Irradiation test facilities for COTS EEE components
- Posted by Alessandra Costantino
- On November 18, 2019
- 0
Part 1
RADIATION SPACE ENVIRONMENT
Ionising radiation in the space environment
- Radiation belts trapped by planets’ magnetospheres, consisting mostly of protons and electrons
- Particles originating from the activity of the Sun, which include also heavy ions
- And cosmic rays with very high energy
Space environment in solar system
Space weather
- Solar cycle (11years)
- Magnetosphere
- Solar wind and solar flares
Ionising radiation effects on EEE components
Part 2
TID TESTING
Total ionising dose
TID – Co60 gamma ray irradiation
Part 3
SEE TESTING
Single Event Effects
Beam energy and Linear energy transfer
SEE Testing to estimate cross section vs LET
SEE tests with heavy ions
Cyclotrons
Cyclotrons
Heavy ion beams
Range of heavy ions
COTS EEE components
High energy beam
Very High energy beam
Ultra High energy beam
Very and Ultra high energy beams
Limitations:
- Few facilities worldwide that provide such beam (requiring heavy ion synchrotron); beam time scarce and expensive
- High penetration linked to relatively low LET values; high LET values only reachable near Bragg peak
- Advantages:
- Energies closer to actual GCR space environment, therefore tests are potentially more representative (i.e. for cases in which LET is not an appropriate figure of merit)
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- High penetration: testing in air, at constant LET and with packaged components/boards (could be the “only” way of performing ion tests in 3D structures, complex packages, etc.)
Part 4
BOARD LEVEL SEE TESTING WITH PROTONS
Board level SEE testing with protons
Higher range (mm-cm), Lower LET
- Screening for destructive SEEs at board-level (eg the effectiveness of such protection to detect and mitigate against destructive SEEs)
- Identification of soft errors and potential proton induced events (e.g. SEFI) considerably affecting the spacecraft/instrument availability
Summary of test facilities
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