Results from the ESA SREM monitors and comparison with existing radiation belt models |
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Authors: | H.D.R. Evans, P. Bü hler, W. Hajdas, E.J. Daly, P. Nieminen,A. Mohammadzadeh |
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Affiliation: | aEuropean Space Agency, ESTEC, Postbus 299, Noordwijk, 2200 AG, The Netherlands;bRhea System SA, B-1348 Louvain-la-Neuve, Belgium;cPB, AT-1130, Vienna, Austria;dPaul Scherrer Institut, CH-5232 Villigen PSI, Switzerland |
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Abstract: | The Standard Radiation Environment Monitor (SREM) is a simple particle detector developed for wide application on ESA satellites. It measures high-energy protons and electrons of the space environment with a 20° angular resolution and limited spectral information. Of the ten SREMs that have been manufactured, four have so far flown. The first model on STRV-1c functioned well until an early spacecraft failure. The other three are on-board, the ESA spacecraft INTEGRAL, ROSETTA and PROBA-1. Another model is flying on GIOVE-B, launched in April 2008 with three L-2 science missions to follow: both Herschel and Planck in 2008, and GAIA in 2011). The diverse orbits of these spacecraft and the common calibration of the monitors provides a unique dataset covering a wide range of B-L* space, providing a direct comparison of the radiation levels in the belts at different locations, and the effects of geomagnetic shielding. Data from the PROBA/SREM and INTEGRAL/IREM are compared with existing radiation belt models. |
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Keywords: | Radiation monitor Radiation environment SREM Radiation belt model AE-8 AP-8 Solar proton events Magnetosphere |
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