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ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 1 ESA U
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Qualifying Photonics for the Space Environment
Iain McKenzie Trieste 20/02/2015
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 2 ESA U
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Qualifying Microphotonic Devices for Space
Vacuum • Outgassing • Contamination • Packaging
Mechanical • vibration • Pyro-shock
Space radiation • Displacement damage • TID • Charging due to interaction
with charged particles
Thermal • Large temperature
variations
15 years service life • No maintenance • Guarantee of end of life performance
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 3 ESA U
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NASA vs. Telcordia Test Requirements
Due to the usage of MIL-STD-883 in Telcordia specifications, the random
vibration environmental parameters and duration are of greater intensity
than is required for space flight launch vehicles.
Reliability of Optical Fiber Modulators for Space Flight Environments, M. Ott, et al, NASA Parts and Packaging Program Report,
Electronic Parts Project, IPPAQ Task Report, October 2002.
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 4 ESA U
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Radiation Effects on Fibre Optic Sensor Hardware
Induced attenuation in optical fibres
Refractive index change in glass (FBG shift)
Impact on fibre optic coating (FBG shift)
Displacement damage semiconductor laser (increased laser threshold,
decreased slope efficiency)
Displacement damage in detector (increased dark current, reduced
efficiency)
SEE – laser driver sensitivity
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 5 ESA U
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Other Parameters that Effect Darkening
Stress in the fibre
Photo bleaching
Photobleaching test for two Standard Telecom fiber samples (97 m)
on the same spool with low and high optical power coupled in the fibers
0
1
2
3
4
5
6
7
0 200 400 600 800 1000 1200
Accumulated dose [Gy]
Rad
iati
on
in
du
ced
att
en
uati
on
[d
B]
Low Power (1 uW)
High Power (~10 mW)
Average dose rate = 449 Gy/h
Total dose = 1000 Gy
Wavelength = 980 nm
Fibres outside
irradiation setup
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 6 ESA U
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Radiation Darkening of Optical Fibers
Radiation-induced attenuation in some COTS fiber samples (100 metres)
Average dose rate = 157 Gy/h, Total dose = 1000 Gy
0
1
2
3
4
5
6
7
8
9
10
11
12
0 200 400 600 800 1000 1200
Accumulated dose [Gy]
Ra
dia
tio
n-i
nd
uc
ed
att
en
ua
tio
n [
dB
]
Draka MaxCap 300 Radhard optimized
Draka MaxCap 300 Standard
Draka MaxCap 300 Radhard
INO 712A1
Telecom Standard
Telecom Radhard
fiber is not
irradiated in this
area,
time of recovery
= 60 minutes
Radiation-induced attenuation at 850 nm
performed at an average temperature of -17 °C
0
5
10
15
20
25
30
35
40
45
50
0 200 400 600 800 1000 1200
Accumulated dose [Gy]
Ra
dia
tio
n-i
nd
uc
ed
att
en
ua
tio
n [
dB
]
Draka MaxCap 300 Radhard Optimized
Telecom Standard
Draka MaxCap 300 Radhard Optimized(21 C)
Average dose rate = 429 Gy/h
Wavelength = 850 nm
Average dose rate = 429 Gy/h
Wavelength = 850 nm
Radiation-induced attenuation fits and extrapolations at 850 nm
of the Draka MaxCap 300 Radhard Optimized fiber
exposed to gamma radiations
0
1
2
3
4
5
6
7
8
9
0 100 200 300 400 500 600 700 800 900 1000
Accumulated dose [Gy]
Rad
iati
on
-in
du
ced
att
en
uati
on
[d
B]
452 Gy/h
157 Gy/h
452 Gy/h Fit
157 Gy/h Fit
20.4 Gy/h extrapolation
0.06 Gy/h extrapolation
Courtesy of INO And SpaceFibre Project
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 7 ESA U
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FBG Wavelength Shift Due to Radiation
Applications include laser wavelength stabilisation, filtering, and sensing
FBGs show a shift in peak wavelength with radiation due partly to change in n
Changes for 1Mrad are on the order of some 10s pm
Radiation hardness improves with good selection of fibre, FBG writing approach, annealing process (thermal and UV), even coating type.
Femto second laser writing approaches so better radiation hardness
CH 10
-0.005
0.000
0.005
0.010
0.015
0.020
0.025
0.030
0.035
0.040
0.045
0 50 100 150 200
Time, h
Pea
k S
hif
t, n
m .
T10-1 T10-2 T10-3
Results courtesy of SCK-CEN ESA contract.
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 8 ESA U
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Radiation Testing of SOI Devices
• Co-60 TID testing of SOI ring resonator devices
• Total dose 300kRad • 0.39 pm/kRad shift of
resonance peaks • Important to note that
~100pm/K is expected due to thermally induced refractive index changes.
