Numerical experiments are carried out to study the effects of continents on
the structure of thermal convection in the mantle. The mantle is modelled
by a viscous fluid occupying a horizontally extended rectangular 2-D region
of aspect ratio 10:1. Continents are treated as thick rigid heat-conductin
g plates placed in the mantle, with free-slip and with no-slip conditions.
Continents restrict the heat release from the underlying mantle; the mantle
material heats up and becomes lighter; as a result, a hot upwelling flow r
eplaces downwelling. We calculate the characteristic time tau of this restr
ucturing for various values of model parameters and obtain analytical appro
ximations for tau as function of Rayleigh number Ra, plate length L, and pl
ate thickness d. For commonly accepted mean parameters of the Earth's mantl
e, giving Ra = 10(7), with continental plate thickness about 300 km and len
gth about 6000 km, the restructuring time tau is estimated as 2.10(8) a. As
the continents are not fixed, but drift, the possibility of forming an asc
ending mantle flow exists if the continent does not significantly shift dur
ing an interval of about tau relative to the mantle by more than half of it
s length. Hence, under a continent drifting relative to the mantle with spe
ed less than 1 cm/a an ascending mantle flow is expected, whereas under rap
idly moving continents such an ascending flow has not enough time to develo
p. (C) 1998 Elsevier Science Ltd. All rights reserved.