22-Mec-A1 Applied Thermodynamics and Heat Transfer · May 2014
Question 7 of 8: Vertical Power-Amplifier Plate — Convection and Radiation
Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)
Notes on this paper
Paper: National Examinations — 07-Mec-A1 Applied Thermodynamics and Heat Transfer, May 2014. Open-book, 3-hour paper. Part A (Thermodynamics, Q1–Q4) and Part B (Heat Transfer, Q5–Q8); a complete paper is any five questions — three from one part and two from the other, all of equal value. Full worked solutions to all eight questions are given below.
Reference texts: Çengel & Boles, Thermodynamics: An Engineering Approach (9th ed., McGraw-Hill) — closed- and open-system energy balances, steam tables, gas power cycles, reciprocating compressors and vapour-compression refrigeration; Çengel & Ghajar, Heat and Mass Transfer (6th ed.) and Incropera, DeWitt, Bergman & Lavine, Fundamentals of Heat and Mass Transfer (8th ed., Wiley) — composite-wall conduction, internal-flow and cross-flow convection correlations, natural convection with radiation, and the ε–NTU heat-exchanger method. Freon-12 property data are taken from the appendix supplied with the exam; steam and air data from standard tables.
Given. Vertical plate, height $L=0.040\ \text{m}$, width $0.050\ \text{m}$; both faces exposed, so surface area $A=2(0.040\times0.050)=4.0\times10^{-3}\ \text{m}^2$; $\varepsilon=0.82$; ambient/surroundings $T_\infty=25\ ^\circ\text{C}=298.15\ \text{K}$; dissipation $Q=7\ \text{W}$.
Find. The steady surface temperature $T_s$ with combined free convection and radiation.
Approach. Write the surface energy balance $Q=Q_\text{conv}+Q_\text{rad}$, with the free-convection coefficient from the Churchill–Chu vertical-plate correlation (evaluated at the film temperature) and radiation to large surroundings; solve iteratively for $T_s$.
Energy balance. $$Q=\bar h A(T_s-T_\infty)+\varepsilon\sigma A\!\left(T_s^4-T_\infty^4\right)=7\ \text{W}.$$
Free-convection coefficient (Churchill–Chu). With $L=0.04\ \text{m}$ and film properties, the Rayleigh number is $\text{Ra}_L=g\beta(T_s-T_\infty)L^3/(\nu\alpha)$, and$$\text{Nu}_L=\left\{0.68+\frac{0.670\,\text{Ra}_L^{1/4}}{\left[1+(0.492/\text{Pr})^{9/16}\right]^{4/9}}\right\},\quad \bar h=\frac{\text{Nu}_L k}{L}.$$
Iterate. Converging on $T_s\approx125\ ^\circ\text{C}$ (398 K): film ≈ 75 °C gives $\text{Ra}_L\approx2.9\times10^5$, $\text{Nu}_L\approx12.6$, $\bar h\approx9.4\ \text{W/m}^2\text{K}$.$$Q_\text{conv}=9.4(4.0\times10^{-3})(100)=3.8\ \text{W},\quad Q_\text{rad}=0.82(5.67\times10^{-8})(4.0\times10^{-3})(398^4-298^4)=3.2\ \text{W}.$$ Their sum is 7.0 W, so$$\boxed{T_s\approx125\ ^\circ\text{C}}.$$
Check
Both faces of the thin plate are assumed active for convection and radiation ($A=2LW=40\ \text{cm}^2$); if only one face dissipated, $T_s$ would be markedly higher. Convection (3.8 W) and radiation (3.2 W) carry comparable shares, so the emissivity matters — neglecting radiation would over-predict $T_s$ by tens of degrees. Laminar free convection ($\text{Ra}_L<10^9$) is confirmed.