  After the sunset, under calm and clear sky conditions, aerosol laden surface
air-layer, cools radiatively to the upper atmosphere. Predominant effect of the
radiative cooling on the vertical temperature profile extends to several
hundred meters from the surface. This results in the development of a stable,
nocturnal inversion layer. However, ground surface, owing to its higher thermal
inertia, lags in the cooling process. Due to this about a meter thick air layer
just above the ground can be (2-6)deg Celsius cooler than the ground. Thus, at
the surface an unstable convective layer is present, which is capped by a
stable inversion layer that extends up to several hundred meters. This
configuration involving a convective mixed layer topped by a stably stratified
inversion layer is a classic case of penetrative convection.
Micrometeorological phenomenon at the surface, such as occurrence of fog, is
determined by temperature profile, heat and moisture transport from the ground.
Here, we present a computational study of the model penetrative convection,
formed due to radiative cooling, in the nocturnal atmospheric boundary layer.
