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This document is subject to the controls of the Export Administration Regulations (EAR) and has been classified as EAR99 under U.S. Export Control laws and
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Fiber Raman Amplifier Development for Laser Absorption Spectroscopy
Measurements of Atmospheric Oxygen near 1.26 Micron
J. T. Dobler1, J. A. Nagel2, V. Temyanko2, T.
Zaccheo3, B. Karpowicz3, and M. Braun1
1ITT Geospatial Systems, Fort Wayne, IN 2TIPD, LLC & College of Optical Sciences, University of Arizona, Tucson, AZ
3Atmospheric and Environmental Research, Inc, Lexington, MA
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Overview
• Multifunctional Fiber-Laser Lidar (MFLL) overview
• Recent CO2 work
• Raman amplifier development
• Ground testing
• Preliminary results
• Current and future work
June 23, 2011 2
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Active Sensing of CO2 Emissions over Nights, Days and Seasons [ASCENDS]: A Multi-Functional Fiber Laser Lidar for Climate Variability and Atmosphere Composition
• Comprehensive Instrument Suite:
• CO2 Lidar
• O2 Lidar
• PN Laser Ranger
• Passive Temperature Sounder
• Passive CO Sensor
• Dedicated Payload
June 23, 2011 3
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CO2 EDU Instrument Overview
June 23, 2011 4
•Simultaneous transmit/receive of all wavelengths
•Software based digital lock-in separates channels
•Leverages highly reliable CW telecom laser components
•No free space optics allows for rugged design
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EDU Flight History
June 23, 2011 5
DC-8UC-12Lear-25ITT EDU
The CO2 EDU has been deployed in 10 flight campaigns
since May 2005; with more than 50 flights spanning 3
different aircraft. Flights have been conducted over
various land types and over water, during both day and
night operations. Recent results for the CO2 instrument
as compared to high precision in-situ data have shown
absolute comparisons to better the 0.5 ppm with
standard deviation of ~2ppm.
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Fiber Raman Amplifier Objectives
• Amplify a 50 kHz or greater modulated CW 1.26-1.27 µm seed
signal to Watt level average power (5 W goal)
• Simultaneously transmit online and offline wavelengths
• Design fibers to suppress stimulated Brillouin scattering (SBS)
to allow for narrow linewidth amplification
• Varying core diameter
• Reduce overlap between optical and acoustic modes
• Simple, efficient, and robust architecture
June 23, 2011 6
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First Generation Fiber Raman Amplifier
7
Galeener, et. al., Apl. Phys. Lett.,
32, 34, 1978.
Nagel, et. al., IEEE Photon. Technol. Lett., 23, 585, 2011.
• Core variation broadens SBS spectrum by
50 MHz for ~3 dB SBS suppression
• 1.8 W average power achieved
• 2.4 W peak online (~30% optical efficiency)
• 0.58 W peak offline (~10% optical efficiency)
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First Amplifier and Test Setup
June 23, 2011 8
Data acquisition and control
done through integration
with ITT CO2 EDU
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After Integrating With the EDU Tests Were Performed at ITT’s Ground Test Facility
TX/RX
680 m
Path
Weather
TX/RX
680 m
Path
Weather
9
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AER’s End-to-End Analysis Software, Previously
Developed For the CO2 EDU was Updated to
Include O2
Ingest/Analysis
Interface
User-Defined Model Results
Web Interface to
Current/Historical
Weather Conditions
Interactive
Analyses
The data is fed into LBLRTM to generate values of optical depth for a given pressure, temperature, relative
humidity, and distance to target. The values for optical depth are computed in wavelength range of the
IPDA instrument, and values for online/offline optical depth are selected based upon the measured
wavelengths provided by the IPDA system. The difference between online and offline optical depths are
taken to compare with measurements of differential optical depth taken with the IPDA.
