Air pollution episodes have been recorded in Cairo, during the fall
season, since 1999, as a result of specific meteorological conditions
combined with large quantity of pollutants created by several
ground-based sources.
The main reason for the smog-like episodes (black clouds) is adverse
weather conditions with low and variable winds, high humidity and
strong temperature inversions in the few-hundred meters above the
ground. The two important types of temperature inversion affecting the
air pollution are surface or ground (radiation) inversion and
subsidence (elevated) inversion. The surface temperature inversion is
associated with a rapid decrease in the ground surface temperature with
the simultaneous existence of warm air in the lower troposphere. The
inversion develops at dusk and continues until the surface warms again
the following day. Pollutants emitted during the night are caught under
this “inversion lid.” Subsidence inversion forms when warm air masses
move over colder air masses. The inversion develops with a stagnating
high-pressure system (generally associated with fair weather). Under
these conditions, the pressure gradient becomes progressively weaker so
that winds become light. These light winds greatly reduce the
horizontal transport and dispersion of pollutants. At the same time,
the subsidence inversion acts as a barrier to the vertical dispersion
of the pollutants.
In this study, the Penn State/NCAR meso -scale model (MM5) is used to
simulate the temperature inversion phenomenon over Greater Cairo region
during the fall season of 2004. Accurate computations of the heat
transfer at the surface are needed to capture this phenomenon. This can
only be achieved by high-resolution simulations in both horizontal and
vertical directions. Hence, for accurate simulation of the temperature
inversion over Greater Cairo, four nested domains of resolutions of 27
km, 9 km, 3 km and 1 km, respectively, were used in the horizontal
planes. Furthermore, 42 levels were used in the vertical direction to
capture the correct surface heat flux and to observe the small changes
in the vertical temperature gradient.
The results of the numerical model showed that it is possible to
capture both types of temperature inversion during the night and early
morning hours. This can be observed from the results of the vertical
temperature profile and temperature gradient, which indicate that an
inversion system was present over Cairo at a layer extending between
300 m and 800 m above the ground.