Last Updated: 07/15/2024

UPOS Radiation Belt

Version: 1.0

Satellites in space are instrumental in providing surveillance, communication, and navigation capability. Geomagnetic disturbances, which are related to enhancements of MeV electron intensity at geostationary orbit, can hamper these operations and can cause malfunction or failure of satellites and their onboard sensors. Accurate prediction of daily-averaged MeV electron intensity at geostationary orbit can be used to monitor the daily dosage of these MeV electrons for geostationary satellites. A recent significant advance in predicting the daily averaged intensity of energetic electrons at geostationary orbit was reported by Li et al. (Geophys. Res. Lett., 28, 1887-1890, 2001) based solely on real-time solar wind parameters and a simple radial diffusion model. This model gives predictions 1-2 days in advance. This project has extended the work of Li et al. by improving the diffusion coefficient used and by providing predictions 27 days in advance.

Inputs

Near-real time ACE data including IMF, solar wind bulk speed and proton density.

Outputs

Predictions of daily averages of MeV electron fluxes at geostationary orbit 27 days in advance

Model is time-dependent.

Domains

  • Geospace
  • Magnetosphere / Inner Magnetosphere / RadiationBelt

Space Weather Impacts

  • Near-earth radiation and plasma environment (aerospace assets functionality)

Publication Policy

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