Preprints
https://doi.org/10.5194/egusphere-2026-5744
https://doi.org/10.5194/egusphere-2026-5744
09 Oct 2026
 | 09 Oct 2026
Status: this preprint is open for discussion and under review for Atmospheric Measurement Techniques (AMT).

The Versatile Atmospheric Laser Doppler Instrument VALDI: A single Fizeau interferometer and imaging detector, for simultaneous wind speed, temperature and scattering ratio measurements from molecular and aerosol scattering

Michael Vaughan, Kevin Ridley, Oliver Reitebuch, and Benjamin Witschas

Abstract. This feasibility study demonstrates, through modelling and simulation, that a Versatile Atmospheric Laser Doppler Instrument (VALDI), based on a single Fizeau interferometer and imaging detector, has the potential for precise, high-sensitivity, simultaneous measurements of wind speeds, temperature and atmospheric scattering ratio (ASR). In simple principle, the linear frequency dispersion of the Fizeau interferometer creates in the fringe plane an extended spectrum of atmospheric scattering. This is made up of broadband molecular scattering resulting in a Rayleigh-Brillouin spectral component of ≈4 GHz full width at half maximum (at 355 nm wavelength), and a narrow band spectral component originating from aerosol (Mie) scattering with spectral characteristics defined by the laser source and Fizeau design parameters. For the present investigation, a 16 channel detector, similar to those employed in ESA’s Aeolus spaceborne lidar is considered, together with an adapted Fizeau interferometer of specifications (plate separation, wedge angle, finesse, etc.) well within current practice. Extensive modelling and simulation demonstrates that the 16 detector channels of spectral information provide versatile, high sensitivity operation, for widely varying atmospheric scattering and attenuation conditions throughout the troposphere and lower stratosphere. Drawing on operational data and experience of the ESA Aeolus spaceborne lidar systems, simulations indicate that a spaceborne VALDI could achieve wind speed uncertainties σvHLOS in the range of ±1.4 m s−1 to ±3.2 m s−1, from the aerosol signal in central detector channels (with ASR ≈ 2 and 12 km observational path). The outer channels, dominated by molecular signal, should give wind speed uncertainties between ±2.4 m s−1 and ±3.4 m s−1 (for 87 km observation path length). It is further shown that fast analytical ratio techniques provide Doppler frequency analysis with accuracy approaching the Cramér-Rao ultimate quantum limit within 10 % to 20 %. Finally, questions of practical design, construction and operation are considered. In this regard the single interferometer and detector, with single optical delivery train, offers considerable advantages of optical simplicity, high signal throughput efficiency, robustness and good long term alignment control and stability, plus wide frequency/wind speed capability extending well above 100 m s−1.

Competing interests: One of the (co-)authors (Oliver Reitebuch) is a member of the editorial board of Atmospheric Measurement Techniques.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
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Michael Vaughan, Kevin Ridley, Oliver Reitebuch, and Benjamin Witschas

Status: open (until 14 Nov 2026)

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Michael Vaughan, Kevin Ridley, Oliver Reitebuch, and Benjamin Witschas
Michael Vaughan, Kevin Ridley, Oliver Reitebuch, and Benjamin Witschas
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Short summary
We investigate a new space-based lidar concept for measuring atmospheric winds, aerosol levels and temperature at the same time. Using computer modelling and experience from the Aeolus mission, we assess whether one optical receiver could provide all these measurements. The results show that the concept has the potential to deliver accurate atmospheric observations from space, offering a compact approach for future Earth-observation missions.
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