Last Updated: 03/20/2023
iPATH
Version: 2Physics-based SEP Forecasting model
Inputs
- Background solar wind parameters, 2) CME parameters (speed, width, duration etc.) 3) Suprathermal seed population density/spectral index
Outputs
Time intensity profile and event-integrated spectra for protons, O, and Fe
Model is time-dependant.
Domains
- Heliosphere / Inner Heliosphere
Space Weather Impacts
- Near-earth radiation and plasma environment (aerospace assets functionality)
- Solar energetic particles - SEPs (human exploration, aviation safety, aerospace assets functionality)
Phenomena
- Solar Energetic Particles
Publications
Code
Code Languages: Fortran
Contacts
- Gary Zank, UAH (Model Developer)
- Zheyi Ding, UAH (Model Developer)
- Junxiang Hu, University of Alabama Huntsville (Model Developer)
- Gang Li, University of Alabama Huntsville (Model Developer)
- M Leila Mays, NASA GSFC CCMC (CCMC Model Host)
Publication Policy
In addition to any model-specific policy, please refer to the General Publication Policy.