Fast Widely-Tunable CW Single Frequency 2-micron Laser Charley P. Hale and Sammy W. Henderson Beyond Photonics LLC 1650 Coal Creek Avenue, Ste. B Lafayette, CO 80026 Presented at: 18 th Coherent Laser Radar Conference Boulder, CO 26 June-1 July 2016
Outline Applications of Frequency-Stable and Tunable SLM Lasers SWIFT: Solid-State Single-Frequency cw Laser Design Overview Wavelength/Frequency Tuning of SWIFT Frequency Stability of SWIFT Prototype Summary 1
Applications: Global Wind Monitoring Application Eyesafe Doppler lidar continues to be of great interest for global characterization of the winds from space Problem System efficiency is critical Doppler shifts from space platforms exceed COTS high efficiency 2 um detector bandwidths Typical high QE extended wavelength InGaAs BW = 500 MHz Typical platform velocities demand +/- 7 GHz Solutions Improved detector/receiver bandwidth High risk detector development Expensive RF electronics with higher noise figure Offset locked frequency MO/LO lasers Complex optical servo Fast slew rate and settling time 2
Applications: Differential Absorption Lidar (DIAL) Application CO2 concentration monitoring Global warming on Problem Need frequency agile Laser to probe on and off absorption wavelengths Or to tune through absorption features Solution Offset-locked frequency agile cw local oscillator laser 3
SWIFT cw SLM Laser Tm,Ho:YLF: 2047-2059 nm factory-set peak wavelength; user-tunable ± 0.14 nm. Other NIR and SWIR wavelengths possible Integral 60 db Faraday isolation and PM fiber coupling CW single-frequency output power in excess of 30 mw; higher powers possible. Very compact laser head: 1.2 W x 2.8 L x 1 H; conduction cooled; smaller version under development Fast piezo frequency tuning (>20 GHz); also capable of thermal tuning Linewidth less than 10 khz/ms (dependent on piezo drive characteristics) Long-term frequency drift less than 1 GHz/day. Improved linewidth and long-term frequency stability possible by locking to an external reference. 4
MLM Output Power (mw) SLM Output Power (mw) SWIFT cw Diode-Pumped Output Power SWIFT prototype uses 6% Tm, 0.5% Ho-doped YLF, 1 mm length, pumped at 780 nm with < 2 W; SLM operation via thin intracavity etalon Very short crystal length limits pump absorption but permits extremely short cavity length/wide FSR (61 GHz in prototype); longer crystals for applications requiring less tuning range will be more efficient 350 300 250 200 SWIFT MLM Pump in/power Out ResT 7.1/5.5C Set/Act ResT 17.0/16.5C Set/Act ResT 25.0/25.3C Set/Act ResT 30.1/30.9C Set/Act 100 90 80 70 60 50 OC/PZT fully clamped 75 VDC PZT bias 15degC Res Set T SLM throughout, ~ 2050.7 nm SWIFT SLM Output Power 150 40 100 30 20 50 10 0 0 200 400 600 800 1000 1200 1400 1600 1800 Diode Pump Power Incident on Rod (mw) 0 200 400 600 800 1000 1200 1400 1600 1800 Pump Power Incident on Laser Rod (mw) 5
DIAL Detector Intensity (mv) PZT Tuning Example Tm:Ho:YLF for CO 2 Absorption Measurements CO2 Absorption feature measured with PZT tuned Tm,Ho:YLF Intracavity etalon coarse tuning to 2051 nm (2047-2059 nm possible) Thermal tuning to select e.g. 2050.95 absorption feature PZT tuning over absorption feature Direct detection measurements agree with FASCOD/HITRAN (320 ppm CO 2 ) 15 GHz Thermal PZT Tm,Ho:YLF Laser Etalon 30 25 FASCOD 20 Measurements 15 10 2050.9 2050.95 2051 2051.05 2051.1 Laser Wavelength (nm) 6
SLM Wavelength (nm) SWIFT Piezo Tunability SWIFT prototype cavity FSR is 61 GHz via very short crystal and reentrant output coupler design Very small, low-v PZT actuator scans cavity length across FSR resulting in as much as 50 GHz (0.7 nm) SLM mode-hop-free tuning range Piezo V: ~ 815 MHz/V; Resonator T: ~480 MHz/ºC; Pump I: ~ 7.5 MHz/mA SWIFT SLM Piezo Tuning 2051 2050.9 2050.8 2050.7 2050.6 2050.5 2050.4 (50 GHz) (815 MHz/V) 2050.3 35 45 55 65 75 85 95 SWIFT Piezo Bias Voltage (V DC) 7
SWIFT Piezo Tuning Bandwidth Ring PZT is mechanically loaded by output coupler and exhibits ~ 40 khz bandwidth, -20/+100 V; tuning ~ 800 MHz/V Small-signal (0.5 V p-p; 400 MHz p-p) 1 st resonance ~ 38 khz Sinusoidal PZT drive (Ch 1) produces laser frequency modulation (Ch 2); still well-behaved (minimal phase shift) at 35 khz drive frequency 2.5 khz drive 35 khz drive Ch 1 Ch 1 Ch 2 Ch 2 8
SWIFT Piezo Tuning Bandwidth Large signal (10 V p-p) @ 3 khz produces ~ 8 GHz Δν in 170 μs No phase delay up to ~ 10 khz sinusoidal drive frequency; didn t exceed due to PZT damage concerns Static 80 GHz Fabry-Perot interferometer used to assess broad laser slew rate; e.g., 0.9 V ΔV results in ~ 0.7 GHz/V sensitivity 9
SWIFT Prototype Frequency Stability SWIFT prototype head was not sealed and so was open to air currents, barometric pressure change, acoustic noise in lab Nominally linear slope of a static 1 GHz FSR F-P interferometer fringe was cross-calibrated: 0.63 khz/mv photodiode output; 100 μs captures Typical prototype stability ~ 60 khz p-p out of 10 14 Hz; expect ~ 5 khz/ms with fully sealed laser head 10
Summary Improvements continue in cw SLM MO/LO lasers for coherent winds, atmospheric DIAL; potential for next-gen gravitational wave det SWIFT laser developed under NASA Phase I SBIR funding extends performance at 2.05 μm; potential for extension to other wavelengths of interest (1, 1.5, 1.6, 2.0 μm) Basic design readily applicable to higher cw powers, Q-switched pulsed applications Product versions at 2.05 μm expected 2016/17 11
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