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Space Radiation Environment P. Nieminen, ESA/ESTEC, The Netherlands

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In space, long-term data from various missions ... Rosetta. 11 February 2000. Genova (I) 12. ESA Space Environment & Effects Analysis Section ... – PowerPoint PPT presentation

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Title: Space Radiation Environment P. Nieminen, ESA/ESTEC, The Netherlands


1
Space Radiation Environment P. Nieminen,
ESA/ESTEC, The Netherlands
  • Overview
  • Solar cosmic rays
  • Trapped particles in the Earths magnetosphere
  • Cosmic Rays
  • Other sources
  • SREM on ESA missions
  • Conclusions

ESA Space Environment Effects Analysis Section
2
Anomalous cosmic rays
Galactic and extra-galactic cosmic rays
Jovian electrons
Neutrinos
Solar X-rays
Trapped particles
Induced emission
Solar flare neutrons and g-rays
Solar flare electrons, protons, and heavy ions
3
Solar cycles
Sunspot number from 1750
Yohkoh SXT 1991 and 1995
ESA Space Environment Effects Analysis Section
4
Solar proton/ion events
SOHO EIT
New Mexico Ha image
Proton event on 20-23 April -98 ISO Star
Tracker fake counts
ESA Space Environment Effects Analysis Section
5
SOHO LASCO instrument before the event...
and after.
ESA Space Environment Effects Analysis Section
6
Trapped particles
The SAA
ESA Space Environment Effects Analysis Section
7
Trapped particles
Electron spectra
Proton spectra
REM data
ESA Space Environment Effects Analysis Section
8
Cosmic rays
Peak at 500 MeV
In space, long-term data from various missions
On ground, terrestrial source (cosmic ray
showers) Neutron monitor network
Anomalous CR
High-energy tail up to 1022 eV
ESA Space Environment Effects Analysis Section
9
Exotic sources
Jovian electrons from Mercury to outer Solar
System
Knee at 20 MeV
Solar neutrons (at 1 AU 10 MeV and above)
ESA Space Environment Effects Analysis Section
10
Standard Radiation Environment Monitor (SREM)
Aluminum
Tantalum
Silicon (detectors)
e-
Trade-off- Performance- Cost- Mass-
Volume
e-
(p)
D1
D2
Optimised Al-Ta Sandwich structure.
Simulation outcome modularity (D3)
- Electrons gt 0.5 MeV- Protons gt 10 MeV- Heavy
ions qualitatively
ESA Space Environment Effects Analysis Section
11
Missions with SREM...
ESA Space Environment Effects Analysis Section
12
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

ESA Space Environment Effects Analysis Section
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