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Principles of Waves, Fluids and Thermodynamics

Heat Transfer: Conduction, Convection, Radiation

Physics I 235 words Free to read

Conduction & Convection

Your skin measures heat flow, not temperature. Conduction, convection, and radiation are the three highways that flow takes. Engineering a thermos simply blocks all three.

Conduction is heat transfer via molecular collisions. Governed by Fourier's law:

dQdt=kAdTdx\frac{dQ}{dt} = -kA\frac{dT}{dx}

Where kk is thermal conductivity in W/(mK)W/(m \cdot K), AA is area, and dTdx\frac{dT}{dx} is the temperature gradient.

For a slab of thickness LL, we define thermal resistance:

Rth=LkA,dQdt=ΔTRthR_{\text{th}} = \frac{L}{kA}, \quad \frac{dQ}{dt} = \frac{\Delta T}{R_{\text{th}}}

Convection is heat carried by fluid motion. Governed by Newton's law of cooling:

dQdt=hA(TsT)\frac{dQ}{dt} = hA(T_s - T_\infty)

Where hh is the convective heat transfer coefficient, TsT_s is surface temperature, and TT_\infty is fluid temperature.

Radiation & Thermal Rules

Radiation emits thermal energy via electromagnetic waves. Governed by the Stefan-Boltzmann law:

P=εσAT4P = \varepsilon\sigma A T^4

SymbolConstant / MeaningValue
σ\sigmaStefan-Boltzmann constant5.67×1085.67\times 10^{-8} W/(m2K4m^2 K^4)
ε\varepsilonEmissivity00 (reflector) to 11 (blackbody)

Wien's displacement law finds the peak wavelength of blackbody radiation:

λmaxT=2.898×103  m K\lambda_{\max} T = 2.898\times 10^{-3}\;\text{m K}

Physics link: The Sun (57785778 K) peaks at 500\approx 500 nm (visible). The Earth (288288 K) peaks at 10μ\approx 10\,\mum (infrared).
Common pitfall: "Cold" does not flow into you. Heat always flows out from hot to cold; reversing this direction causes sign errors.
Placeholder: Heat Transfer: Conduction, Convection, Radiation

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Principles of Waves, Fluids and Thermodynamics