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PSU & GATE Mechanical Engineering Master Course

Lesson 6.1: Modes of Heat Transfer (Conduction, Convection, Radiation)

Heat Transfer is essential in thermal engineering, power plants, and HVAC systems. GATE and PSU exams often test basic concepts, formulas, and applications.


🔹 1. Introduction

  • Definition: Heat transfer is energy transfer due to temperature difference.

  • Applications: Boilers, heat exchangers, turbines, refrigerators

  • Key Concepts:

    1. Temperature gradient drives heat transfer

    2. Modes: Conduction, Convection, Radiation


🔹 2. Conduction

  • Definition: Heat transfer through solid or stationary fluid due to temperature gradient

  • Fourier’s Law:

q=−kdTdxq = -k \frac{dT}{dx}

Where: k = thermal conductivity, dT/dx = temperature gradient

  • Example: Heat through wall of thickness 0.05 m, k = 50 W/m·K, ΔT = 100 K → q?

q=kΔTL=50∗100/0.05=100kW/m2q = k \frac{\Delta T}{L} = 50*100/0.05 = 100 kW/m^2


🔹 3. Convection

  • Definition: Heat transfer by fluid motion

  • Newton’s Law of Cooling:

q=hA(Ts−T∞)q = h A (T_s – T_\infty)

Where: h = convective heat transfer coefficient

  • Types:

    1. Natural Convection: Fluid motion due to buoyancy

    2. Forced Convection: Fluid motion forced by pump/fan


🔹 4. Radiation

  • Definition: Heat transfer by electromagnetic waves without medium

  • Stefan–Boltzmann Law:

q=ϵσA(Ts4−T∞4)q = \epsilon \sigma A (T_s^4 – T_\infty^4)

Where ε = emissivity, σ = Stefan–Boltzmann constant

  • Example: Black body, T_s = 500 K, T∞ = 300 K → q?


🔹 5. Solved Examples (PYQ Style)

  1. Heat conduction through composite wall

  2. Convection from flat plate in air

  3. Radiation heat loss from furnace wall


🔹 6. Practice Exercises

  1. Compute heat flux in conduction, convection, and radiation

  2. Determine convective coefficient from experimental data

  3. Compare conduction, convection, and radiation in practical systems


🔹 7. Summary

  • Conduction: Through stationary medium, Fourier’s Law

  • Convection: Fluid motion, Newton’s Law of Cooling

  • Radiation: Electromagnetic waves, Stefan–Boltzmann Law

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