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Solar Cell Degradation due to Proton Belt Enhancements During Electric Orbit Raising to GEO

Lozinski, Alexander R. ORCID: https://orcid.org/0000-0002-6508-487X; Horne, Richard B. ORCID: https://orcid.org/0000-0002-0412-6407; Glauert, Sarah A. ORCID: https://orcid.org/0000-0003-0149-8608; Del Zanna, Giulio; Heynderickx, Daniel; Evans, Hugh D.R.. 2019 Solar Cell Degradation due to Proton Belt Enhancements During Electric Orbit Raising to GEO. Space Weather, 17 (7). 1059-1072. https://doi.org/10.1029/2019SW002213

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Abstract/Summary

The recent introduction of all‐electric propulsion on geosynchronous satellites enables lower‐cost access to space by replacing chemical propellant. However, the time period required to initially raise the satellite to geostationary orbit (GEO) is around 200 days. During this time the satellite can be exposed to dynamic increases in trapped flux which are challenging to model. To understand the potential penalty of this new technique in terms of radiation exposure, the influence of several key parameters on solar cell degradation during the electric orbit raising period has been investigated. This is achieved by calculating the accumulation of non‐ionising dose through time for a range of approaches. We demonstrate the changes in degradation caused by launching during a long‐lived (100s of days) enhancement in MeV trapped proton flux for three different electric orbit raising scenarios and three different thicknesses of coverglass. Results show that launching in an active environment can increase solar cell degradation due to trapped protons by ~5% before start of service compared with a quiet environment. The crucial energy range for such enhancements in proton flux is 3‐10MeV (depending on shielding). Further changes of a few percent can occur between different trajectories, or when a 50μm change in coverglass thickness is applied.

Item Type: Publication - Article
Digital Object Identifier (DOI): https://doi.org/10.1029/2019SW002213
Additional Keywords: Proton belt, Electron Orbit Raising, Solar cell degradation, Non-ionising dose, Solar energetic particle, Geostationary satellite
Date made live: 15 Jul 2019 11:45 +0 (UTC)
URI: https://nora.nerc.ac.uk/id/eprint/522730

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