Direct numerical simulations (DNS) of natural convection in a vertical chan
nel by Versteegh & Nieuwstadt (1998) are used for assessing the budget of t
he turbulent heat flux <(theta u(i))over bar> and the temperature variance
<(theta(2))over bar>, and for modelling the transport equations governing t
hese two properties. The analysis is confined to a simple fully developed s
ituation in which the gravitational vector, as the sole driving force, is p
erpendicular to the only non-zero component of the mean temperature gradien
t. Despite its simplicity, the flow displays many interesting features and
represents a generic case of the interaction of buoyancy-driven turbulent t
emperature and velocity fields. The paper discusses the near-wall variation
of the second moments and their budgets, as well as possible scaling of <(
theta u(i))over bar> and <(theta(2))over bar> both in the near-wall region
and away from the wall. Various proposals for the Reynolds-averaged modelli
ng are analysed and new models are proposed for these two transport equatio
ns using the term-by-term approach. An a priori test (using the DNS data fo
r properties other than <(theta u(i))over bar> and <(theta(2))over bar>) re
produced very well all terms in the transport equations, as well as their n
ear-wall behaviours and wall limits, without the use of any wall-topology-d
ependent parameters. The computational effort is still comparable to that f
or the 'basic model'. The new term-by-term model of the <(theta u(i))over b
ar> and <(theta(2))over bar> equations was then used for a full simulation
in conjunction with a low-Reynolds-number second-moment velocity closure, w
hich was earlier found to reproduce satisfactorily a variety of isothermal
wall flows. Despite excellent term-by-term reproduction of thermal turbulen
ce, the predictions with the full model show less satisfactory agreement wi
th the DNS data than a priori validation, indicating a further need for imp
rovement of the modelling of buoyancy effects on mechanical turbulence.