Abstract. Deep convective clouds are critically important to the distribution of
atmospheric constituents throughout the troposphere but are difficult
environments to study. The Deep Convective Clouds and Chemistry (DC3) study
in 2012 provided the environment, platforms, and instrumentation to test
oxidation chemistry around deep convective clouds and their impacts downwind.
Measurements on the NASA DC-8 aircraft included those of the radicals
hydroxyl (OH) and hydroperoxyl (HO2), OH reactivity, and more than
100 other chemical species and atmospheric properties. OH, HO2, and
OH reactivity were compared to photochemical models, some with and some
without simplified heterogeneous chemistry, to test the understanding of
atmospheric oxidation as encoded in the model. In general, the agreement
between the observed and modeled OH, HO2, and OH reactivity was
within the combined uncertainties for the model without heterogeneous
chemistry and the model including heterogeneous chemistry with small OH and
HO2 uptake consistent with laboratory studies. This agreement is
generally independent of the altitude, ozone photolysis rate, nitric oxide
and ozone abundances, modeled OH reactivity, and aerosol and ice surface
area. For a sunrise to midday flight downwind of a nighttime mesoscale
convective system, the observed ozone increase is consistent with the
calculated ozone production rate. Even with some observed-to-modeled
discrepancies, these results provide evidence that a current
measurement-constrained photochemical model can simulate observed atmospheric
oxidation processes to within combined uncertainties, even around convective
clouds. For this DC3 study, reduction in the combined uncertainties would be
needed to confidently unmask errors or omissions in the model chemical
mechanism.