High Energy Parametric Laser Source and Frequency-Comb-Based Wavelength Reference for CO2 and Water Vapor DIAL in the 2 mu m Region: Design and Pre-Development ExperimentationsShow others and affiliations
2021 (English)In: Atmosphere, E-ISSN 2073-4433, Vol. 12, no 3, article id 402
Article in journal (Refereed) Published
Abstract [en]
We present a differential absorption lidar (DIAL) laser transmitter concept designed around a Nested Cavity Optical Parametric Oscillator (NesCOPO) based Master Oscillator Power Amplifier (MOPA). The spectral bands are located around 2051 nm for CO2 probing and 1982 nm for (H2O)-O-16 and (HDO)-O-16 water vapor isotopes. This laser is aimed at being integrated into an airborne lidar, intended to demonstrate future spaceborne instrument characteristics: high-energy (several tens of mJ nanosecond pulses) and high optical frequency stability (less than a few hundreds of kHz long term drift). For integration and efficiency purposes, the proposed design is oriented toward the use of state-of-the-art high aperture periodically poled nonlinear materials. This approach is supported by numerical calculations and preliminary experimental validations, showing that it is possible to achieve energies in the 40-50 mJ range, reaching the requirement levels for spaceborne Integrated Path Differential Absorption (IPDA) measurements. We also propose a frequency referencing technique based on beat note measurement of the laser signal with a self-stabilized optical frequency comb, which is expected to enable frequency measurement precisions better than a few 100 kHz over tens of seconds integration time, and will then be used to feed the cavity locking of the NesCOPO.
Place, publisher, year, edition, pages
MDPI AG , 2021. Vol. 12, no 3, article id 402
Keywords [en]
lidar, CO2 sounding, water vapor, parametric laser, frequency comb
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-293143DOI: 10.3390/atmos12030402ISI: 000633310900001Scopus ID: 2-s2.0-85103466447OAI: oai:DiVA.org:kth-293143DiVA, id: diva2:1545871
Note
QC 20210420
2021-04-202021-04-202025-03-28Bibliographically approved