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Governing Equations for Rayleigh-Bénard Convection (NOB) - Part 1


Basic Laws

The three major dynamical law governing Rayleigh-Bénard convection are, namely, the

These laws describe the conservation of mass (or volume for incompressible flows), momentum and energy in continuum mechanics.  
 
The relevant dimensional non-Oberbeck-Bousinessq Rayleigh-Bénard is then formulated by assuming:

Non-dimensionalisation of the non-Oberbeck Rayleigh-Bénard equations will be detailed in Part 2.  
 
Also see sources for detailed derivation.


Continuity Equation

For incompressible flows,

·u=0

 


Equations of Motion

  1. Incompressible Navier-Stokes in conservative form
uit+ujuixj=1ρPxi+ν(T)2uixjxj+fi
  1. More succinctly:
Dtu=1ρP+·[ν(u+(u)T)]+F
  1. A multitude of body forces can be included depending on the nature of the problem. For a simple, rotating NOB Rayleigh-Bénard problem (see 1):
    1. Buoyancy force: $- \rho \boldsymbol{g} \alpha \Delta $
    2. Coriolis force: 2Ω×u  
       

Energy equation

Internal energy equation (see 2):

ρCpDtT=·(kT)+βTDtP+τ:u+Q τ:u=[τ11τ12τ13τ21τ22τ23τ31τ32τ33]u

Equation simplifies to:

ρCpDtT=·(CpρκT)

And thus:

Dt=·[κT]

 
 


References

  1. P. A. Davidson, Turbulence in Rotating, Stratified and Electrically Conducting Fluids. Cambridge: Cambridge University Press, 2013.

  2. Ronald L. Panton. Incompressible Flow. John Wiley Sons, Ltd, 2013.

#NOB #RBC