Global determinations of the response of radio wave absorption in the
ionosphere to changes in the solar zenith angle show that this respons
e is relatively weak in winter compared to that in summer and equinox
in non-equatorial regions. In a bid to understand this behaviour, a nu
merical simulation of the response has been attempted employing solsti
ce and equinox electron density profiles derived from minor neutral sp
ecies concentrations of a zonally averaged photochemical-transport tim
e-dependent model of the middle atmosphere, ion chemistry and solar ir
radiance fluxes. The results have established that the seasonal variat
ion in the response is related to seasonally and latitudinally varying
nitric oxide abundance in the mesosphere resulting from corresponding
changes in its chemistry and transport.