June 23, 2011 10
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Initial Testing Results First Gen Amplifier
June 23, 2011
y = 0.8898x - 0.0023R² = 0.9782
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45
Measu
red
Preliminary Model
Measured vs. Modeled Diff OD
y = -0.0001x + 0.9783R² = 0.9657
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0 500 1000 1500 2000 2500 3000
Measu
red
Dif
f T
ran
sm
issio
n
Range to Target [m]
• Measurements were made
over ranges from 600 m –
2.7 km
•The preliminary model
comparisons show good
correlation with the O2 IPDA
measurements
11
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Second Generation Fiber Raman Amplifier
• Reduced size by 2X
• Reduced weight by 40 lbs
• Reduced power by 110 VA
• Forward pumping produced 13.2 W peak
with 3 db bandwidth of <3 MHz, but out of
band ASE becomes significant @ ~10 dB
down
• Backward pumping produces clean
spectrum (>45 dB side-mode and ASE
suppression) but with output limited to
~ 3 W peak from the amplifier
• Implemented at 1262 nm to take advantage
of trough between two lines
• Clean modulation demonstrated for both
forward and backward pumping schemes
June 23, 2011 12
Forward Stimulated Raman Scattering Modulation After 170m Sinusoidally Varying Core Fiber at 38A Pump Current
0
0.05
0.1
0.15
0.2
0.25
0 5 10 15 20 25 30 35 40
Time (us)
Am
plitu
de (
V)
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Spectrum Forward vs. Backward Pumping
Forward Pumping
13.2 W peak, 3 dB
bandwidth ~3 MHzForward Stimulated Raman Scattering Spectrum for 200m First Generation Raman Fiber and 29W
Pump Power
-80
-75
-70
-65
-60
-55
-50
-45
-40
-35
-30
1260 1260.5 1261 1261.5 1262 1262.5 1263 1263.5 1264 1264.5 1265
Wavelength (nm)
dB
m
Backward Pumping
2.4 W peak, 3 dB
bandwidth ~2 MHz
Offline Forward Raman Spectrum at Full Pump Power (60A) from 40dB Tap
-80
-70
-60
-50
-40
-30
-20
1260 1260.5 1261 1261.5 1262 1262.5 1263 1263.5 1264 1264.5 1265
Wavelength (nm)
dB
m
June 23, 2011 13
Major loss for backward pumping is efficiency. Need longer fibers/more SBS suppression
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Initial Ground Measurements with 2nd
Generation Amplifier (Backward Pumping)
June 23, 2011 14
0.7
0.75
0.8
0.85
0.9
0.95
1
1.05
1262.49000 1262.50000 1262.51000 1262.52000 1262.53000 1262.54000 1262.55000 1262.56000 1262.57000 1262.58000
Dif
fere
nti
al T
ran
sm
iss
ion
Wavellength
Preliminary Stepped Sweep of O2 Absorption Feature vs Model Prediction for Target 680 m Away
Measured
model
Not calibrated for
Optical filter
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Ongoing Fiber Development
First fiber with acoustic
guiding layer had irregular
core shape and guided
significant light in the
inner cladding
Adjustments were made
to the heating elements
used to collapse the
MCVD tube which has
resulted in circular cores
on subsequent fibers
June 23, 2011 15
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Recent Work to Obtain Required SBS Suppression
Latest iterative fiber
design
Results from latest
preform
June 23, 2011 16
-60 -40 -20 0 20 40 60-8
-6
-4
-2
0
2
4
6x 10
-3
m
n
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Optical Mode
m
m
0 5 10 15
0
2
4
6
8
10
12
14
16-3.5
-3
-2.5
-2
-1.5
-1
-0.5
0
m
m
Acoustic Mode 1
0 5 10 15
0
2
4
6
8
10
12
14
16 -2
-1.8
-1.6
-1.4
-1.2
-1
-0.8
-0.6
-0.4
-0.2
0
m
m
Acoustic Mode 2 (Degenerate Mode)
0 5 10 15
0
2
4
6
8
10
12
14
16
-2
-1.5
-1
-0.5
0
0.5
m
m
Acoustic Mode 3 (Degenerate Mode)
0 2 4 6 8 10 12 14 16
0
2
4
6
8
10
12
14
16 -2
-1.5
-1
-0.5
0
0.5
1
1.5
2
2.5
3
m
m
Acoustic Mode 4 (Degenerate Mode)
0 5 10 15
0
2
4
6
8
10
12
14
16
-2
-1.5
-1
-0.5
0
0.5
1
1.5
2
2.5
3
Fiber Design Performance Modeling
June 23, 2011 17
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Packaging Amplifier for DC-8 Flights
• HP wave meter for
monitoring offline
wavelength
• Seed laser and modulation
box
• Bristol wave meter for
monitoring online
wavelength
• Polarization control
• Raman amplifier
• Pump Laser
June 23, 2011 18
Detector
is being
provided
by LaRC
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Current and Future Work
• Second generation amplifier is currently at ITT and is being
packaged into a DC-8 rack and integrated with the CO2 EDU
• Ground tests are being conducted over the next two weeks.
• Flight testing is planned for July and August on the NASA DC-
8 aircraft.
• New single mode fibers compatible for splicing with Hi-1060
fiber have been manufactured and are being evaluated for
their acoustic profiles and doping concentrations.
• We are currently pursuing funding to exploit the progress we
have made in the design and manufacture of acoustic guided
fibers for this wavelength. With plans to combine the varying
core diameter approach for maximum SBS suppression.
June 23, 2011 19
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Acknowledgements
• This work is supported by NASA, Earth Science Technology
Office (ESTO) under the Advanced Component Technology
Grant #NNGX09AD79G awarded to ITT Geospatial Systems.
• Additional collaborators:
• ITT – Doug McGregor, Mark Neal, Steve Horney
• TIPD, LLC, & College of Optical Sciences – Nasser
Peyghambarian and Robert Norwood
• AER – Hilary E. Snell
June 23, 2011 20