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COTS, New Space, LEO Constellations

Irradiation test facilities for COTS EEE components

  • Posted by Alessandra Costantino
  • On November 18, 2019
  • 0

Part 1

RADIATION SPACE ENVIRONMENT

ionisingIonising 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 environmentSpace environment in solar system

Space weather 

  • Solar cycle (11years)
  • Magnetosphere 
  • Solar wind and solar flares

stadistics

 

Ionising radiation effects on EEE components

effects

Part 2

TID TESTING

Total ionising dose 

dose

 

TID – Co60 gamma ray irradiation 

tid

Part 3

SEE TESTING

Single Event Effects

single event effects

Beam energy and Linear energy transfer 

beam energy

SEE Testing to estimate cross section vs LET

see testing

SEE tests with heavy ions

see tests

 

Cyclotrons 

Cyclotrons

Cyclotrons

 

Heavy ion beams

beams

 

Range of heavy ions

ions

 

COTS EEE components

COTS EEE components

 

High energy beam

high energy

 

Very High energy beam

very high

 

Ultra High energy beam

ultra high

 

Very and Ultra high energy beams

very and ultra

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)
    • 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

board levelHigher 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

summary

  • Author
  • Recent Posts
Alessandra Costantino
Alessandra Costantino

Physic engineer working as consultant for ESA at ESTEC since 2011 on radiation effects testing.
Since 2013 is the focal point for the ESTEC Co60 facility, and ESA contact point for external irradiation test facilities.
Alessandra Costantino
Latest posts by Alessandra Costantino (see all)
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