5.3 Thermal Radiation & Industrial Heat Exchanger Design

Key Takeaways

  • Stefan-Boltzmann law states blackbody emissive power is Eb = sigma * T^4 (sigma = 5.670374 x 10^-8 W/m²·K^4), requiring absolute temperatures in Kelvin.
  • Wien's Displacement Law dictates peak spectral emission wavelength lambda_max * T = 2897.8 micrometer·K.
  • Radiative exchange between diffuse-gray surfaces uses view factors F_ij governed by reciprocity (A_i F_ij = A_j F_ji) and summation (sum F_ij = 1) rules.
  • Inserting N radiation shields of identical emissivity between parallel plates reduces net radiative heat transfer by a factor of 1 / (N + 1).
  • Industrial heat exchangers are analyzed using the Logarithmic Mean Temperature Difference (LMTD) method (q = U A F DeltaT_lm) when fluid temperatures are known, or Effectiveness-NTU (epsilon-NTU) method when outlet temperatures are unknown.
Last updated: July 2026

5.3 Thermal Radiation & Industrial Heat Exchanger Design

Thermal radiation is the electromagnetic energy emitted by matter as a result of its finite temperature. Unlike conduction and convection, radiation requires no intervening medium and travels at the speed of light in a vacuum ($c_0 \approx 3 \times 10^8\text{ m/s}$).


1. Fundamentals of Thermal Radiation & Blackbody Laws

Blackbody Radiation

A blackbody is an idealized physical body that absorbs all incident electromagnetic radiation, regardless of wavelength or direction, and emits the maximum possible thermal radiation at a given temperature.

  • Stefan-Boltzmann Law: Total emissive power of a blackbody $E_b$ is proportional to the fourth power of its absolute temperature:

Eb=σT4[W/m2]E_b = \sigma T^4 \quad [\text{W/m}^2]

Where:

  • $\sigma = 5.670374 \times 10^{-8} \text{ W/m}^2\cdot\text{K}^4$ = Stefan-Boltzmann Constant

  • $T$ = Absolute temperature of the surface in Kelvin ($\text{K} = ^\circ\text{C} + 273.15$)

  • Wien's Displacement Law: The wavelength $\lambda_{max}$ at which blackbody spectral emissive power is maximum is inversely proportional to absolute temperature:

λmaxT=2897.8[μmK]\lambda_{max} T = 2897.8 \quad [\mu\text{m}\cdot\text{K}]

Example: The sun ($T \approx 5800\text{ K}$) has peak emission at $\lambda_{max} \approx 0.5\mu\text{m}$ (visible green-yellow light), while a surface at $300\text{ K}$ peaks at $\lambda_{max} \approx 9.66\mu\text{m}$ (infrared spectrum).

Real Surface Properties & Kirchhoff's Law

Real surfaces emit and reflect less radiation than a blackbody:

  • Emissivity ($\epsilon$): $\epsilon = \frac{E(T)}{E_b(T)} \le 1.0$
  • Absorptivity ($\alpha$): Fraction of incident radiation absorbed.
  • Reflectivity ($\rho$): Fraction reflected.
  • Transmissivity ($\tau$): Fraction transmitted through medium.

For any surface, energy conservation dictates:

α+ρ+τ=1.0\alpha + \rho + \tau = 1.0

For an opaque body ($\tau = 0$), $\alpha + \rho = 1.0$.

Kirchhoff's Law of Radiation: For any surface in thermal equilibrium with its surroundings, monochromatic directional emissivity equals monochromatic directional absorptivity ($\epsilon_\lambda = \alpha_\lambda$). For a diffuse-gray surface, total emissivity equals total absorptivity ($\epsilon = \alpha$).


2. View Factor Algebra & Radiative Heat Exchange

The View Factor (or shape factor) $F_{ij}$ is defined as the fraction of radiation leaving diffuse surface $i$ that strikes diffuse surface $j$ directly.

