edward daykin* abel diaz, cenobio ... - ohio state university
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WORK IN PROGRESSA Multiplexed Many-Point PDV (MPDV)
Techniques and Technologies
Edward Daykin*Abel Diaz, Cenobio Gallegos,
Carlos Perez, Araceli Rutkowski(* Daykinep@NV.DOE.GOV)
Presented to The 5th Annual PDV WorkshopThe Ohio State University
September 8, 2010
This work was done under Contract No. DE-AC52-06NA25946 with the U.S. Department of Energy.
DOE/NV/25946--1071
Motivation: Digitizer Cost & Availability of Digitizer Bandwidth and Memory
Digitizer MemoryTypical data lasts a few microseconds; digitizer memory allows record lengths ~ millisecond Time Multiplexing
Digitizer BandwidthTypical data uses a few gigahertz; digitizer bandwidth & sampling allow ~ 10 to 20 GHz Frequency MultiplexingAvailable Frequency Space
… please use me
2September 8, 2010
Inspiration: Bruce Marshall How to Complicate an Elegantly Simple Measurement without
Really Trying … PDV Workshop 2006
3September 8, 2010
• Wavelength division multiplexing– Lasers available on the ITU Grid?– Laser frequency ‘spacing’?– Application of Dense Wavelength Division Multiplexers (DWDMs)?
• Time division multiplexing– Coherence length and degree of polarization effects?
• Optical heterodyne approach: optical up-shift OR down-shift– Laser wavelength tunable?– Laser stable in frequency to ~ 10 MHz for hours?– Flexibility to up-shift for increased precision OR down-shift for
increased ‘effective’ bandwidth (e.g. high velocities)?
• A Laser Safe System– Optical pre-amplification on the ‘back end’ vs conventional high
power amplification on the ‘front end’?– Pre-amp gain saturation & dynamic hole burning affects?
Some Topics of Interest
4September 8, 2010
Evaluation of Photonic Technologies and Techniques
Seed Laser on ITU Grid
How can we leverage commercially available Telecom hardware?
5September 8, 2010
EDFA Optical Amplifier
DWDM
RedfernIntegratedOptics Inc.“RIO ORION”www.rio-inc.com
Wavelength Division Multiplexing – Notional
DW
DM
Mu
x
P
P
P
P
DW
DM
Mu
x
DW
DM
DeM
ux
Laser, ITU29Laser, ITU31Laser, ITU33Laser, ITU35
DW
DM
Probe 1-1Probe 1-2Probe 1-3Probe1-4
VariableOpticalAttenuators
F/O PowerMonitors
ToPhoto-Detector
6September 8, 2010
Seed Lasers: CW Power = 10 mWLinewidth = 15 kHz
ITU29 = 1554.13 nm (192900 GHz)ITU31 = 1552.52 nm ( 193100 GHz)ITU33 = 1550.92 nm (193300 GHz)ITU35 = 1549.32 nm (193500 GHz)
= 200 GHz
Wavelength Division Multiplexing with Optical Pre-Amplification – Notional
DW
DM
Mu
x
P
P
P
P
DW
DM
Mu
x
DW
DM
DeM
ux
Laser, ITU29Laser, ITU31Laser, ITU33Laser, ITU35
DW
DM
Probe 1-1Probe 1-2Probe 1-3Probe1-4
EDFA
ToPhoto-Detector
7September 8, 2010
Optical Pre-AmpErbium Doped Fiber Amplifier (EDFA)
Multiplexing, Pre-Amp & Optical Heterodyne
DW
DM
Mu
x
Laser, ITU29Laser, ITU31Laser, ITU33Laser, ITU35
DW
DM
Mu
x
P
P
P
P
DW
DM
Mu
x
DW
DM
DeM
ux
Laser, ITU29Laser, ITU31Laser, ITU33Laser, ITU35
DW
DM
Probe 1-1Probe 1-2Probe 1-3Probe1-4
EDFA 1x2
F/O CombinerToP-D
‘Local Oscillators’
8September 8, 2010
P
Temperature Tuned to User Determined Beat Frequency
Wavelength Division Multiplexing & Optical Heterodyne Up-Shifting … Lab Data
Laser Driven ‘Slapper Foil’ Triplexed Lab Data
9September 8, 2010
… and Time Division Multiplexing (~ 25 s)
10September 8, 2010
EDFA
Fiber-Optic Delay Line
DW
DM
DeM
ux
Laser Safe PDV: EDFA Pre-Amplification Benchmark Measurements
DW
DM
Mu
x
Laser, ITU29Laser, ITU31
DW
DM
Mu
x
P
P
DW
DM
DeM
ux
Laser, ITU29
Laser, ITU31
Probe 1
EDFA
1x2
F/O Combiners
ToP-D #1
‘Local Oscillators’
EDFA
Booster Amp125 mW
10 mW
Pre-AmpChannel
ITU29
ITU31
PRtn
ReferenceChannel
Compare Booster Amp ‘front end’ (prior to circulator) vs Pre-Amp ‘back end’ (post circulator)
11September 8, 2010
P
1x2ToP-D #2
September 8, 2010 Page 12
Benchmark Lab Data
‘Conventional’ PDV, No pre-amp : launch power = 125 mW, probe efficiency =14 dB, recorded onto digitizer channel 1
Laser Safe PDV, With EDFA pre-amp : launch power = 10 mW, probe efficiency range 14 dB to 60 dB, recorded onto digitizer channel 2
Laser Safe PDV: Benchmark Data
Pre-Amp Channel PRtn= -4 dBm
Reference ChannelPRtn= 7 dBm(Attenuated to match pre-amp power)
Pre-Amp Channel PRtn= -30 dBm
Pre-Amp Channels PRtn = -40 dBmPRtn = -50 dBm
13September 8, 2010
Optical power at photo-diode for Pre-Amp Channel & Reference Channel adjusted to be equal in all cases
• Multiplexing techniques promise increased PDV channel count, improved fidelity and improved cost effectiveness.
• Heterodyning is advantageous – allows user verification of beat signal amplitude (data quality assurance), flexibility to determine beat frequency (up/down shift), improves precision (see D. Dolan).
• Laser safe PDV operations via EDFA pre-amp appear feasible for probe efficiencies greater than ~ 40dB.
• Future Investigations:– Complete assembly of a 4x MPDV demonstration system for further testing on
high explosive experiments.– Investigate methods to ‘manage’ polarization dependence– Investigate methods to ‘gain clamp’ or ‘gain compress’ return signals to avoid
data loss upon saturation.
September 8, 2010 Page 14
Concluding Remarks & Future Investigations
September 8, 2010 Page 15
Acknowledgements
• Howard Bender, Program manager for NSTec SDRD Program
• Cenobio ‘Sonny’ Gallegos and his laser driven slapper laboratory
• Araceli Rutkowski et al. and her high frequency laboratory
• Carlos Perez and his perseverance with vendors and making it all work
• Many helpful discussions with Ted Strand (LLNL) and David Holtkamp (LANL)
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