Last Updated: 06/13/2025

WSA-Enlil-at-SWPC

Version: 3

WSA-Enlil is a large-scale, physics-based numerical model of the inner heliosphere used by NOAA's Space Weather Prediction Center (SWPC) to provide 1-4 day advance forecasts of solar wind structures and Earth-directed coronal mass ejections (CMEs) that can cause geomagnetic storms. The model combines two sub-models:

  1. Wang-Sheeley-Arge (WSA): a semi-empirical near-Sun model that uses photospheric magnetic field observations (primarily from the GONG network) to generate global solar wind solutions in the solar corona.
  2. Enlil: a 3-D magnetohydrodynamic (MHD) numerical model that simulates the propagation of solar wind and CMEs through the inner heliosphere.
WSA provides input boundary conditions for Enlil, which then computes the quasi-steady ambient solar wind and transient CME disturbances propagating toward Earth and other locations such as STEREO spacecraft. The model predicts solar wind parameters including density, velocity, and magnetic field to assess potential impacts on geomagnetic storms, satellite drag, GPS navigation, power grids, and communications systems.

Caveats:

  • The accuracy of model outputs heavily depends on the quality of input magnetic maps and the characterization of CMEs.
  • The WSA-Enlil model represents CMEs as cone-shaped structures, which may not fully capture the complex, asymmetric nature of real CMEs.
  • The prediction horizon is limited by the spatial domain of the model and the inherent variability of the solar wind.
  • CME parameters are approximations derived from coronagraph observations and may not reflect the full complexity of CME structures.
  • Therefore, when interpreting model predictions, it is important to consider these input uncertainties and simplifications inherent in the modeling approach.

Inputs

Photospheric magnetic field synoptic maps from the GONG network, combined over one solar rotation, providing input for WSA. CME parameters derived from coronagraph imagery, including timing, location, direction, and speed, characterize CMEs injected into the modeled solar wind.

Outputs

Hourly and higher cadence predictions of solar wind plasma parameters (density, velocity, temperature) and magnetic field at multiple locations including Earth (L1) and spacecraft positions such as STEREO A. Outputs include 3-D solar wind structures, CME propagation, and time series of predicted solar wind conditions for forecast intervals typically around 3 to 5 days.

Model is time-dependent.

Change Log

SWPC WSA-Enlil Version 1.0

  • Date: December 13, 2011
  • Deployment: Initial implementation on NCEP’s Central Computing System
  • Components:
    • WSA v2.2 (driven by GONG mrbqs synoptic maps)
    • Enlil v2.6
SWPC WSA-Enlil Version 2.0
  • Date: May 28, 2019
  • Deployment: NCEP’s Weather and Climate Operational Supercomputing System (WCOSS)
  • Model Updates:
    • Enlil v2.6 → v2.9e
    • Ambient retuning: amb=a3b2 → amb=a8b1
SWPC WSA-Enlil Version 2.1
  • Date: December 9, 2019
  • Deployment: WCOSS
  • Model Updates:
    • Planetary ephemerides extended through end of 2030
SWPC WSA-Enlil Version 3.0
  • Date: April 4, 2023
  • Deployment: WCOSS2
  • Model Updates:
    • WSA v2.2 → WSA v5.4
    • Implemented zeropoint-corrected GONG mrzqs synoptic maps
    • Implemented run-on-demand capability for CME runs, retiring bi-hourly executions
    • Adopted single (00Z) daily ambient run
    • Changed data acquisition point from Earth to L1, replacing evo.earth.nc with evo.l1.nc

Domains

  • Solar
  • Heliosphere / Inner Heliosphere

Space Weather Impacts

  • Geomagnetically induced currents - GICs (electric power systems)
  • Ionosphere variability (navigation, communications)
  • Atmosphere variability (satellite/debris drag)
  • Near-earth radiation and plasma environment (aerospace assets functionality)
  • Solar energetic particles - SEPs (human exploration, aviation safety, aerospace assets functionality)

Phenomena

  • Solar Magnetic Field
  • Coronal Holes
  • Coronal Mass Ejections
  • Ambient Solar Wind
  • Stream Interaction Regions
  • Interplanetary Shocks
  • Coronal Mass Ejections Propagation
  • Coronal Mass Ejection Arrival

Publications

Code

Code Languages: Fortran (core model), IDL and Python (tools and visualization)

Contacts

Publication Policy

In addition to any model-specific policy, please refer to the General Publication Policy.