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- W3089370918 abstract "<p>The Helios mission consisted of two almost identical spacecraft in highly elliptic orbits launched in 1974 (Helios A) and 1976 (Helios B). Until Parker Solar Probes first perihelion, Helios B was the first spacecraft to reach a distance of 0.29 AU to the Sun. One of its instruments is the Experiment 6 (E6) which was designed and built at the Christian-Albrechts-University Kiel in order to measure ions (protons up to iron) in the energy range of 1.3 MeV/nucleon up to several GeV/nucleon and electrons in the energy range from 0.3 to about 8 MeV. The instrument relies on the dE/dx-E and on the dE/dx-Cherenkov method for stopping and penetrating particles, respectively. Electrons are separated from ions by the signal in the first 100 &#181;m thick solid state detector. Any particle that does not trigger this detector is identified as an electron. Since the solid state detectors are not working perfectly, a significant part of protons is identified as electrons. Here, we present a new method to correct the electron measurements for the cross talk based on detailed instrument simulations.</p>" @default.
- W3089370918 created "2020-10-08" @default.
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- W3089370918 date "2020-03-23" @default.
- W3089370918 modified "2023-10-14" @default.
- W3089370918 title "GEANT 4 Simulation of the Helios E6 - Proton Contamination of Relativistic Electron Measurements" @default.
- W3089370918 doi "https://doi.org/10.5194/egusphere-egu2020-4911" @default.
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