Abstract. Gaseous sulfuric acid (SA) has received a lot of
attention for its crucial role in atmospheric new particle formation (NPF). And for this reason, studies until now have mainly focused on daytime SA
when most NPF events occur. While daytime SA production is driven by
SO2 oxidation of OH radicals of photochemical origin, the formation of
SA during nighttime and its potential influence on particle formation remains
poorly understood. Here we present evidence for significant nighttime SA
production in urban Beijing during winter, yielding concentrations between
1.0 and 3.0 × 106 cm−3. We found a high frequency
(∼ 30 %) of nighttime SA events, which are defined by the
appearance of a distinct SA peak observed between 20:00 and 04:00 local
time, with the maximum concentration exceeding 1.0 × 106 cm−3. These events mostly occurred during unpolluted nights with a low
vapor condensation sink. Furthermore, we found that under very clean
conditions (visibility > 16.0 km) with abundant ozone
(concentration > 2.0 × 1011 cm−3,
∼ 7 ppb), the overall sink of SA was strongly correlated with
the products of O3, alkenes and SO2 concentrations, suggesting
that the ozonolysis of alkenes played a major role in nighttime SA formation
under such conditions. This is in light of previous studies showing that
the ozonolysis of alkenes can form OH radicals and stabilized Criegee
intermediates (SCIs), both of which are able to oxidize SO2 and thus
lead to SA formation. However, we also need to point out that there exist
additional sources of SA under more polluted conditions, which are not
investigated in this study. Moreover, there was a strong correlation between
SA concentration and the number concentration of sub-3 nm particles on both
clean and polluted nights. Different from forest environments, where
oxidized biogenic vapors are the main driver of nighttime clustering, our
study demonstrates that the formation of nighttime cluster mode particles in
urban environments is mainly driven by nighttime SA production.