Heat Transfer: Conduction, Convection, Radiation

Interactive Lecture

Conduction, Convection, and Radiation Heat Transfer

by Dr Arnaldo Delli Carri

Understanding Heat Transfer

Heat transfer is the movement of thermal energy from one object or material to another due to a temperature difference. It is a fundamental concept in engineering, governing everything from building insulation to electronic cooling systems. Heat naturally flows from regions of higher temperature to regions of lower temperature until thermal equilibrium is reached.

Heat moves by three mechanisms — conduction (direct contact), convection (fluid motion), and radiation (electromagnetic waves). Most engineering problems combine two or three of them at once.

Mode 1: Conduction

Conduction is heat transfer through a solid material or between materials in direct contact. It occurs when faster-moving molecules (at higher temperature) collide with slower-moving molecules (at lower temperature), transferring kinetic energy.

Fourier's Law of Heat Conduction:

\[Q = -kA\frac{dT}{dx}\]

For steady-state conduction through a plane wall:

\[Q = \frac{kA(T_1 - T_2)}{L}\]

Where:

Dividing through by area gives the heat flux, the heat rate per unit area:

\[q = \frac{Q}{A} \text{ (W/m}^2\text{)}\]

Thermal Conductivity: Different materials have vastly different thermal conductivities:

Thermal Resistance (Conduction):

\[R_{cond} = \frac{L}{kA}\]

Using thermal resistance analogy (similar to electrical resistance):

\[Q = \frac{\Delta T}{R_{total}}\]

Mode 2: Convection

Convection is heat transfer between a solid surface and a moving fluid (liquid or gas). It combines conduction within the fluid and the bulk motion of the fluid.

Newton's Law of Cooling:

\[Q = hA(T_s - T_\infty)\]

Where:

Types of Convection:

Thermal Resistance (Convection):

\[R_{conv} = \frac{1}{hA}\]

Mode 3: Radiation

Radiation is heat transfer through electromagnetic waves, requiring no medium. All objects emit thermal radiation proportional to the fourth power of their absolute temperature.

Stefan-Boltzmann Law:

\[Q = \varepsilon \sigma A T^4\]

For radiation exchange between two surfaces:

\[Q = \varepsilon \sigma A (T_A^4 - T_B^4)\]

Where:

Emissivity Values:

Combined Heat Transfer

In most engineering applications, heat transfer occurs through multiple modes simultaneously. For example, heat loss from a building involves conduction through the wall, convection at the surfaces, and possibly radiation.

Overall Heat Transfer Coefficient:

For a composite wall with convection at both surfaces:

\[Q = UA\Delta T\]

Where \(U\) is the overall heat transfer coefficient:

\[\frac{1}{UA} = R_{total} = R_{conv,1} + R_{cond,1} + R_{cond,2} + \cdots + R_{conv,2}\]

\[\frac{1}{U} = \frac{1}{h_1} + \frac{L_1}{k_1} + \frac{L_2}{k_2} + \cdots + \frac{1}{h_2}\]

Interactive Simulation: Heat Transfer Through a Wall

Explore how different materials, thicknesses, and boundary conditions affect heat transfer. Observe temperature distribution and heat flux through a composite wall.

In "All Three Modes", the sim treats the combined conduction/convection path and the radiation path as parallel routes between the same two boundary temperatures: \(Q_{total} = Q_{cond+conv} + Q_{rad}\), each driven by the full \(\Delta T\). The infobox reports an equivalent resistance \(R = \Delta T / Q_{total}\) — a lumped value, not a series network with a separate radiation resistance.

80 °C
20 °C
20 cm
0.50 W/m·K
150 150 0.40 60

Engineering Applications

Summary of Key Equations

Concept Equation Description
Fourier's Law (Conduction) \(Q = -kA\frac{dT}{dx}\) Heat conduction rate
Conduction (Plane Wall) \(Q = \frac{kA(T_1 - T_2)}{L}\) Steady-state heat transfer through wall
Thermal Resistance (Cond.) \(R_{cond} = \frac{L}{kA}\) Conduction thermal resistance
Newton's Law of Cooling \(Q = hA(T_s - T_\infty)\) Convective heat transfer
Thermal Resistance (Conv.) \(R_{conv} = \frac{1}{hA}\) Convection thermal resistance
Stefan-Boltzmann Law \(Q = \varepsilon\sigma A(T_A^4 - T_B^4)\) Radiation heat transfer
Overall Heat Transfer \(Q = UA\Delta T\) Combined heat transfer modes
Overall HT Coefficient \(\frac{1}{U} = \frac{1}{h_1} + \frac{L_1}{k_1} + \frac{L_2}{k_2} + \cdots + \frac{1}{h_2}\) Series thermal resistances (multi-layer)
Thermal Diffusivity \(\alpha = \frac{k}{\rho c_p}\) Rate of temperature change
Biot Number \(Bi = \frac{hL_c}{k}\) Ratio of internal to surface resistance

Practice Problems

Problem 1: Heat Conduction Through a Wall

A concrete wall (k = 1.4 W/m·K) is 20 cm thick. The inside surface temperature is 25°C and the outside surface temperature is 5°C. Calculate:

  1. The heat flux through the wall (W/m²)
  2. The heat transfer rate for a wall area of 15 m²

Show Solution

Problem 2: Convection Heat Transfer

A hot plate at 150°C is cooled by air at 25°C flowing over it. The convection heat transfer coefficient is h = 20 W/m²·K. If the plate area is 0.5 m², calculate:

  1. The heat transfer rate from the plate
  2. The convective thermal resistance

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Problem 3: Composite Wall with Convection

A composite wall consists of:

Inside convection: h₁ = 10 W/m²·K, T∞,1 = 22°C

Outside convection: h₂ = 25 W/m²·K, T∞,2 = -5°C

Calculate:

  1. The overall heat transfer coefficient U
  2. The heat flux through the wall
  3. The interface temperature between the two layers

Show Solution

Problem 4: Radiative Heat Loss

A radiator surface at 80°C (ε = 0.9, A = 2 m²) radiates to surroundings at 20°C. Calculate the net radiative heat transfer rate.

Show Solution

Knowledge Check Quiz

Question 1: Which mode of heat transfer requires a physical medium?

Question 2: According to Fourier's law, heat flux is proportional to:

Question 3: Which material would be best for insulation?

Question 4: In the Stefan-Boltzmann law, heat transfer by radiation is proportional to:

Question 5: Forced convection differs from natural convection in that: