Introduction & Context

The convective heat-transfer coefficient h quantifies how effectively heat is carried away from a surface by an adjacent moving fluid. In process engineering it is the key parameter that links the driving temperature difference to the rate of heat removal, so it appears in every heat-exchanger, reactor, furnace, or cooler design calculation. A quick estimate of h is often obtained from a conductive-layer model: the fluid very close to the wall is assumed to behave as a stagnant film whose thickness δ is fixed by the flow regime; once δ is known, h follows directly from the fluid thermal conductivity k. The sheet below shows how to compute h and the resulting heat duty q for a single flat plate of length L and unit width.

Methodology & Formulas

  1. Convert the film thickness from millimetres to metres: \[ \delta = \frac{\delta_{\text{mm}}}{1000} \]
  2. Compute the convective heat-transfer coefficient: \[ h = \frac{k}{\delta} \] where k is the thermal conductivity of the fluid evaluated at the film temperature.
  3. Determine the temperature driving force: \[ \Delta T = T_{\text{plate}} - T_{\text{air}} \]
  4. Calculate the heat-transfer area (unit width): \[ A = L \cdot \text{width} \]
  5. Obtain the total heat-flow rate: \[ q = h \cdot A \cdot \Delta T \]
Flow regime Typical δ range (mm) Remarks
Laminar boundary layer 0.5 – 2 Natural or low-speed forced convection
Turbulent boundary layer 0.1 – 0.5 High-speed forced convection