Abstract
We studied numerically the heat transfer for a turbulent flow of supercritical helium. A finite difference model is constructed with three different models of turbulence: the mixing length,k- andk-ε model. The stationary results compared to experimental data reveal that the mixing length model gives the best prediction of turbulence in this situation. A severe deterioration from the widely used Nusselt correlation by Giarratano is observed for cases near the pseudocritical temperature, while a far better correspondance is found with the more recent Yaskin correlation. The maxima and minima in the heat transfer curves can be understood by interpretation of the wall and bulk temperature together with the strong changes in density.
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Abbreviations
- A μ :
-
constant ink-model
- A + :
-
constant in van Driest hypothesis
- C D :
-
Constant ink/k-ε model
- Cp :
-
Specific heat J/kgK
- C 1 :
-
Constant ink-ε model
- C 2 :
-
Constant ink-ε model
- C μ :
-
Constant inμ t expression
- D :
-
Pipe diameter m
- G :
-
Mass flow kg/m2 s
- Gr:
-
Grashoff number Δρ kg/m2s
- h :
-
heat transfer coefficient W/m2K
- H :
-
Enthalpy J/kg
- k :
-
Kinetic energy of turbulence (m/s)2
- l m :
-
Mixing length
- Nu:
-
Nusselt numbrhD/λ
- P :
-
Pressure N/m2 atm
- Pr:
-
Prandtl number μ/Cpλ
- q :
-
Heat flux W/m2
- r :
-
radial coordinate m
- R :
-
Pipe radius m
- Re:
-
Reynolds number ρvD/μ
- Re k :
-
Turbulent reynolds number ρyk 1/2/μ
- T :
-
Temperature K
- T b :
-
Bulk temperature K
- T w :
-
Wall temperature K
- u :
-
Velocity component m/s
- u + :
-
Dimensionless velocityu(τ w/ρ)−1/2
- u ++ :
-
Dimensionless velocity
- v :
-
Velocity component/vector m/s
- Vz:
-
Axial velocity component m/s
- Vr:
-
Radial velocity component m/s
- x :
-
Coordinate m
- y :
-
Distance from wall m
- y + :
-
Dimensionless distance from wally(τ w ρ)1/2/μ
- y ++ :
-
Dimensionless distance from wall
- z :
-
axial coordinate m
- β:
-
compressibility −(1/ρ)(∂ρ/ϖT) 1/K
- ρ:
-
Density kg/m3
- λ:
-
thermal conductivity W/mK
- ϕ:
-
Correlating factorqD 0.2/G 0.8
- σ k :
-
Constant ink/k-ε model
- σ∈ :
-
Constant ink-ε model
- ε:
-
Dissipation of turbulence-energy
- μ:
-
Laminar viscosity kg/ms
- μ t :
-
Turbulent viscosity kg/ms
- μ eff :
-
μ+μt
- τ w :
-
Wall shear stress N/m2
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Cornelissen, M.C.M., Hoogendoorn, C.J. Forced convection heat transfer to supercritical helium. Appl. Sci. Res. 42, 161–183 (1985). https://doi.org/10.1007/BF02421348
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DOI: https://doi.org/10.1007/BF02421348