High-power semiconductor lasers for in-situ sensing of atmospheric gases Carl Borgentun Microdevices laboratory (MDL), JPL/Caltech Copyright 2013 California.

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Presentation transcript:

High-power semiconductor lasers for in-situ sensing of atmospheric gases Carl Borgentun Microdevices laboratory (MDL), JPL/Caltech Copyright 2013 California Institute of Technology. Government sponsorship acknowledged.

Outline Background Laser design and fabrication Performance Next target Postdoc seminar – Carl Borgentun2

Background Postdoc seminar – Carl Borgentun3

Gas sensing Postdoc seminar – Carl Borgentun4 Earth science Planetary science Safety Credit: NASA

Credit: Richard W. Pogge, Ohio state university Absorption spectroscopy basics Credit: David Sayres, Harvard Postdoc seminar – Carl Borgentun5 state.edu/~pogge/Ast161/Unit5/atmos.html

Laser spectroscopy basics Laser Detector Gas 1980s Liquid helium-cooled lasers (1000kg) 1990s Liquid nitrogen-cooled lasers (70 kg) 2000s Thermoelectrically cooled lasers (0.1 kg) Postdoc seminar – Carl Borgentun6

Example application – Earth science Carnegie airborne observatory Credit: Carnegie institute of science Postdoc seminar – Carl Borgentun7 Earth science

Example application – Planetary science Mars polar lander Mars science laboratory Credit: NASA Postdoc seminar – Carl Borgentun8 Planetary science

Example application – Safety Carbon monoxide monitoring instrument Credit: NASA Postdoc seminar – Carl Borgentun9 Safety

Ozone depletion Chlorine compounds destroy ozone, but only at cold temperatures. Water vapor in the stratosphere increases the threshold temperature, at which ozone destruction can take place. Risk of thinner ozone layer not only at the poles, but also at lower latitudes where people, animals, and plants live Postdoc seminar – Carl Borgentun10 James G. Anderson et al., Science, 337 (6096), , Various explanations for high mixing ratios of water vapor, distinguishable by measuring water isotopologues.

Traditional absorption techniques are not sensitive enough for the simultaneous measurement of water and its less abundant isotopologues. Jim Anderson’s group at Harvard are developing a cavity- enhanced instrument. A high-power laser source at the right wavelength is needed. In this case: Right wavelength ~ 3777 cm-1 (2.65 µm) In this case: High-power > 10 mW Need for more sensitive instrument Credit: NASA; Jim Anderson, Harvard Postdoc seminar – Carl Borgentun11

Laser design and fabrication Postdoc seminar – Carl Borgentun12

Two criteria: Optical gain Cavity Laser crash course Postdoc seminar – Carl Borgentun13 Active medium Cavity Pumping Mirror Output beam

Molecular Beam Epitaxy Credit: JPL Postdoc seminar – Carl Borgentun14 Active region 215 nm 66 Å

Processing Postdoc seminar – Carl Borgentun15 Etch ridge Insulate and contact Etch grating

Single-mode emission Postdoc seminar – Carl Borgentun16 Wavelength [µm]

Grating Distributed feedback (DFB) laser using a Bragg grating => single-mode emission. Etched, i.e. non-metal => less loss. Laterally coupled => no epitaxial re- growth necessary. Credit: JPL Postdoc seminar – Carl Borgentun17 Wavelength [µm]

SEM pictures Credit: Cliff Frez Postdoc seminar – Carl Borgentun18

Coating, cleaving, and bonding Credit: Cliff Frez Postdoc seminar – Carl Borgentun19 Wavelength: 2.0 – 3.5 µm Wavelength: 2.0 – 3.5 µm

Performance Postdoc seminar – Carl Borgentun20

Power characteristics Output power at 35 10C, 600 mA. Still more than 20 30C, 600 mA. No sign of thermal roll-over. Dips in LI curves are due to absorption of ambient water (feature, not a bug!) Postdoc seminar – Carl Borgentun21

Spectral performance Wavelength is tunable by temperature and/or drive current Postdoc seminar – Carl Borgentun22

Reliability and life-time Reliability and life-time test: devices submitted to elevated drive currents and mount temperatures. Over 3000 hours of accumulated testing has been performed, without a single failure. Peak wavenumber stabilizes after hours. The change in peak wavenumber is less than 2 cm -1. The output power is not reduced Postdoc seminar – Carl Borgentun23

Lasers integrated into TO-3 packages. No significant degradation in performance noticed after packaging.Packaging Before After Postdoc seminar – Carl Borgentun24

Shape of output beam Divergent and highly elliptical, normal for edge-emitters. Divergence angles: ~ 110 and 40 degrees Postdoc seminar – Carl Borgentun25

Instrument aperture Collimating the beam Postdoc seminar – Carl Borgentun26 Laser Laser package

Package with internal lens TO-3 header TEC Tilted, coated, sapphire window Black housing Coated lens (XYZ active alignment) Precision spacer Laser Cu submount Postdoc seminar – Carl Borgentun27

Next target: CH Postdoc seminar – Carl Borgentun28

Initial results Postdoc seminar – Carl Borgentun29 Hit target wavelength (3058 cm-1). Increase in output power (6 mW vs 1.5 mW)

Summary Successfully delivered 2 laser modules emitting more than 10 mW at 3777 cm-1 to Harvard for water detection. Developing laser package complete with collimating optics. Initial results show promising outlook for future methane detection missions like TLS Postdoc seminar – Carl Borgentun30

Acknowledgements Supervisor: Siamak Forouhar Colleagues: Cliff Frez, Ryan Briggs, Mahmood Bagheri Postdoc seminar – Carl Borgentun31

Thanks for the attention! Postdoc seminar – Carl Borgentun32

High-power semiconductor lasers for in-situ sensing of atmospheric gases Carl Borgentun, Microdevices laboratory (MDL)