Contamination in electron observations of the silicon detector on board Cluster/RAPID/IES instrument in Earth's radiation belts and ring current

Since more than 15 years, the Cluster mission passes through Earth's radiation belts at least once every 2 days for several hours, measuring the electron intensity at energies from 30 to 400 keV. These data have previously been considered not usable due to contamination caused by penetrating en...

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Veröffentlicht in:Space Weather 2016-06, Vol.14 (6), p.449-462
Hauptverfasser: Kronberg, E. A., Rashev, M. V., Daly, P. W., Shprits, Y. Y., Turner, D. L., Drozdov, A., Dobynde, M., Kellerman, A. C., Fritz, T. A., Pierrard, V., Borremans, K., Klecker, B., Friedel, R.
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container_end_page 462
container_issue 6
container_start_page 449
container_title Space Weather
container_volume 14
creator Kronberg, E. A.
Rashev, M. V.
Daly, P. W.
Shprits, Y. Y.
Turner, D. L.
Drozdov, A.
Dobynde, M.
Kellerman, A. C.
Fritz, T. A.
Pierrard, V.
Borremans, K.
Klecker, B.
Friedel, R.
description Since more than 15 years, the Cluster mission passes through Earth's radiation belts at least once every 2 days for several hours, measuring the electron intensity at energies from 30 to 400 keV. These data have previously been considered not usable due to contamination caused by penetrating energetic particles (protons at >100 keV and electrons at >400 keV). In this study, we assess the level of distortion of energetic electron spectra from the Research with Adaptive Particle Imaging Detector (RAPID)/Imaging Electron Spectrometer (IES) detector, determining the efficiency of its shielding. We base our assessment on the analysis of experimental data and a radiation transport code (Geant4). In simulations, we use the incident particle energy distribution of the AE9/AP9 radiation belt models. We identify the Roederer L values, L⋆, and energy channels that should be used with caution: at 3≤L⋆≤4, all energy channels (40–400 keV) are contaminated by protons (≃230 to 630 keV and >600 MeV); at L⋆≃1 and 4–6, the energy channels at 95–400 keV are contaminated by high‐energy electrons (>400 keV). Comparison of the data with electron and proton observations from RBSP/MagEIS indicates that the subtraction of proton fluxes at energies ≃ 230–630 keV from the IES electron data adequately removes the proton contamination. We demonstrate the usefulness of the corrected data for scientific applications. Key Points IES data in the radiation belts contaminated by energetic protons and electrons Radiation belt regions and energies of contamination are identified Methods to correct the IES data are proposed
doi_str_mv 10.1002/2016SW001369
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In this study, we assess the level of distortion of energetic electron spectra from the Research with Adaptive Particle Imaging Detector (RAPID)/Imaging Electron Spectrometer (IES) detector, determining the efficiency of its shielding. We base our assessment on the analysis of experimental data and a radiation transport code (Geant4). In simulations, we use the incident particle energy distribution of the AE9/AP9 radiation belt models. We identify the Roederer L values, L⋆, and energy channels that should be used with caution: at 3≤L⋆≤4, all energy channels (40–400 keV) are contaminated by protons (≃230 to 630 keV and &gt;600 MeV); at L⋆≃1 and 4–6, the energy channels at 95–400 keV are contaminated by high‐energy electrons (&gt;400 keV). Comparison of the data with electron and proton observations from RBSP/MagEIS indicates that the subtraction of proton fluxes at energies ≃ 230–630 keV from the IES electron data adequately removes the proton contamination. 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These data have previously been considered not usable due to contamination caused by penetrating energetic particles (protons at &gt;100 keV and electrons at &gt;400 keV). In this study, we assess the level of distortion of energetic electron spectra from the Research with Adaptive Particle Imaging Detector (RAPID)/Imaging Electron Spectrometer (IES) detector, determining the efficiency of its shielding. We base our assessment on the analysis of experimental data and a radiation transport code (Geant4). In simulations, we use the incident particle energy distribution of the AE9/AP9 radiation belt models. We identify the Roederer L values, L⋆, and energy channels that should be used with caution: at 3≤L⋆≤4, all energy channels (40–400 keV) are contaminated by protons (≃230 to 630 keV and &gt;600 MeV); at L⋆≃1 and 4–6, the energy channels at 95–400 keV are contaminated by high‐energy electrons (&gt;400 keV). Comparison of the data with electron and proton observations from RBSP/MagEIS indicates that the subtraction of proton fluxes at energies ≃ 230–630 keV from the IES electron data adequately removes the proton contamination. We demonstrate the usefulness of the corrected data for scientific applications. 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Comparison of the data with electron and proton observations from RBSP/MagEIS indicates that the subtraction of proton fluxes at energies ≃ 230–630 keV from the IES electron data adequately removes the proton contamination. We demonstrate the usefulness of the corrected data for scientific applications. Key Points IES data in the radiation belts contaminated by energetic protons and electrons Radiation belt regions and energies of contamination are identified Methods to correct the IES data are proposed</abstract><cop>Washington</cop><pub>John Wiley &amp; Sons, Inc</pub><doi>10.1002/2016SW001369</doi><tpages>14</tpages><oa>free_for_read</oa></addata></record>
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source Wiley Online Library Journals Frontfile Complete; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals
subjects Assessments
Channels
Contamination
Detectors
Earth
Earth science
Electrons
Geophysics
Imaging
Radiation
Radiation belts
Scientific apparatus & instruments
silicon detector
Space weather
title Contamination in electron observations of the silicon detector on board Cluster/RAPID/IES instrument in Earth's radiation belts and ring current
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