11 February 2000Genova (I)1 ESA Space Environment & Effects Analysis Section Space Radiation Environment P. Nieminen, ESA/ESTEC, The Netherlands Overview Solar cosmic rays Trapped particles in the Earth’s magnetosphere Cosmic Rays Other sources SREM on ESA missions Conclusions
11 February 2000Genova (I)2 Solar flare electrons, protons, and heavy ions Jovian electrons Solar flare neutrons and -rays Solar X-rays Galactic and extra-galactic cosmic rays Induced emission Neutrinos Trapped particles Anomalous cosmic rays
11 February 2000Genova (I)3 Solar cycles Sunspot number from 1750 Yohkoh SXT 1991 and 1995 ESA Space Environment & Effects Analysis Section
11 February 2000Genova (I)4 Solar proton/ion events Proton event on April -98 & ISO Star Tracker fake counts SOHO EIT New Mexico H image ESA Space Environment & Effects Analysis Section
11 February 2000Genova (I)5 SOHO LASCO instrument before the event... … and after. ESA Space Environment & Effects Analysis Section
11 February 2000Genova (I)6 Trapped particles The SAA ESA Space Environment & Effects Analysis Section
11 February 2000Genova (I)7 Trapped particles Electron spectra Proton spectra REM data ESA Space Environment & Effects Analysis Section
11 February 2000Genova (I)8 Cosmic rays In space, long-term data from various missions On ground, terrestrial source (cosmic ray showers): Neutron monitor network High-energy tail up to ~10 22 eV Peak at ~500 MeV Anomalous CR ESA Space Environment & Effects Analysis Section
11 February 2000Genova (I)9 “Exotic” sources Jovian electrons from Mercury to outer Solar System Solar neutrons (at 1 AU ~10 MeV and above) “Knee” at ~20 MeV ESA Space Environment & Effects Analysis Section
11 February 2000Genova (I)10 Standard Radiation Environment Monitor (SREM) ESA Space Environment & Effects Analysis Section Optimised Al-Ta “Sandwich structure”. Aluminum Tantalum Silicon (detectors) D1 D2 Trade-off: - Performance - Cost - Mass - Volume e- (p+) e- Simulation outcome: modularity (D3) - Electrons > 0.5 MeV - Protons > 10 MeV - Heavy ions qualitatively
11 February 2000Genova (I)11 ESA Space Environment & Effects Analysis Section FIRST INTEGRAL PROBA International Space Station Mars Express Missions with SREM... Rosetta
11 February 2000Genova (I)12 ESA Space Environment & Effects Analysis Section Conclusions Space radiation environment highly complex and dynamic From DNA damage point of view, heavy ions have priority; however other sources & secondary emissions also need to be considered ESA-sponsored work on several space-specific modules completed or underway; the toolkit has the required basic capabilities