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Our lidar instruments are specifically designed for different platforms. We developed TELMA and CORAL as ground-based instruments. They are used as technology testbeds, miniaturizing the instruments and developing techniques for remote and autonomous control. They are portable and were used world-wide in extreme conditions. For a balloon-borne platform we developed BOLIDE - lightweight, small, inside a pressure vessel with remote control over limited satellite bandwidth and advanced telemetry options. ALIMA is designed to fit into an aircraft rack and be operated in this specific environment.
ALIMAThe Airborne Lidar for Middle Atmosphere Research (ALIMA) is a Rayleigh and Doppler iron lidar designed to fly on an aircraft. Its development started in 2014. It is currently being built and certified for operation on the HALO research aircraft. The first campaign will be SOUTHTRAK in southern America in fall 2019.
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Type: Rayleigh backscatter lidar The Balloon Lidar Experiment (BOLIDE) is a compact, balloon-borne lidar housed in a pressure vessel that flew on the NASA long-duration balloon mission PMC-Turbo in July 2018. |
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CORAL
Type: Rayleigh backscatter lidar |
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The Compact Rayleigh Autonomous Lidar (CORAL) is a stratosphere/mesosphere temperature lidar developed in 2015. The primary objective of the instrument is to autonomously collect high-resolution soundings of atmospheric gravity waves. To achieve this, CORAL features several technologies which are new to middle atmosphere lidars: diode-pumped laser, highly integrated electronics, redundant computer systems, advance software with fault protection algorithms. CORAL was employed during the NORTHWAVE campaign in Sodankylä, Finland, in winter 2015/2016, for the LART-A/ARISE-2 campaign in the Bavarian Forest in summer 2016 and in the SOUTHWAVE campaign in Rio Grande, Tierra del Fuego, Argentina since November 2017.
The Temperature Lidar for the Middle Atmosphere (TELMA) is the predecessor of CORAL with support for remote operation that was used during the DEEPWAVE campaign at Lauder, New Zealand in southern winter 2014. The instrument is housed in an 11-foot container. It emits 12 W at 532 nm and uses a 63 cm aperture telescope. The field of view is 200 microrad. |
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