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 9 ESA U
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Vacuum
Material Selection – Outgassing
Contamination (hermetic sealing)
Packaging and Mounting
Hermetic Sealing required for active optoelectronic components (lasers
and detectors) – problems with moisture in package.
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 10 ESA U
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SMOS Qualification Program
SMOS Mission (Soil Moisture and Ocean
Salinity) Payload Module:
Microwave Imaging Radiometer with
Aperture Synthesis (MIRAS)
COTS components used:
Modulight AlGaInAs 1300nm FP laser diodes,
Hamamatsu InGaAs PIN photodiodes,
Gooch and Housego Fiber Splitters
Gore FO Cable
Diamond AVIM connectors
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 11 ESA U
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Qualification Approach
Highest quality level for commercial off-the-shelf opto-
electronic components is according to Telcordia standard or
similar.
Subsea is a good starting point – very high reliability
requirements – 20 year life expectancy
Space qualified components usually not existing
A full qualification exercise as per ESCC specification not
feasible due to
- time and cost constraints
- industry is too fast moving
What to do?
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 12 ESA U
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Qualification Approach
Partial evaluation of 2 alternatives
Full qualification of 1 FL plus samples
• + costs are moderate (only one qualification)
• + risk of qualification failure low
• – impact on overall schedule is high as procurement has to be
performed for the samples and after successful evaluation for
the FL again
In order to reduce risk:
Evaluation phase with two possible COTS candidates for each
component (subjected to most critical tests, constructional
analysis, manufacturer assessment)
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 13 ESA U
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Evaluation Process
Procurement from two different suppliers
Detailed constructional analysis
Critical selection and performance tests – Standard evaluation tests
should be designed to stress components and reveal failure
mechanisms. Depending on schedule and budget this may not be
possible.
Visit and make assessment of supplier’s manufacturing procedures
Based on final assessment procure flight lot
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 14 ESA U
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Flight Lot Acceptance Testing (LAT)
Selection testing (Evaluation phase):
1. - vibration, shock
2. - thermal vacuum cycling
3. - radiation (gamma & proton)
4. - constructional analysis & manufacturer assessment
Flight lot screening / qualification
1. - extended burn-in
2. - acceptance thermal cycling
3. - measurement at high and low temperature
Flight lot acceptance testing
1. - thermal cycling, vibration, shock and radiation
2. - life test
3. - bending, fibre pull, mating, DPA
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 15 ESA U
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Lessons Learnt from SMOS Qual.
Most manufacturers are not willing to customise their process
for a small volume order.
Be fast, products change fast – telecom market.
Smaller manufacturers show greater interest and higher
flexibility to customise their manufacturing and/or disclose the
exact processing
Be very accurate in manufacturer assessment (which activities
are outsourced, how is the visibility)
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 16 ESA U
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Evaluation and Qualification of AVIM FO Connector
Project Scope:
Evaluate and qualify connector set AVIM
Document and write specifications for connector sets and assemblies
Qualify a patchcord patchcord=fiber+cable+connectors-set+assembly-
process
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 17 ESA U
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Evaluation Test Plan (ETP)
Purpose of an ETP is to test resistance limits to understand safety
factors and define Qualification values
Scope: Break things and doing FA look why and when Find the
extreme temperature and define Tmin and Tmax for the long term
tests and cycles.
Evaluate limit in vibration and shock
Evaluate survivability to special condition (dust, salt mist,..)
Configuration Tested:
PM fiber Fujikura SM.15-P-8/125-UV/UV-400 1550nm, acrylate
coating
Loose tube OD=1mm PEEK Victrex 450G
Pigtails configuration (two connectors assembled when tested)
.
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 18 ESA U
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Evaluation Test Plan
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 19 ESA U
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Temperature Step Stress
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 20 ESA U
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Random Vibration Step Stress
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 21 ESA U
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Shock Step Stress
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 22 ESA U
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Mating – Demating Test
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 23 ESA U
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Qualification Values
Temperature cycles 100 cycles
• AVIM -55°C to +125°C
• Mini-AVIM -55°C to +85°C
Vibration 35gRMS, 20..2000Hz
Shock 500g
Endurance 1000h at Tmax
Mating durability 100 mating-
demating
Torsion 3N
Static side load 0.2 N
Cable retention 5N
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 24 ESA U
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Qualification Test Plan
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 25 ESA U
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Rocked Defect Investigation
Strange failure mode on ISS fibers observed in 1999
ESA Presentation | Iain McKenzie | Trieste | 20/02/2015 | TEC-MME ESA ESTEC | Slide 26 ESA U
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Night lights from space
Thank you for your attention.