2007
DOI: 10.1117/12.701187
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Frequency stabilization of Q-switched Nd:YAG oscillators for airborne and spaceborne lidar systems

Abstract: Lidar Systems for the measurement of three-dimensional wind or cloud and aerosol formations in the earth atmosphere require highly stable pulsed single frequency laser systems with a narrow line width. The lasers for ESAs ADM-Aeolus and EarthCARE missions require frequency stabilities of 4 and 10 MHz rms at a wavelength of 355 nm and a line width below 50 MHz at 30 ns pulse duration[1]. Transferred to the fundamental wavelength of the laser systems the stability requirement is 1.3 and 3.3 MHz, respectively. In… Show more

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Cited by 32 publications
(20 citation statements)
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“…In addition to the strict requirements in terms of frequency stability, a further challenge is imposed by the necessity to trigger the receiver electronics about 60 µs before the laser pulse emission with an error of less than 100 ns. Therefore, a dedicated active frequency stabilization technique was developed which is based on the ramp-delay-fire method (Nicklaus et al, 2007). Fast detection of the master oscillator cavity resonances with the seed laser frequency enabled effective compensation of higher-frequency vibrations, while providing a sufficiently early trigger for the detector electronics with a timing stability of around 80 ns .…”
Section: Laser Transmitter Telescope and Front Opticsmentioning
confidence: 99%
“…In addition to the strict requirements in terms of frequency stability, a further challenge is imposed by the necessity to trigger the receiver electronics about 60 µs before the laser pulse emission with an error of less than 100 ns. Therefore, a dedicated active frequency stabilization technique was developed which is based on the ramp-delay-fire method (Nicklaus et al, 2007). Fast detection of the master oscillator cavity resonances with the seed laser frequency enabled effective compensation of higher-frequency vibrations, while providing a sufficiently early trigger for the detector electronics with a timing stability of around 80 ns .…”
Section: Laser Transmitter Telescope and Front Opticsmentioning
confidence: 99%
“…Due to remaining imperfections in the seeding process (thermal perturbations etc.) the wavelength of the outgoing laser pulse can show an offset to the seed laser (Nicklaus et al, 2007). Therefore we measure the emitted wavelength during the atmospheric measurements with an I 2 pulse spectrometer .…”
Section: Methods and Instrumental Setupmentioning
confidence: 99%
“…In addition to the strict requirements in terms of frequency stability, a further challenge is imposed by the necessity to trigger the receiver electronics about 60 μs before the laser pulse emission with an error of less than 100 ns. Therefore, a dedicated active frequency stabilization technique was developed which is based on the Ramp-Delay-Fire method (Nicklaus et al, 2007). Fast detection of the master oscillator cavity resonances with 5 the seed laser frequency enabled effective compensation of higher-frequency vibrations, while providing a sufficiently early trigger for the detector electronics with a timing stability of around 80 ns (Lemmerz et al, 2017).…”
Section: Laser Transmitter Telescope and Front Opticsmentioning
confidence: 99%