View the article online for updates and enhancements. Abstract. Urban air quality assessment requires the knowledge of the temporal and spatial structure of the mixing-layer height (MLH), because this variable controls the vertical space for rapid mixing of near-surface pollutants. Because MLH is a consequence of vertical temperature and moisture profiles in the lower atmosphere, remote sensing is a suitable tool to monitor MLH. Two ceilometers, a Vaisala LD40 and a Vaisala CL31, have been run for many months in the German city of Augsburg to observe the vertical aerosol distribution. Wind and temperature profile information have been obtained for the same period from sodar observations. This paper compares the MLH determined from the optical backscatter intensity received by the two ceilometers among each other and with the MLH derived from the acoustic backscatter intensity and the variance of the vertical wind component from sodar measurements.
Related content
IntroductionThe mixing layer height (MLH) is assumed to be a key parameter for the characterisation of air pollution, because this variable controls the vertical space for rapid mixing of near-surface pollutants. The determination and modelling of the MLH has therefore found considerable interest in the recent decade [1], especially in urban meteorology. With today's availability of ground-based remote sensing devices for monitoring the structure of the atmospheric boundary layer (ABL) it has been shown that the ABL sometimes exhibits multiple layering (e.g. internal boundary layers, near-surface inversions and residual layers at night-time and in the morning hours) [2]. It was demonstrated that the lowest stable layer or inversion limits the vertical exchange of primary pollutants emitted at or near the surface [3] and thus controls the near-surface pollutant concentrations. Acoustic remote sensing has also been used to derive climatologic statistics of MLH for towns ([4], [5]) and wind and turbulence profiles over towns [6]. Multiple inversions within a few hundred meters above ground have been detected both with optical and acoustic remote sensing in an Alpine valley [7]. MLH information is also necessary for special kinds of satellite data interpretation, e. g. the retrievals of optical depths for the particle concentration near the surface [8].