Abstract

An extreme haze event occurred in the Beijing area from 17 to 23 December 2015. Ground-based measurements and satellite observations during this event were used to further our understanding of the formation process of haze pollution and aerosol optical properties. The results suggest that high relative humidity, poor diffusion conditions (low wind speed and stable stratification) and favorable secondary transformation conditions under the hygroscopic growth of aerosol and high emissions led to this serious haze episode. During the haze period, the daily average value was 1.15 and 0.42 for aerosol optical depth (AOD500nm) and columnar water-vapor (CWV, in cm), respectively. On 19 December, the correlation coefficient between CWV and AOD500nm was 0.91, indicating the effect of hygroscopic growth of fine-mode articles. The daily average values for Ångström exponent, fine-mode fraction, aerosol absorption optical depth, and Ångström absorption exponent were 1.19, 0.81, 0.11 and 1.47, respectively, which suggests that fine aerosol particles were dominant in the atmosphere and fine-mode particles were the dominant contributor to atmospheric extinction during the haze period. Moreover, it also reflects that there were more absorbing aerosol particles during the haze period. Compared with other polluted periods with a bimodal distribution, there was an obvious trimodal distribution on 19 December. There were three peaks at radii of about 0.1 μm, 0.5–0.8 μm and 4 μm. Satellite observations show that there was an obvious aerosol layer in the Beijing area during the haze period, concentrated at ground level to within 2 km in the upper layers. The types of aerosol were mainly composed of mixed pollution aerosols.

Highlights

  • Aerosol particles have a substantial influence on global and regional climate change by absorbing and scattering solar radiation [1,2]

  • It can be CWV reduced to 0.35 cm with a smooth trend of change, hygroscopic growth of aerosols was not seen from Figure 5b that the fine-mode fraction (FMF) on 22 December was larger than 98%, indicating that fine-mode significant, and the AE concentrated at around 1.2

  • The CALIPSO satellite can provide vertical structure and optical be influenced by the noise of strong solar radiation, so the daytime data in this case were only used for be influenced by the noise of strong solarduring radiation, the daytime in this the casedaytime were only used property information regarding aerosol hazeso periods

Read more

Summary

Introduction

Aerosol particles have a substantial influence on global and regional climate change by absorbing and scattering solar radiation [1,2]. There are several well-known ground-based networks that use sunphotometers, such as AERONET (Aerosol Robotic Network) [19], PHOTONS (PHOtométrie pour le Traitement Opérationnel de Normalisation Satellitaire) [20], CARSNET (China Aerosol Remote Sensing Network) [21,22], and SKYNET [23]. These networks have been used to measure direct and diffuse solar radiation, and so derive aerosol optical, microphysical and radiative properties for aerosol research and the characterization and validation of satellite retrievals. The results will help to uncover the mechanism of haze event formation, and improve knowledge on aerosol optical properties during haze events in the Beijing area

Site Description and Instrumentation
Meteorological Data and Ground Measurements
Satellite Datasets
Analysis of PM and Meteorological Data
17 Dece mber December December December December December December
23 December
Analysis
Aerosol Optical
2.62. The AE
SSA and Size Distribution
23 December b
Aerosol
17 Dec ember
Satellite View of the Haze over Beijing
Backward Trajectory Analysis
Conclusions
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call