Last Updated: 05/26/2022
iPATH
Version: V1.0Physics-based SEP Forecasting model
Inputs
- CME width, 2) CME speed, 3) CME duration
Outputs
time intensity profile and event-integrated spectra for proton, 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)
Publications
- Modeling Particle Acceleration and Transport at a 2-D CME-Driven Shock Modeling Particle Acceleration and Transport at a 2-D CME-Driven Shock
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.