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Ahmet Çelik
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Chapter 3: One-Dimensional Steady-State Conduction

MECH302

Source files used: late Heat Transfer (05), Heat Transfer (06), Heat Transfer (07), Heat Transfer (08), Heat Transfer (09); textbook Chapter 3 as support. No worked examples are included.

1. Big Picture

Chapter 3 is where conduction becomes an engineering tool. Chapter 2 taught how to pose conduction problems with differential equations. Chapter 3 shows that many steady, one-dimensional conduction problems can be reduced to thermal resistance networks.

Biddle’s basic idea is:

Heat flow behaves like current through resistors.\boxed{\text{Heat flow behaves like current through resistors.}}

Temperature difference acts like voltage difference. Heat rate acts like current. Thermal resistance controls how much heat flows.

q˙=ΔTRtotal\dot{q}=\frac{\Delta T}{R_{\text{total}}}

This chapter also covers fins. Fins are extended surfaces used to increase convection area. Biddle motivates them with radiator/electronics examples: if you cannot change the fluid or temperature difference much, increasing surface area is often the practical engineering move.


2. Core Ideas

2.1 Resistance Method

For steady, one-dimensional conduction with no generation:

q˙=ThotTcoldR\dot{q}=\frac{T_{\text{hot}}-T_{\text{cold}}}{R}

This works because the same heat rate passes through each layer in series. If 100 W100\ \text{W} enters layer A, 100 W100\ \text{W} leaves layer A and enters layer B, assuming steady state and no generation.

Thermal resistance units:

[R]=K/W or C/W[R]=\text{K/W or }^\circ\text{C/W}

The resistance method is valid when:

  • heat flow is essentially one-dimensional,
  • steady state applies,
  • properties are constant or represented by average values,
  • no internal generation appears in the resistance segment,
  • temperatures are uniform over each surface/node.

2.2 Series and Parallel Networks

Series: same heat rate through each resistance.

Rtotal=R1+R2+R3+R_{\text{total}}=R_1+R_2+R_3+\cdots q˙=T1T2Rtotal\dot{q}=\frac{T_1-T_2}{R_{\text{total}}}

Parallel: same temperature difference across multiple paths, heat rates split.

q˙total=q1+q2+\dot{q}_{\text{total}}=q_1+q_2+\cdots 1Req=1R1+1R2+\frac{1}{R_{\text{eq}}}=\frac{1}{R_1}+\frac{1}{R_2}+\cdots

Use parallel networks when heat can take multiple paths between the same two temperature nodes.


2.3 Temperature Drop Logic

Biddle emphasizes this intuition with composite walls:

q=kdTdxq''=k\left|\frac{dT}{dx}\right|

If two materials carry the same heat flux, the material with lower kk must have a larger temperature gradient. So insulation has a large temperature drop; copper has a small temperature drop.


2.4 Overall Heat Transfer Coefficient

The overall heat transfer coefficient UU is a shorthand for a whole network of conduction and convection resistances.

q˙=UAΔT\dot{q}=UA\Delta T

But UAUA is really:

UA=1RtotalUA=\frac{1}{R_{\text{total}}}

For tubes, the chosen area matters. You may define UiU_i based on inside area or UoU_o based on outside area. The product UAUA stays tied to the same total resistance.


2.5 Thermal Contact Resistance

Real surfaces are rough. When two materials touch, microscopic air gaps may exist. Air is a poor conductor, so the interface adds resistance.

Thermal contact resistance is inserted between two material resistances:

Material A resistance → contact resistance → Material B resistance

If a problem gives contact resistance, include it in the network.


2.6 Fins / Extended Surfaces

Fins increase heat transfer by increasing surface area. They are used in radiators, electronics cooling, baseboard heaters, engine components, and many other systems.

Newton’s law says:

q˙=hA(TsT)\dot{q}=hA(T_s-T_\infty)

If hh, TsT_s, and TT_\infty are hard to change, increasing area AA is the practical option.

But fins are not isothermal. The fin is hottest near the base and cooler near the tip, so we need fin efficiency.


3. Main Governing Equations and Formulas

3.1 Plane Wall Conduction Resistance

Rcond=LkAR_{\text{cond}}=\frac{L}{kA} q˙=T1T2L/(kA)=kAT1T2L\dot{q}=\frac{T_1-T_2}{L/(kA)}=kA\frac{T_1-T_2}{L}

Use for steady 1D conduction through a flat wall.

Assumptions:

  • steady,
  • 1D,
  • constant kk,
  • no generation.

3.2 Cylindrical Wall Conduction Resistance

For radial conduction through a cylinder:

Rcond,cyl=ln(r2/r1)2πkLR_{cond,cyl}=\frac{\ln(r_2/r_1)}{2\pi kL} q˙=T1T2ln(r2/r1)/(2πkL)\dot{q}=\frac{T_1-T_2}{\ln(r_2/r_1)/(2\pi kL)}

where:

  • r1r_1: inner radius,
  • r2r_2: outer radius,
  • LL: cylinder length.

