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Results from the ESA SREM monitors and comparison with existing radiation belt models
Authors:HDR Evans  P Bühler  W Hajdas  EJ Daly  P Nieminen  A Mohammadzadeh
Institution: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
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.
Keywords:Radiation monitor  Radiation environment  SREM  Radiation belt model  AE-8  AP-8  Solar proton events  Magnetosphere
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