Fundamental View Factor Relations

  1. Reciprocity Relation:

    AiFij=AjFjiA_i F_{ij} = A_j F_{ji}

  2. Summation Rule (for an enclosure of $N$ surfaces forming a complete interior space):

    j=1NFij=1.0for i=1,2,,N\sum_{j=1}^{N} F_{ij} = 1.0 \quad \text{for } i = 1, 2, \dots, N

  3. Superposition Rule: If surface $j$ is subdivided into parts $k$ and $l$ ($A_j = A_k + A_l$):

    Fi(k+l)=Fik+FilF_{i(k+l)} = F_{ik} + F_{il}

  4. Flat or Convex Surfaces: Cannot see themselves, so $F_{ii} = 0$. Concave surfaces have $F_{ii} > 0$.

Net Radiative Exchange Between Diffuse-Gray Surfaces

  • Two Infinite Parallel Plates ($ A_1 = A_2 = A$):

    q12=q12A=σ(T14T24)1ϵ1+1ϵ21q_{12}'' = \frac{q_{12}}{A} = \frac{\sigma (T_1^4 - T_2^4)}{\frac{1}{\epsilon_1} + \frac{1}{\epsilon_2} - 1}

  • Small Object 1 Enclosed by Large Surface 2 ($A_1 \ll A_2, F_{12} = 1.0$):

    q12=ϵ1A1σ(T14T24)q_{12} = \epsilon_1 A_1 \sigma (T_1^4 - T_2^4)

Radiation Shields

Radiation shields are thin, highly reflective sheets placed between radiating surfaces to reduce net radiative heat transfer. Inserting $N$ thin shields of identical emissivity $\epsilon_s$ equal to plate emissivities ($\epsilon_1 = \epsilon_2 = \epsilon_s$) reduces net heat transfer rate to:

qshielded=1N+1qunshieldedq_{shielded} = \frac{1}{N + 1} q_{unshielded}


3. Industrial Heat Exchangers & Overall Heat Transfer Coefficient ($U$)

Heat exchangers are devices that facilitate heat transfer between two fluid streams at different temperatures without mixing them.

Primary Heat Exchanger Configurations

  1. Double-Pipe (Concentric Tube):
    • Parallel-Flow: Both hot and cold fluids enter at the same end and flow in the same direction.
    • Counter-Flow: Hot and cold fluids enter at opposite ends and flow in opposite directions. (Produces higher outlet cold fluid temperature and larger average temperature difference).
  2. Shell-and-Tube: Most common industrial type; contains a bundle of tubes inside a outer shell equipped with baffles (1-shell pass, 2-tube pass; 2-shell pass, 4-tube pass).
  3. Cross-Flow: Fluids flow perpendicular to each other (e.g., automobile radiator); streams can be unmixed or mixed.

Overall Heat Transfer Coefficient ($U$)

The thermal resistance across a clean tubular heat exchanger wall is:

1UA=1UiAi=1UoAo=1hiAi+Rf,i1Ai+ln(ro/ri)2πkL+Rf,o1Ao+1hoAo\frac{1}{U A} = \frac{1}{U_i A_i} = \frac{1}{U_o A_o} = \frac{1}{h_i A_i} + R_{f,i}'' \frac{1}{A_i} + \frac{\ln(r_o/r_i)}{2 \pi k L} + R_{f,o}'' \frac{1}{A_o} + \frac{1}{h_o A_o}

Where $R_f''$ represents fouling factors ($\text{m}^2\cdot\text{K/W}$) resulting from chemical deposits, rust, or biological scaling.


4. Logarithmic Mean Temperature Difference (LMTD) Method

The LMTD method is preferred for heat exchanger sizing when fluid inlet and outlet temperatures are known or specified.

q=UAFΔTlmq = U A F \Delta T_{lm}

Where:

  • $\Delta T_{lm}$ = Logarithmic Mean Temperature Difference for pure counter-flow
  • $F$ = LMTD Correction Factor ($F \le 1.0$; $F = 1.0$ for pure counter-flow or parallel-flow)

Counter-Flow LMTD Equation

ΔTlm,CF=ΔT1ΔT2ln(ΔT1/ΔT2)\Delta T_{lm,CF} = \frac{\Delta T_1 - \Delta T_2}{\ln(\Delta T_1 / \Delta T_2)}

Where:

  • $\Delta T_1 = T_{h,in} - T_{c,out}$
  • $\Delta T_2 = T_{h,out} - T_{c,in}$

(Note: If $\Delta T_1 = \Delta T_2$, then $\Delta T_{lm} = \Delta T_1$.)

