PreMevE Update: Forecasting Ultra-Relativistic Electrons Inside Earth's Outer Radiation Belt

Journal Article · 24 August 2021 · Space Weather

DOI: https://doi.org/10.1029/2021sw002773 · OSTI ID:1880491

Sinha, Saurabh  ^[1]; Chen, Yue  ^[2]; Lin, Youzuo  ^[2]; Pires de Lima, Rafael  ^[3]

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1. Los Alamos National Lab. (LANL), Los Alamos, NM (United States); Univ. of Oklahoma, Norman, OK (United States)
2. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
3. Geological Survey of Brazil, São Paulo (Brazil)

Energetic electrons inside Earth's Van Allen belts pose a major radiation threat to spaceborne electronics that often play vital roles in modern society. Ultra-relativistic electrons with energies greater than or equal to two megaelectron-volt (MeV) are of particular interest, and thus forecasting these ≥2 MeV electrons has a significant meaning to all space sectors. Here, we update the latest development of the predictive model for MeV electrons in the outer radiation belt. The new version, called PREdictive MEV Electron (PreMevE)-2E, forecasts ultra-relativistic electron flux distributions across the outer belt, with no need for in situ measurements of the trapped MeV electron population except at the geosynchronous orbit (GEO). Model inputs include precipitating electrons observed in low-Earthorbits by NOAA satellites, upstream solar wind speeds and densities from solar wind monitors, as well as ultra-relativistic electrons measured by one Los Alamos GEO satellite. We evaluated 32 supervised machine learning models that fall into four different classes of linear and neural network architectures, and successfully tested ensemble forecasting by using groups of top-performing models. All models are individually trained, validated, and tested by in situ electron data from NASA's Van Allen Probes mission. It is shown that the final ensemble model outperforms individual models at most L-shells, and this PreMevE-2E model can provide 25-h (~1-day) and 50-h (~2-day) forecasts with high mean performance efficiency and correlation values. Our results also suggest that this new model is dominated by nonlinear components at L-shells <~4 for ultra-relativistic electrons, different from the dominance of linear components for 1 MeV electrons as previously discovered.

• Research Organization: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
• Sponsoring Organization: National Aeronautics and Space Administration (NASA); USDOE National Nuclear Security Administration (NNSA)
• Grant/Contract Number: 89233218CNA000001
• OSTI ID: 1880491
• Report Number(s): LA-UR-21-22963
• Journal Information: Space Weather, Journal Name: Space Weather Journal Issue: 9 Vol. 19; ISSN 1542-7390
• Publisher: American Geophysical UnionCopyright Statement
• Country of Publication: United States
• Language: English