Abstract

Abstract. Multi-axis differential optical absorption spectroscopy (MAX-DOAS) observations of trace gases can be strongly influenced by clouds and aerosols. Thus it is important to identify clouds and characterize their properties. In a recent study Wagner et al. (2014) developed a cloud classification scheme based on the MAX-DOAS measurements themselves with which different "sky conditions" (e.g., clear sky, continuous clouds, broken clouds) can be distinguished. Here we apply this scheme to long-term MAX-DOAS measurements from 2011 to 2013 in Wuxi, China (31.57° N, 120.31° E). The original algorithm has been adapted to the characteristics of the Wuxi instrument, and extended towards smaller solar zenith angles (SZA). Moreover, a method for the determination and correction of instrumental degradation is developed to avoid artificial trends of the cloud classification results. We compared the results of the MAX-DOAS cloud classification scheme to several independent measurements: aerosol optical depth from a nearby Aerosol Robotic Network (AERONET) station and from two Moderate Resolution Imaging Spectroradiometer (MODIS) instruments, visibility derived from a visibility meter and various cloud parameters from different satellite instruments (MODIS, the Ozone Monitoring Instrument (OMI) and the Global Ozone Monitoring Experiment (GOME-2)). Here it should be noted that no quantitative comparison between the MAX-DOAS results and the independent data sets is possible, because (a) not exactly the same quantities are measured, and (b) the spatial and temporal sampling is quite different. Thus our comparison is performed in a semi-quantitative way: the MAX-DOAS cloud classification results are studied as a function of the external quantities. The most important findings from these comparisons are as follows: (1) most cases characterized as clear sky with low or high aerosol load were associated with the respective aerosol optical depth (AOD) ranges obtained by AERONET and MODIS; (2) the observed dependences of MAX-DOAS results on cloud optical thickness and effective cloud fraction from satellite confirm that the MAX-DOAS cloud classification scheme is sensitive to cloud (optical) properties; (3) the separation of cloudy scenes by cloud pressure shows that the MAX-DOAS cloud classification scheme is also capable of detecting high clouds; (4) for some cloud-free conditions, especially with high aerosol load, the coincident satellite observations indicated optically thin and low clouds. This finding indicates that the satellite cloud products contain valuable information on aerosols.

Highlights

  • In the last decade, multi-axis (MAX-) differential optical absorption spectroscopy (DOAS) has received considerable attention due to its application to the retrieval of vertical distributions of trace gases and aerosols (Hönninger et al, 2004; Bobrowski et al, 2003; Pikelnaya et al, 2007; Sinreich et al, 2007; Theys et al, 2007; Clémer et al, 2009, 2010; Wagner et al, 2011; Vlemmix et al, 2010, 2011, 2015)

  • We compared the results of the MAX-DOAS cloud classification scheme to several independent measurements: aerosol optical depth from a nearby Aerosol Robotic Network (AERONET) station and from two Moderate Resolution Imaging Spectroradiometer (MODIS) instruments, visibility derived from a visibility meter and various cloud parameters from different satellite instruments (MODIS, the Ozone Monitoring Instrument (OMI) and the Global Ozone Monitoring Experiment (GOME-2))

  • The most important findings from these comparisons are as follows: (1) most cases characterized as clear sky with low or high aerosol load were associated with the respective aerosol optical depth (AOD) ranges obtained by AERONET and MODIS; (2) the observed dependences of MAX-DOAS results on cloud optical thickness and effective cloud fraction from satellite confirm that the MAX-DOAS cloud classification scheme is sensitive to cloud properties; (3) the separation of cloudy scenes by cloud pressure shows that the MAX-DOAS cloud classification scheme is capable of detecting high clouds; (4) for some cloud-free conditions, especially with high aerosol load, the coincident satellite observations indicated optically thin and low clouds

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Summary

Introduction

Multi-axis (MAX-) differential optical absorption spectroscopy (DOAS) has received considerable attention due to its application to the retrieval of vertical distributions of trace gases and aerosols (Hönninger et al, 2004; Bobrowski et al, 2003; Pikelnaya et al, 2007; Sinreich et al, 2007; Theys et al, 2007; Clémer et al, 2009, 2010; Wagner et al, 2011; Vlemmix et al, 2010, 2011, 2015). To verify the cloud classification scheme, the sky conditions identified by MAX-DOAS are compared to cloud and aerosol products from a variety of independent ground-based and satellite instruments, such as the Aerosol Robotic Network (AERONET) (Holben et al, 1998, 2001), a visibility meter, the Ozone Monitoring Instrument (OMI) (Levelt et al, 2006a, b), the Global Ozone Monitoring Experiment (GOME-2) (Callies et al, 2000; Munro et al, 2006, 2015) and the two Moderate Resolution Imaging Spectroradiometer (MODIS) instruments (http://modis.gsfc.nasa.gov/) (Kaufmann et al, 2002) It should, be noted that no direct comparison between the MAX-DOAS results and the independent data sets is possible because of two reasons.

MAX-DOAS instrument
Quantities from MAX-DOAS observations
Radiance and color index
O4 absorption
The scheme of the classification of sky conditions
General principles and construction of the classification scheme
Description of the adapted scheme
Continuous clouds for small SZA
Exceptional case: extremely high midday CI
Spread of the CI
AERONET AOD and visibility meter
OMI and GOME-2 cloud products
Results
Uncertainties of the classification method
Comparison with coincident ground-based and satellite measurements
Comparison to AERONET AOD
Comparison to visibility meter
Influence of the spatial and temporal averaging on the comparison results
Discussion and conclusion
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