Multipass LMTD Correction Factor ($F$)

For shell-and-tube or cross-flow heat exchangers, $F$ is obtained from standard charts using two dimensionless ratios:

P=touttinTintin(Thermal Effectiveness Ratio)P = \frac{t_{out} - t_{in}}{T_{in} - t_{in}} \quad \text{(Thermal Effectiveness Ratio)}

R=TinTouttouttin=m˙ccp,cm˙hcp,h=CcCh(Heat Capacity Ratio)R = \frac{T_{in} - T_{out}}{t_{out} - t_{in}} = \frac{\dot{m}_c c_{p,c}}{\dot{m}_h c_{p,h}} = \frac{C_c}{C_h} \quad \text{(Heat Capacity Ratio)}

Where $T$ refers to shell-side fluid and $t$ refers to tube-side fluid.


5. Effectiveness-NTU ($\epsilon$-NTU) Method

When fluid outlet temperatures are unknown, the LMTD method requires tedious iteration. The $\epsilon$-NTU Method directly solves performance without iteration.

Definitions

  • Heat Capacity Rates: $C_h = \dot{m}h c{p,h}$ and $C_c = \dot{m}c c{p,c}$

  • Minimum Capacity Rate: $C_{min} = \min(C_h, C_c)$

  • Capacity Ratio: $C_r = \frac{C_{min}}{C_{max}} \le 1.0$

  • Maximum Possible Heat Transfer Rate ($q_{max}$):

    qmax=Cmin(Th,inTc,in)q_{max} = C_{min} (T_{h,in} - T_{c,in})

  • Heat Exchanger Effectiveness ($\epsilon$):

    ϵ=qactualqmax=Ch(Th,inTh,out)Cmin(Th,inTc,in)=Cc(Tc,outTc,in)Cmin(Th,inTc,in)\epsilon = \frac{q_{actual}}{q_{max}} = \frac{C_h (T_{h,in} - T_{h,out})}{C_{min} (T_{h,in} - T_{c,in})} = \frac{C_c (T_{c,out} - T_{c,in})}{C_{min} (T_{h,in} - T_{c,in})}

  • Number of Transfer Units (NTU):

    NTU=UACminNTU = \frac{U A}{C_{min}}

Representative $\epsilon$-NTU Formulas

Heat Exchanger TypeEffectiveness Equation $\epsilon = f(NTU, C_r)$
Double-Pipe Counter-Flow$\epsilon = \frac{1 - \exp[-NTU (1 - C_r)]}{1 - C_r \exp[-NTU (1 - C_r)]}$ (For $C_r < 1$)
Double-Pipe Parallel-Flow$\epsilon = \frac{1 - \exp[-NTU (1 + C_r)]}{1 + C_r}$
Boiler or Condenser ($C_r = 0$)$\epsilon = 1 - \exp(-NTU)$

6. Step-by-Step Worked Engineering Calculation (MELE Board Exam Style)

Problem Statement

A double-pipe counter-flow heat exchanger is used to cool engine lube oil ($c_{p,h} = 2.10\text{ kJ/kg}\cdot\text{K}$) from $T_{h,in} = 110^\circ\text{C}$ to $T_{h,out} = 50^\circ\text{C}$ at a mass flow rate of $\dot{m}h = 1.5\text{ kg/s}$. Cooling water ($c{p,c} = 4.18\text{ kJ/kg}\cdot\text{K}$) enters the heat exchanger at $T_{c,in} = 20^\circ\text{C}$ with a mass flow rate of $\dot{m}_c = 1.2\text{ kg/s}$. The overall heat transfer coefficient is $U = 650\text{ W/m}^2\cdot\text{K}$.

  1. Calculate the total heat transfer rate $q$.
  2. Calculate the exit temperature of cooling water $T_{c,out}$.
  3. Determine the Logarithmic Mean Temperature Difference $\Delta T_{lm}$.
  4. Calculate the required heat exchanger heat transfer surface area $A$.