Use for pipes, tubes, cylindrical insulation, and rods with radial heat flow.


3.3 Spherical Shell Conduction Resistance

Rcond,sph=14πk(1r11r2)R_{cond,sph}=\frac{1}{4\pi k}\left(\frac{1}{r_1}-\frac{1}{r_2}\right)

Use for radial conduction through spherical shells.


3.4 Convection Resistance

Rconv=1hAR_{\text{conv}}=\frac{1}{hA} q˙=TsT1/(hA)=hA(TsT)\dot{q}=\frac{T_s-T_\infty}{1/(hA)}=hA(T_s-T_\infty)

Use when a surface exchanges heat with a fluid.

Area must match the surface where convection occurs.


3.5 Composite Wall in Series

q˙=T,1T,21h1A+LAkAA+LBkBA+1h2A\dot{q}=\frac{T_{\infty,1}-T_{\infty,2}}{\frac{1}{h_1A}+\frac{L_A}{k_AA}+\frac{L_B}{k_BA}+\frac{1}{h_2A}}

Use when fluids exist on both sides of a composite wall.


3.6 Cylindrical Tube with Inside and Outside Convection

q˙=T,iT,o1hiAi+ln(ro/ri)2πkL+1hoAo\dot{q}=\frac{T_{\infty,i}-T_{\infty,o}}{\frac{1}{h_iA_i}+\frac{\ln(r_o/r_i)}{2\pi kL}+\frac{1}{h_oA_o}}

where:

Ai=2πriL,Ao=2πroLA_i=2\pi r_iL,\qquad A_o=2\pi r_oL

Use for heat transfer through pipe/tube walls.


3.7 Overall Heat Transfer Coefficient

q˙=UAΔT\dot{q}=UA\Delta T 1UA=Rtotal\frac{1}{UA}=R_{\text{total}}

For a tube:

1UiAi=1hiAi+ln(ro/ri)2πkL+1hoAo\frac{1}{U_iA_i}=\frac{1}{h_iA_i}+\frac{\ln(r_o/r_i)}{2\pi kL}+\frac{1}{h_oA_o}

or

1UoAo=1hiAi+ln(ro/ri)2πkL+1hoAo\frac{1}{U_oA_o}=\frac{1}{h_iA_i}+\frac{\ln(r_o/r_i)}{2\pi kL}+\frac{1}{h_oA_o}

The numerical values of UiU_i and UoU_o differ because the areas differ. The total conductance UAUA represents the same total resistance.


3.8 Thermal Contact Resistance

If contact resistance per unit area is given as Rt,cR_{t,c}'':

Rt,c=Rt,cAR_{t,c}=\frac{R_{t,c}''}{A}

Temperature drop across contact:

ΔTcontact=qRt,c\Delta T_{contact}=qR_{t,c}

Use only if the problem gives or requires contact resistance.


3.9 Plane Wall with Uniform Heat Generation

For a slab of half-thickness LL, symmetry at x=0x=0, surfaces at x=±Lx=\pm L, surface temperature TsT_s:

T(x)=Ts+q˙2k(L2x2)T(x)=T_s+\frac{\dot{q}}{2k}(L^2-x^2)

Maximum temperature at the center:

Tmax=Ts+q˙L22kT_{\text{max}}=T_s+\frac{\dot{q} L^2}{2k}

Surface heat flux:

qs=q˙Lq_s''=\dot{q} L

Use for internally heated plane walls with symmetric cooling.


3.10 Solid Cylinder with Uniform Heat Generation

For a solid cylinder radius ror_o and surface temperature TsT_s:

T(r)=Ts+q˙4k(ro2r2)T(r)=T_s+\frac{\dot{q}}{4k}(r_o^2-r^2)

Maximum temperature at center:

Tmax=Ts+q˙ro24kT_{\text{max}}=T_s+\frac{\dot{q} r_o^2}{4k}

Heat generated per unit length:

q=q˙πro2q'=\dot{q}\pi r_o^2

3.11 Fin Temperature Variable

θ=TT\theta=T-T_\infty

Base excess temperature:

θb=TbT\theta_b=T_b-T_\infty

Fin parameter:

m=hPkAcm=\sqrt{\frac{hP}{kA_c}}

where:

  • PP: fin perimeter exposed to convection,
  • AcA_c: fin cross-sectional area,
  • kk: fin material conductivity,
  • hh: convection coefficient.

Fin differential equation for a uniform cross-section fin:

d2θdx2m2θ=0\frac{d^2\theta}{dx^2}-m^2\theta=0

3.12 Fin Heat Rate — Adiabatic Tip

qf=hPkAcθbtanh(mL)q_f=\sqrt{hPkA_c}\,\theta_b\tanh(mL)

Use when the fin tip is modeled as insulated or by symmetry.


3.13 Fin Heat Rate — Convective Tip

qf=Msinh(mL)+hmkcosh(mL)cosh(mL)+hmksinh(mL)q_f=M\frac{\sinh(mL)+\frac{h}{mk}\cosh(mL)}{\cosh(mL)+\frac{h}{mk}\sinh(mL)}

where:

M=hPkAcθbM=\sqrt{hPkA_c}\,\theta_b

Use when convection from the tip is included directly.


