where g is gravitational acceleration and is density. Further suppose that this density contrast is solely due to a contrast between its temperature and the surroundings:
where is the thermal expansion coefficient and T is temperature. Because the parcel is less dense than its surroundings, it will tend to move upwards. A viscous force:
will act against the buoyancy force. In this expression µ is viscosity, z is the vertical spatial coordinate, and t is time. When these two forces balance:
In addition, the parcel will be losing heat to its new surroundings by conduction, thereby reducing its temperature. The rate at which heat is lost will be proportional to the surface area of the parcel. Thus temperature (and so the density term) is a function of time:
where is the thermal conductivity. Combining 8-3, 8-5 and 8-6 and rearranging:
How far can the parcel move in infinite time? We integrate from zero to infinity:
to find that the distance traversed, z, is:
The terms in the numerator of equation 8-9 have their origin in the buoyancy force and promote upward motion while increasing either viscosity or thermal conductivity in the denominator limits upward motion.
To be able to convect heat, there must be movement across the distance between the two plates separated by a distance h in finite time and so:
By scaling the fluid parcel to the plate separation, through an arbitrary factor f:
substituting into equation 8-10 and rearranging it follows that:
The left hand side of equation 8-12 is called the Rayleigh number:
Lord Rayleigh showed through linear perturbation analysis (for a general discussion see (13), section 7.1.2 or the derivation in (11), section 6-18), that for thermal instabilities to grow in a fluid, the Rayleigh number would have to exceed a critical value (the f scale on the right hand side). When:
the temperature profiles between the two plates will be conductive, while when:
a cellular convection will be established, displacing the isotherms upward in the zone of rising fluid and downward in the zone of downwelling. The value of the critical Rayleigh number depends on the particular geometry and boundary conditions. For convection between parallel plates it lies between 657 (free boundaries) and 1708 (rigid boundaries).
This example is for water convecting between two rigid boundaries for Ra~3000. The temperature field exhibits two narrow boundary layers, with convective stirring between. This temperature distribution is reflected in the velocity field, with sluggish flow at the boundaries and in the interiors of the two cells, strong downwelling at the side boundaries, and strong upwelling in the middle of the domain:
Figure 8-2. Temperature field for a system with Ra~3000.
Figure 8-3. Velocity field for a system with Ra~3000.
(Here the viscosity and density term have been replaced with the kinematic viscosity.). For some representative values
the Rayleigh number is about 10--far in excess of the critical value.
|Oceanography 540 Pages|
Pages Maintained by Russ McDuff (email@example.com)
Copyright (©) 1994-2002 Russell E. McDuff and G. Ross Heath; Copyright Notice
Content Last Modified 10/16/2002 | Page Last Built 10/16/2002