Introduction & Context
In process engineering, the convective heat transfer coefficient h is a critical parameter for designing heat exchangers, reactors, and piping systems. Because h is not a fundamental property of a fluid, it must be determined through empirical correlations that relate the flow regime to the thermal boundary layer. Dimensionless groups—specifically the Reynolds (Re), Prandtl (Pr), and Nusselt (Nu) numbers—provide a generalized framework to calculate this coefficient across different scales and fluid types.
This calculation is typically used in the design phase of thermal systems to ensure that heat transfer rates meet process requirements while maintaining flow within desired regimes (e.g., ensuring turbulent flow for enhanced mixing and heat transfer). It is specifically applicable to steady, fully developed internal pipe flow. For the Dittus-Boelter correlation, fluid properties in the Reynolds and Prandtl numbers are evaluated at the bulk fluid temperature \(T_{b}\). The film temperature \(T_{f}\) is introduced for evaluating fluid properties used in the Grashof number calculation when assessing buoyancy effects.
Methodology & Formulas
The calculation follows a systematic approach to characterize the fluid flow and heat transfer regime. First, the film temperature is determined as the arithmetic mean of the bulk fluid temperature and the pipe wall temperature. This temperature is used for evaluating fluid properties in the Grashof number:
\[ T_{f} = \frac{T_{b} + T_{s}}{2} \]The flow regime is characterized by the Reynolds number, which represents the ratio of inertial forces to viscous forces. All fluid properties in this expression are evaluated at the bulk temperature \(T_{b}\):
\[ Re = \frac{\rho \cdot V \cdot D}{\mu} \]The Prandtl number represents the ratio of momentum diffusivity to thermal diffusivity, characterizing the relationship between the velocity and thermal boundary layers. Fluid properties are evaluated at the bulk temperature \(T_{b}\):
\[ Pr = \frac{\mu \cdot C_{p}}{k} \]For turbulent forced convection, the Nusselt number is calculated using the Dittus‑Boelter correlation for turbulent flow in pipes. This empirical relation is valid for heating or cooling scenarios, with the exponent n adjusted accordingly ( n = 0.4 for heating where \(T_{s} > T_{b}\), n = 0.3 for cooling where \(T_{s} < T_{b}\)).
\[ Nu = 0.023 \cdot Re^{0.8} \cdot Pr^{n} \]Once the Nusselt number is determined, the convective heat transfer coefficient h is derived from the definition of the Nusselt number:
\[ h = \frac{Nu \cdot k}{D} \]To assess the influence of natural convection (buoyancy) on the forced flow, the Grashof number is calculated. All fluid properties in the Grashof number are evaluated at the film temperature \(T_{f}\), and the temperature difference is defined as \(\Delta T = |T_{s} - T_{b}|\):
\[ Gr = \frac{g \cdot \beta \cdot \Delta T \cdot D^{3} \cdot \rho^{2}}{\mu^{2}} \]For ideal gases, the volumetric thermal expansion coefficient is \(\beta = 1 / T_{f}\) where \(T_{f}\) is expressed in absolute units (Kelvin or Rankine). For liquids, \(\beta\) must be obtained from property tables at the film temperature.
| Parameter | Condition / Threshold | Regime / Validity |
|---|---|---|
| Reynolds Number (Re) | Re ≥ 10,000 | Turbulent Flow (Dittus-Boelter valid) |
| Prandtl Number (Pr) | 0.6 ≤ Pr ≤ 160 | Dittus-Boelter valid range |
| Length-to-Diameter (L/D) | L/D ≥ 10 | Fully developed flow assumption |
| Buoyancy Ratio (Gr/Re2) | Gr/Re2 < 0.1 | Pure forced convection (negligible buoyancy) |