Abstract. To investigate the physical and chemical processes of
fine particle matter (PM) at the mid-upper planetary boundary layer (PBL), we
conducted 1-year continuous measurements of fine PM, the
chemical composition of non-refractory submicron aerosol (NR-PM1), and
some gas species (including sulfur dioxide, nitrogen oxides, and ozone) at an
opening observatory (∼ 600 m) at the top of Shanghai Tower
(SHT), which is China's first and the world's second highest building
located in the typical financial central business district of Shanghai,
China. This is the first report on the characteristics of fine particles
based on continuous and sophisticated online measurements at the mid-upper
level of the urban PBL. The observed PM2.5 and PM1 mass concentrations
at SHT were 25.5 ± 17.7 and 17.3 ± 11.7 µg m−3,
respectively. Organics, nitrate (NO3), and sulfate (SO4) occupied
the first three leading contributions to NR-PM1 at SHT, accounting for
35.8 %, 28.6 %, and 20.8 %, respectively. The lower PM2.5
concentration was observed at SHT by 16.4 % compared with that near the
surface during the observation period. It was attributed to the decreased
nighttime PM2.5 concentrations (29.4 % lower than the surface) at SHT in
all seasons due to the complete isolations from both emissions and gas
precursors near the surface. However, daytime PM2.5 concentrations at SHT
were 12.4 %–35.1 % higher than those near the surface from June to October,
resulted from unexpected larger PM2.5 levels during early to middle
afternoon at SHT than at the surface. We suppose the significant chemical
production of secondary aerosols existed in the mid-upper PBL, because strong
solar irradiance, adequate gas precursors (e.g., NOx), and lower temperature
were observed at SHT, favorable for both photochemical production and
gas-to-particle partitioning. This was further demonstrated by the
significant increasing rate of oxygenated organic aerosols and NO3
observed at SHT during 08:00–12:00 in spring (7.4 % h−1 and 12.9 % h−1), fall (9.3 % h−1 and 9.1 % h−1), and summer (13.0 % h−1 and 11.4 % h−1), which cannot be fully explained by
vertical mixing. It was noted that extremely high NO3 was observed at
SHT both in daytime and nighttime in winter, accounting for 37.2 % in
NR-PM1, suggesting the efficient pathway from heterogeneous and gas
oxidation formation. Therefore, we highlight the priority of NOx reduction in
Shanghai for the further improvement of air quality. This study reported
greater daytime PM2.5 concentrations at the height of 600 m in the urban
PBL compared with surface measurement, providing insight into their
potential effects on local air quality, radiation forcing, and cloud and/or fog
formations. We propose that the efficient production of secondary aerosol in the
mid-upper PBL should be cognized and explored more comprehensively by
synergetic observations in future.