A Monte Carlo simulation of the NOAA POES Medium Energy Proton and Electron Detector instrument

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On the storm‐time evolution of relativistic electron phase space density in Earth's outer radiation belt (2013, methodology): “The POES MEPED fluxes shown in this paper are from the >6.9 MeV proton channel, which responds to >1 MeV electrons throughout the outer radiation belt [Yando et al., 2011].”
Solar Forcing for CMIP6 (v3.1) (2016, methodology): “Improved calibration of the SEM-2 detectors has been undertaken by Yando et al. (2011) using modeling techniques contained in the GEANT-4 code to determine the detector geometric conversion factor, or detector efficiency (following the original work described in Evans and Greer, 2000).”