The combined effect of ultraviolet radiation and turbulent mixing on chemis
try in a cloud-topped boundary layer is investigated. The authors study a R
ow driven by longwave radiative cooling at cloud top. They consider a chemi
cal cycle that is composed of a first-order reaction whose photodissociatio
n rate depends on the cloud properties and time and a second-order chemical
reaction between an abundant entrained reactant and a species with an init
ial concentration in the boundary layer. This turbulent reacting flow is re
presented numerically by means of a large eddy simulation. The simulation d
oes not take evaporative cooling and aqueous-phase chemistry into account;
that is, the authors simulate a dry smoke cloud.
The vertical concentration profiles of the reactants not in excess clearly
show the appearance of gradients due to the chemical sources and sinks in t
he cloud. Moreover, the vertical-flux profiles depart from a linear profile
. Fluxes that, in the absence of chemistry, are directed upward could chang
e direction due to the different chemical reaction rate constants inside an
d below the cloud and because of the dominant downward motions generated by
radiative cooling. The flux-budget analysis shows the relevance of the che
mical term for the nonabundant species inside of the cloud, The exchange fl
ux between the free troposphere and the boundary layer also depends on the
chemical transformation above and in the cloud. An expression for the excha
nge velocity of reactive species is proposed in terms of an in-cloud flux,
the production-depletion chemical rates, and the concentration jump at the
inversion height. The calculated exchange velocity values For the smoke and
the reactants differ considerably.