3.14 Infinite Fin Approximation

qf=hPkAcθbq_f=\sqrt{hPkA_c}\,\theta_b

Use only when the fin is long enough. Biddle corrected the criterion in lecture: do not use the transient-conduction value by mistake. The infinite-fin model is acceptable only for sufficiently large mLmL, commonly around mL2.65mL\ge 2.65 for the table criterion he used.


3.15 Corrected Length Approximation

For many straight fins:

Lc=L+AcPL_c=L+\frac{A_c}{P}

Then approximate a convective-tip fin as an adiabatic-tip fin with corrected length:

qfhPkAcθbtanh(mLc)q_f\approx\sqrt{hPkA_c}\,\theta_b\tanh(mL_c)

3.16 Fin Efficiency

ηf=qfhAfθb\eta_f=\frac{q_f}{hA_f\theta_b}

where hAfθbhA_f\theta_b is the heat transfer if the whole fin were at base temperature.


3.17 Overall Surface Efficiency

ηo=1AfAt(1ηf)\eta_o=1-\frac{A_f}{A_t}(1-\eta_f)

Total heat transfer from a finned surface:

qt=ηohAtθbq_t=\eta_o hA_t\theta_b

where:

  • AfA_f: total fin area,
  • AtA_t: total exposed area including fins and exposed base.

4. Problem-Solving Workflow

4.1 Resistance Network Problems

  1. Draw the physical heat path.
  2. Identify temperature nodes: fluid temperatures, surface temperatures, interfaces.
  3. Identify each resistance: convection, conduction, contact, radiation if included approximately.
  4. Decide series or parallel.
  5. Compute total resistance.
  6. Use q˙=ΔT/Rtotal\dot{q}=\Delta T/R_{\text{total}}.
  7. Find intermediate temperatures from ΔT=qR\Delta T=qR.
  8. Check whether heat flow direction makes sense.

4.2 Finned Surface Problems

  1. Identify fin geometry: rectangular, pin, circumferential, etc.
  2. Determine AcA_c, PP, AfA_f, and LL or LcL_c.
  3. Find material kk and convection coefficient hh.
  4. Compute m=hP/(kAc)m=\sqrt{hP/(kA_c)}.
  5. Choose tip condition: convective, adiabatic, prescribed temperature, or infinite.
  6. Compute qfq_f or ηf\eta_f.
  7. If multiple fins, combine with exposed base area using ηo\eta_o or direct summation.

5. Decision Rules / Decision Trees

5.1 Resistance Network Validity

Steady state? AND one-dimensional path? AND no internal generation in the resistance layer? AND uniform temperatures over nodes? → resistance network is appropriate.

If generation exists inside the layer: → use generation equations or differential equation, not a simple L/(kA)L/(kA) resistance alone.

5.2 Plane Wall vs Cylinder vs Sphere

Flat wall, constant area? → R=L/(kA)R=L/(kA)

Radial pipe/tube conduction? → R=ln(ro/ri)/(2πkL)R=\ln(r_o/r_i)/(2\pi kL)

Radial spherical shell? → R=(1/r11/r2)/(4πk)R=(1/r_1-1/r_2)/(4\pi k)

5.3 Series vs Parallel

Same heat rate through each layer? → series

Heat splits into multiple paths between same temperature nodes? → parallel

5.4 Fin Tip Decision

Tip convection included explicitly? → convective-tip formula

Tip heat loss negligible or symmetry plane? → adiabatic-tip formula

Very long fin, mLmL sufficiently large? → infinite-fin formula

Quick engineering approximation for convective tip? → corrected length with adiabatic-tip formula


6. Important Tables / Correlations Needed

6.1 Thermal Resistances

CaseResistance
Plane wallL/(kA)L/(kA)
Cylinderln(r2/r1)/(2πkL)\ln(r_2/r_1)/(2\pi kL)
Sphere(1/r11/r2)/(4πk)(1/r_1-1/r_2)/(4\pi k)
Convection1/(hA)1/(hA)
ContactRt,c/AR_{t,c}''/A

6.2 Fin Geometry Quantities

Fin TypeAcA_cPP
Rectangular fin, width ww, thickness ttwtwtapproximately 2(w+t)2(w+t)
Circular pin fin, diameter DDπD2/4\pi D^2/4πD\pi D

Use the actual geometry stated in the problem.


7. Key Takeaways

  • Thermal resistance networks are the main tool for steady 1D conduction.
  • Same heat rate flows through series resistances.
  • Temperature drops are larger across larger resistances.
  • Low-kk materials produce large temperature gradients.
  • For cylinders, area changes with radius, so the resistance is logarithmic.
  • UU is just shorthand for all resistances combined.
  • Contact resistance can matter when surfaces are rough or poorly bonded.
  • Fins increase area but are not isothermal.
  • Fin efficiency tells how effectively the fin area is used.
  • Always check whether the infinite-fin approximation is valid before using it.