Abstract

Abstract. Vertical profiles of aerosol particle optical properties were explored in a case study near the San Pietro Capofiume (SPC) ground station during the PEGASOS Po Valley campaign in the summer of 2012. A Zeppelin NT airship was employed to investigate the effect of the dynamics of the planetary boundary layer at altitudes between ∼ 50 and 800 m above ground. Determined properties included the aerosol particle size distribution, the hygroscopic growth factor, the effective index of refraction and the light absorption coefficient. The first three parameters were used to retrieve the light scattering coefficient. Simultaneously, direct measurements of both the scattering and absorption coefficient were carried out at the SPC ground station. Additionally, a single wavelength polarization diversity elastic lidar system provided estimates of aerosol extinction coefficients using the Klett method to accomplish the inversion of the signal, for a vertically resolved comparison between in situ and remote-sensing results. Note, however, that the comparison was for the most part done in the altitude range where the overlap function is incomplete and accordingly uncertainties are larger. First, the airborne results at low altitudes were validated with the ground measurements. Agreement within approximately ±25 and ±20 % was found for the dry scattering and absorption coefficient, respectively. The single scattering albedo, ranged between 0.83 and 0.95, indicating the importance of the absorbing particles in the Po Valley region. A clear layering of the atmosphere was observed during the beginning of the flight (until ∼ 10:00 LT – local time) before the mixing layer (ML) was fully developed. Highest extinction coefficients were found at low altitudes, in the new ML, while values in the residual layer, which could be probed at the beginning of the flight at elevated altitudes, were lower. At the end of the flight (after ∼ 12:00 LT) the ML was fully developed, resulting in constant extinction coefficients at all altitudes measured on the Zeppelin NT. Lidar estimates captured these dynamic features well and good agreement was found for the extinction coefficients compared to the in situ results, using fixed lidar ratios (LR) between 30 and 70 sr for the altitudes probed with the Zeppelin. These LR are consistent with values for continental aerosol particles that can be expected in this region.

Highlights

  • Atmospheric aerosol particles are known to interact directly with the incident solar radiation by either scattering or absorbing light

  • If the mixing layer (ML) aerosol imprint is present in the signal, the indetermination in the mixing layer height (MLH) retrieval is of the order of 2–3 signal bins (i.e. ±30–45 m)

  • The aerosol properties in these two layers could potentially be significantly different since the residual layer (RL) is mainly dependent on the planetary boundary layer (PBL) from the day before, while the new ML is affected by direct emissions from the same day

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Summary

Introduction

Atmospheric aerosol particles are known to interact directly with the incident solar radiation by either scattering or absorbing light. One major point of interest is to know whether surface-based measurements can be used to infer aerosol radiative properties at elevated altitudes For this purpose, remote-sensing techniques such as light detection and ranging (lidar) instruments are useful to monitor optical properties such as aerosol extinction and backscattering coefficient over a large range of altitudes. During the PEGASOS (Pan-European gas–aerosols climate interaction study) project a Zeppelin NT airship was employed to study aerosols at altitudes between 50 and 800 m above ground This offered a unique opportunity to compare in situ measurements to low altitude lidar estimates, which is known to be challenging A consistency check for the airborne results is done by comparison to ground-based data

Site and flight description
Aerosol particle size distributions
Hygroscopic properties
Aerosol scattering coefficient
Aerosol absorption coefficient
Aerosol extinction coefficient
Results and discussion
Vertical profiles of aerosol scattering and absorption coefficients
Light scattering enhancement at ambient RH
80 RHambient
Vertical profiles of the single scattering albedo
Vertically resolved aerosol extinction coefficients
Conclusions
Full Text
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