Solution

Step 1: Calculate Heat Transfer Rate $q$

Calculate oil heat capacity rate $C_h$: Ch=m˙hcp,h=1.5 kg/s×2100 J/kgK=3150 W/KC_h = \dot{m}_h c_{p,h} = 1.5\text{ kg/s} \times 2100\text{ J/kg}\cdot\text{K} = 3150\text{ W/K}

Calculate total heat loss rate from oil $q$: q=Ch(Th,inTh,out)=3150×(11050)=3150×60=189,000 W=189.0 kWq = C_h (T_{h,in} - T_{h,out}) = 3150 \times (110 - 50) = 3150 \times 60 = 189,000\text{ W} = 189.0\text{ kW}

Step 2: Calculate Water Exit Temperature $T_{c,out}$

Calculate water heat capacity rate $C_c$: Cc=m˙ccp,c=1.2 kg/s×4180 J/kgK=5016 W/KC_c = \dot{m}_c c_{p,c} = 1.2\text{ kg/s} \times 4180\text{ J/kg}\cdot\text{K} = 5016\text{ W/K}

Energy conservation on water side: q=Cc(Tc,outTc,in)    189,000=5016×(Tc,out20)q = C_c (T_{c,out} - T_{c,in}) \implies 189,000 = 5016 \times (T_{c,out} - 20) Tc,out20=189,0005016=37.68C    Tc,out=57.68CT_{c,out} - 20 = \frac{189,000}{5016} = 37.68^\circ\text{C} \implies T_{c,out} = 57.68^\circ\text{C}

Step 3: Calculate Logarithmic Mean Temperature Difference (LMTD)

For counter-flow arrangement: ΔT1=Th,inTc,out=11057.68=52.32C\Delta T_1 = T_{h,in} - T_{c,out} = 110 - 57.68 = 52.32^\circ\text{C} ΔT2=Th,outTc,in=5020=30.00C\Delta T_2 = T_{h,out} - T_{c,in} = 50 - 20 = 30.00^\circ\text{C}

Calculate $\Delta T_{lm}$: ΔTlm=ΔT1ΔT2ln(ΔT1/ΔT2)=52.3230.00ln(52.32/30.00)=22.32ln(1.7440)=22.320.55618=40.13C\Delta T_{lm} = \frac{\Delta T_1 - \Delta T_2}{\ln(\Delta T_1 / \Delta T_2)} = \frac{52.32 - 30.00}{\ln(52.32 / 30.00)} = \frac{22.32}{\ln(1.7440)} = \frac{22.32}{0.55618} = 40.13^\circ\text{C}

Step 4: Calculate Required Heat Exchanger Surface Area $A$

q=UAΔTlm    A=qUΔTlmq = U A \Delta T_{lm} \implies A = \frac{q}{U \Delta T_{lm}} A=189,000 W650 W/m2K×40.13 K=189,00026,084.5=7.245 m2A = \frac{189,000\text{ W}}{650\text{ W/m}^2\cdot\text{K} \times 40.13\text{ K}} = \frac{189,000}{26,084.5} = 7.245\text{ m}^2

The required surface area for the heat exchanger is $7.25\text{ m}^2$.

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Industrial Heat Exchanger Types, Flow Arrangements, and Analysis Methods
Test Your Knowledge

Two black concentric spheres have inner radius r_1 = 0.10 m (surface area A_1 = 0.1257 m²) and outer radius r_2 = 0.20 m (surface area A_2 = 0.5027 m²). What are the view factors F_12 and F_21?

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Test Your Knowledge

How many thin radiation shields of emissivity equal to the main parallel plates (epsilon_s = epsilon_1 = epsilon_2) must be placed between the two plates to reduce net radiative heat transfer by 80% (i.e., down to 20% of the unshielded rate)?

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Test Your Knowledge

In a heat exchanger with C_min = 2000 W/K and C_max = 4000 W/K (capacity ratio C_r = 0.5), hot fluid enters at 100°C and cold fluid enters at 20°C. If heat exchanger effectiveness is epsilon = 0.65, what is the actual heat transfer rate q?

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