Abstract

Abstract. A new concept for a cluster of compact lidar systems named VAHCOLI (Vertical And Horizontal COverage by LIdars) is presented, which allows for the measurement of temperatures, winds, and aerosols in the middle atmosphere (∼ 10–110 km) with high temporal and vertical resolution of minutes and some tens of meters, respectively, simultaneously covering horizontal scales from a few hundred meters to several hundred kilometers (“four-dimensional coverage”). The individual lidars (“units”) being used in VAHCOLI are based on a diode-pumped alexandrite laser, which is currently designed to detect potassium (λ=770 nm), and on sophisticated laser spectroscopy measuring all relevant frequencies (seeder laser, power laser, backscattered light) with high temporal resolution (2 ms) and high spectral resolution applying Doppler-free spectroscopy. The frequency of the lasers and the narrowband filter in the receiving system are stabilized to typically 10–100 kHz, which is a factor of roughly 10−5 smaller than the Doppler-broadened Rayleigh signal. Narrowband filtering allows for the measurement of Rayleigh and/or resonance scattering separately from the aerosol (Mie) signal during both night and day. Lidars used for VAHCOLI are compact (volume: ∼ 1 m3) and multi-purpose systems which employ contemporary electronic, optical, and mechanical components. The units are designed to autonomously operate under harsh field conditions in remote locations. An error analysis with parameters of the anticipated system demonstrates that temperatures and line-of-sight winds can be measured from the lower stratosphere to the upper mesosphere with an accuracy of ±(0.1–5) K and ±(0.1–10) m s−1, respectively, increasing with altitude. We demonstrate that some crucial dynamical processes in the middle atmosphere, such as gravity waves and stratified turbulence, can be covered by VAHCOLI with sufficient temporal, vertical, and horizontal sampling and resolution. The four-dimensional capabilities of VAHCOLI allow for the performance of time-dependent analysis of the flow field, for example by employing Helmholtz decomposition, and for carrying out statistical tests regarding, for example, intermittency and helicity. The first test measurements under field conditions with a prototype lidar were performed in January 2020. The lidar operated successfully during a 6-week period (night and day) without any adjustment. The observations covered a height range of ∼ 5–100 km and demonstrated the capability and applicability of this unit for the VAHCOLI concept.

Highlights

  • Lidars have been used in atmospheric research for many years

  • Backscattering from molecules (Rayleigh, Raman) and aerosols (Mie) as well as resonance scattering from metal atoms in the upper mesosphere–lower thermosphere have been applied to deduce number densities, temperatures, winds, and important characteristics of aerosols such as noctilucent clouds (NLCs) and polar stratospheric clouds (PSCs)

  • Several improvements regarding the technical performance of lidars being used for VAHCOLI are currently in progress or are foreseen for the near future

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Summary

Introduction

Lidars (light detection and ranging) have been used in atmospheric research for many years. Höffner: VAHCOLI: concept and applications perform measurements in the vertical, but oblique soundings have been applied occasionally, e.g., for the lidars at ALOMAR (Arctic Lidar Observatory for Middle Atmosphere Research) and at the Starfire Optical Range (von Zahn et al, 2000; Chu et al, 2005). Lidars have been developed for applications on airplanes and balloons, which can travel substantial horizontal distances but are limited in resolving temporal and spatial ambiguities (see, for example, Shepherd et al, 1994; Voigt et al, 2018; Fritts et al, 2020). Multistatic radars are available to measure winds in the upper mesosphere–lower thermosphere with extended horizontal coverage (Chau et al, 2017; Vierinen et al, 2019) Compared to lidars these techniques cover a rather limited height range. It must still be able to measure various scattering mechanisms to monitor the atmosphere from approximately 10 to 100 km

General
Spectral characteristics of scattered signals and lidar components
General lidar setup
Laser specifications
Telescope and receiver
Data acquisition and lidar control
Temperatures and winds from Rayleigh and resonance scattering
Aerosol parameters and winds
Metal densities
Lidar operation
First measurements
Expected performance
Error analysis for Rayleigh temperatures
Multi-beam operation and horizontal coverage
Gravity waves
Other dynamical parameters
Findings
Outlook and conclusion
Full Text
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