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
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Definition: Heat transfer is energy transfer due to temperature difference.
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Applications: Boilers, heat exchangers, turbines, refrigerators
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Key Concepts:
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Temperature gradient drives heat transfer
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Modes: Conduction, Convection, Radiation
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🔹 2. Conduction
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Definition: Heat transfer through solid or stationary fluid due to temperature gradient
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Fourier’s Law:
q=−kdTdxq = -k \frac{dT}{dx}
Where: k = thermal conductivity, dT/dx = temperature gradient
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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
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Definition: Heat transfer by fluid motion
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Newton’s Law of Cooling:
q=hA(Ts−T∞)q = h A (T_s – T_\infty)
Where: h = convective heat transfer coefficient
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Types:
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Natural Convection: Fluid motion due to buoyancy
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Forced Convection: Fluid motion forced by pump/fan
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🔹 4. Radiation
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Definition: Heat transfer by electromagnetic waves without medium
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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
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Example: Black body, T_s = 500 K, T∞ = 300 K → q?
🔹 5. Solved Examples (PYQ Style)
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Heat conduction through composite wall
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Convection from flat plate in air
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Radiation heat loss from furnace wall
🔹 6. Practice Exercises
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Compute heat flux in conduction, convection, and radiation
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Determine convective coefficient from experimental data
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Compare conduction, convection, and radiation in practical systems
🔹 7. Summary
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Conduction: Through stationary medium, Fourier’s Law
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Convection: Fluid motion, Newton’s Law of Cooling
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Radiation: Electromagnetic waves, Stefan–Boltzmann Law
