud processes. Common configurations incorporate gas-phase schemes like the Carbon Bond Mechanism Z (CBM-Z), which handles 73 species and 237 reactions, coupled with modules such as for simulating interactions among , , , carbon, black carbon, , and . The CBM-Z/ combination (chem_opt=8) is widely adopted for its balance of computational efficiency and accuracy in reconstructing concentrations and optical depths. WRF-Chem is extensively used for forecasting, such as and predictions, and has been applied in studies of climate- interactions, including and feedback on regional climate variability. WRF-Hydro extends WRF by coupling it with hydrological models to simulate terrestrial components, addressing and land surface interactions. It builds on the Noah-MP land surface model for processes like dynamics and , incorporating routing schemes for overland flow, channel routing, and subsurface exchanges to represent watershed-scale . This supports multi-scale simulations of precipitation-runoff responses and land-atmosphere feedbacks, forming the core of operational systems like the NOAA National Water Model for forecasting. Applications include guidance, seasonal water resource assessments, and hydroclimate impact studies, with the system's parallelized architecture enabling high-resolution runs on diverse terrains. Extensions within the WRF framework, often referred to as WRF+ variants, incorporate specialized modules for urban and fire-related processes to enhance coupled simulations in complex environments. The urban canopy parameterization, including single-layer (SLUCM) and multi-layer (BEP/BEM) schemes, models , , and exchanges in built environments, capturing effects like urban heat islands on local . For fire weather, the WRF-Fire module provides two-way coupling between atmospheric conditions and wildland fire spread, simulating fuel consumption, release, and plume dynamics to predict fire behavior and dispersion. These extensions are applied in studies and risk assessments, integrating with core WRF physics for realistic hazard forecasting. Advancements in WRF version 4.5, released in April 2023, include improved support for building coupled systems via , streamlining compilation for components like WRF-Chem and WRF- on modern platforms, with further updates in versions up to 4.7.1 as of June 2025. This version updates the hydro interface to align with WRF- v5.3.0 and Noah-MP v4.5, enhancing interoperability for coupled runs. Such developments support broader applications, including research campaigns that leverage these systems for integrated .

Evaluation and Limitations

Validation and Performance

The accuracy of the Weather Research and Forecasting (WRF) model is evaluated using standard meteorological verification metrics, including error (RMSE) for surface and forecasts, scores to assess systematic over- or under-predictions, and equitable threat scores () for categorical events such as heavy rainfall or severe storms. For instance, in simulations over complex terrain, WRF's 2-m RMSE typically ranges from 1.5 to 2.5°C for 24-hour forecasts, while often shows slight overestimation in convective regimes, with ETS values exceeding 0.4 for moderate rainfall thresholds in mid-latitude cases. These metrics are computed against observational networks like surface stations and data to quantify across lead times. Annual WRF Users' Workshops, hosted by the (NCAR), feature dedicated sessions on model evaluation where successive versions are tested against real-world cases, including idealized benchmarks and operational hindcasts. For example, version 4.0, released in 2018, incorporated enhanced scale-aware cumulus parameterizations such as the Multi-scale Kain-Fritsch scheme, leading to improved representation of convective processes in high-resolution simulations compared to prior versions. These evaluations often highlight gains in precipitation timing and intensity, with workshop presentations demonstrating reduced errors in mesoscale convective systems through updated physics suites. Comparisons with predecessor models show WRF outperforming the Fifth-Generation Mesoscale Model (MM5) in key areas, such as 36-km resolution forecasts of and , where WRF exhibits lower RMSE and higher skill scores due to advanced nonhydrostatic dynamics and physics options. Against global models like the European Centre for Medium-Range Weather Forecasts (ECMWF) Integrated Forecasting System, WRF benchmarks favorably in mid-latitude regions for short-range , achieving superior spatial detail and reduced bias in convective events within nested domains. WRF's global verifications confirm its adoption by a large exceeding 39,000 registered users across over 160 countries as of 2025, supporting operational and applications worldwide. The model demonstrates high skill in mesoscale forecasts spanning 1 to 48 hours, particularly for regional phenomena, with equitable skill scores often surpassing 0.5 for and predictions in real-time evaluations.

Known Challenges and Improvements

The Weather Research and Forecasting (WRF) model has been noted for its tendency to overpredict the intensity and duration of convective systems, such as lines, particularly in simulations of mesoscale convective systems where trailing stratiform regions are underrepresented or events persist longer than observed. This issue arises from challenges in representing microphysical processes and convective triggering, leading to biases in rainfall forecasts. Additionally, the model's outputs exhibit high to the selection of physics parameterizations, including cumulus, microphysics, and schemes, which can significantly alter simulated dynamics and patterns across different environmental conditions. High-resolution configurations, essential for capturing fine-scale features, incur substantial computational costs due to the need for extensive grid nesting and , limiting operational feasibility over large domains. In regions with complex , such as mountainous areas, the standard WRF configuration often struggles with accurate representation of orographic influences on and precipitation, resulting in errors in surface winds and processes unless specialized variants are employed. Similarly, polar simulations without dedicated variants like Polar WRF exhibit limitations in handling stable layers and ice-related physics, leading to biases in and over high-latitude environments. in WRF also faces gaps in regions with sparse observations, such as oceanic or remote land areas, where the lack of in-situ measurements hinders effective initialization and error correction through techniques like 3DVAR or EnKF. To address these issues, WRF version 4.5, released in April 2023, introduced enhanced compiler support for architectures like ARM64 and AOCC, improving portability and performance on diverse platforms. It also incorporated improved testing capabilities in the configure system, facilitating more robust validation of model builds and physics options. Subsequent releases, including version 4.7.1 in 2025, have added performance enhancements such as refactored schemes for 10-15% speed-ups in simulations. as of 2025 has explored AI-hybrid approaches for postprocessing WRF outputs, including machine learning-based bias correction for variables like and near-surface temperatures in data-sparse scenarios. Looking ahead, efforts are underway to integrate WRF physics schemes into NOAA's Unified Forecast System (UFS), aiming to leverage WRF's mesoscale strengths for improved short-range predictions within a coupled system framework. The WRF community is also advancing machine learning-based parameterizations, such as emulators for cumulus convection and subgrid processes, to reduce sensitivity to traditional schemes and enable more stable long-term simulations.

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