Convective heat transfer
Combine convection on both sides of a wall with conduction through it using a thermal-resistance network.
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ContinueThis page gives the UY1 working model/result for Convective Heat Transfer. You reuse it when you turn thermal intuition into calculable models (energy balances, process reasoning, and kinetic/statistical links), with careful sign/units checks.
- Module path: Thermodynamics (UY1)
- Full routing: UY1 assessment map
- Math toolkit: Mathematics for undergraduate physics
At a glance
- Prerequisites: convection law, slab conduction, steady-state energy balance.
- Outcomes: solve coupled convection-conduction-convection problems.
- Key result: resistances in series give one heat rate through all layers.
- Common trap: assuming wall-surface temperatures equal fluid temperatures.
Setup
Plane wall of thickness L and conductivity k separates two fluids:
- Inside fluid: T_(∞,in), convection coefficient hᵢₙ.
- Outside fluid: T_(∞,out), convection coefficient hₒᵤₜ.
- Wall area A.
At steady state:
Physical interpretation:
- Convection “drops” temperature between the bulk fluid and the wall surface; conduction “drops” temperature through the solid wall.
- The resistance network enforces a single heat-current through all series elements, and the largest resistance sets the bottleneck.
Core derivation / explanation
Thermal resistance network:
Total resistance:
Heat-transfer rate:
Surface temperatures follow from temperature drops:
Bridge note:
- This is the UY1 upgrade from separate conduction/convection formulas to one coupled model.
- Don’t assume wall-surface temperatures equal fluid temperatures; the convection resistances create boundary temperature drops. - Keep Q dot (W) vs q'' = Q dot/A (W m⁻²) consistent. Many textbook examples silently use A = 1. - If radiation is significant, add a radiative element (exact εσ A(T⁴-Tₛᵤᵣ⁴) or a linearized hᵣ) from UY1: Radiation.
Units check:
Physical sanity check:
- If k → ∞, wall resistance vanishes and convection dominates.
- If either h is very small, that side becomes the bottleneck.
Heat loss through a window
Worked example 1
Window thermal resistance
Problem
Find the steady heat rate and heat flux through a 1.0 m² glass window with the following data. Neglect edge losses and radiation.
- T_(∞,in) = 25°C, T_(∞,out) = -15°C.
- L = 2.0 mm = 0.002 m.
- k = 1.05 W m⁻¹K⁻¹ (glass).
- hᵢₙ = 8 W m⁻²K⁻¹, hₒᵤₜ = 20 W m⁻²K⁻¹.
- A = 1.0 m².
Show full solution
Add the three resistances
Method
Calculate both convection resistances and the glass conduction resistance, then add them.Reason
The same steady heat rate crosses each series element; their temperature drops add to the bulk-fluid temperature difference.Working
Answer
Rᵢₙ = 0.125, R_wall = 0.00190, Rₒᵤₜ = 0.050 K W⁻¹.Total Rₜₒₜ = 0.1769 K W⁻¹.
Calculate the rate and flux
Working
Answer
Q dot = (40 K)/(0.1769 K W⁻¹) ≈ 226 W, q'' = (Q dot)/A ≈ 226 W m⁻².Heat flows outward. The rate and flux have equal numerical values here only because A = 1.0 m². Convection accounts for most of the resistance.
Practice set
Check your understanding 1
For the window above, how much does the steady heat rate change if glass thickness doubles while all other data stay fixed?
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Check your understanding 2
For the original window, what happens to heat loss if wind raises hₒᵤₜ from 20 to 40 W m⁻²K⁻¹ with other data fixed?
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Check your understanding 3
Why are the inner and outer glass-surface temperatures different when heat flows through the window?
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Summary + next steps
- Coupled heat-transfer problems are best solved with resistance networks.
- At steady state, one heat rate flows through all series elements.
- Identifying the largest resistance reveals the dominant bottleneck.
Next steps:
- Add radiative resistance ideas from UY1: radiation when surfaces are hot.
- Revisit the component laws: UY1: conduction and UY1: convection.
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Syllabus and review details
No official syllabus alignment is listed for this lesson.