2015
DOI: 10.1109/tgrs.2015.2401333
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Lidars With Narrow FOV for Daylight Measurements

Abstract: Daytime lidar operation in the middle atmosphere requires a narrow field of view (FOV) of the receiving telescope for effective background reduction and a high-transmission narrow-band detection. The laser beam position in the atmosphere relative to the optical axis of the receiving telescope is subject to high-frequency disturbances such as turbulence, vibration, and wind as well as comparable slow drift (thermal effects of the laser, stability of the building, etc.). We developed a beam stabilization system … Show more

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Cited by 13 publications
(8 citation statements)
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“…To reduce the effects of tropospheric turbulence on the laser beam propagation and the alignment of laser and telescope FOV, an active beam stabilization based on a Piezo‐coupled mirror is used [ Eixmann et al , ]. This method was first developed for the mobile IAP iron lidar by Höffner and Lautenbach [].…”
Section: Instrumentation and Datamentioning
confidence: 99%
“…To reduce the effects of tropospheric turbulence on the laser beam propagation and the alignment of laser and telescope FOV, an active beam stabilization based on a Piezo‐coupled mirror is used [ Eixmann et al , ]. This method was first developed for the mobile IAP iron lidar by Höffner and Lautenbach [].…”
Section: Instrumentation and Datamentioning
confidence: 99%
“…Two steering mirrors and one fixed mirror are used to guide the light into the atmosphere, co-axially with the receiving telescope. The first of these steering mirrors is Piezo-mounted and used for beam stabilization (Eixmann et al, 2015). By computer-controlled beam stabilization the beam axis is fixed to the optical axis of the telescope on a single pulse basis to overcome the effects of, e.g., atmospheric turbulence on the geometrical overlap of beam and telescope.…”
Section: Instrumental Setup Of the New Iap Rmr Lidarmentioning
confidence: 99%
“…The laser is emitted co-axially with the receiving telescope by means of different steerable mirrors. A beam-stabilization based on a Piezo-coupled mirror is used to keep the laser beam within the 62 µrad field of view of the telescope [7]. Input for beam-stabilization is provided by a CCD camera observing the beam in real-time through the same telescope and a 90:10 beam splitter.…”
Section: Methodsmentioning
confidence: 99%