Tb. Larsen et al., DYNAMICS OF THERMAL-CONVECTION WITH NEWTONIAN TEMPERATURE-DEPENDENT VISCOSITY AT HIGH RAYLEIGH NUMBER, Physics of the earth and planetary interiors, 89(1-2), 1995, pp. 9-33
Two-dimensional, time-dependent convection with a Newtonian temperatur
e-dependent viscosity has been investigated in wide aspect-ratio boxes
. Large-scale circulations have been found in the regime with volumetr
ically averaged Rayleigh numbers, Ra-v ranging between O(10(5)) and O(
10(8)). Viscosity contrasts up to 1000 have been examined. The horizon
tally averaged temperature in the interior, [T](1/2), does not vary mu
ch within the above range of Ra-v for large-aspect-ratio boxes. The ho
rizontal Fourier spectra of the viscosity field show a decrease of mag
nitude in the viscosity with shorter wavelength. The viscosity spectra
decay differently with decreasing wavelength than the corresponding t
hermal spectra. Lithospheric processes, such as lubrication of subduct
ion and lithospheric thinning, are facilitated by high Ra-v. The verti
cal correlation function for the temperature anomalies used recently f
or comparing convection calculations with tomographic models is found
to be strongly time-dependent for Ra-v O(10(6)). The temporal fluctuat
ions of the vertical correlation function decrease for higher Rayleigh
numbers. Correlation functions for low Ra are broad and smooth, while
those for high Ra, greater than 10(7), are narrow and fragmented.