Annular fin

Governing Equation

To derive the governing equation of an annular fin, certain assumptions must be made. The fin must have constant thermal conductivity and other material properties, there must be no internal heat generation, there must be only one-dimensional conduction, and the fin must be at steady state.

Applying the energy conservation principle to a differential element between radii r and r + Δr yields

: q(2\pi r)(2t)\Bigr|_{r}

• q(2\pi r)(2t)\Bigr|_{r+\Delta r}
• h_c (2) 2\pi r, \Delta r \left( T - T_e \right) = 0,

where the first two terms are heat transferred through conduction, while the third is heat lost due to convection with the surrounding fluid. T represents the temperature at r and Te represents the temperature of the surrounding fluid. Next, applying Fourier's law

:q = -k \frac{\partial T}{\partial r}

and dividing by 4πΔr, letting Δr → 0, yields

: \frac{\partial}{\partial r} \left( r, \frac{\partial T}{\partial r} \right)

• h_c, r, \frac{T - T_e}{k, t} =0.

Assigning new variables z

:z = r \sqrt{ \frac{h_c}{k, t} }

and θ, where Tb is the temperature at the base of the fin,

:\theta = \frac{T - T_e}{T_b - T_e}

results in the governing equation for heat transfer of an annular fin:

: z^2, \frac{\partial^2 \theta}{\partial z^2}

• z, \frac{\partial \theta}{\partial z}

• z^2, \theta =0.

Heat loss and efficiency

The maximum possible heat loss from an annular fin occurs when the fin is isothermal. This ensures that the temperature difference between the fin and the surrounding fluid is maximized at every point along the fin, increasing heat transfer by convection, and ultimately heat loss Q:

: Q = k, \left( 4 \pi r_1 t \right) \left( T_b - T_e \right) \beta \left[ C_2, K_1\left( \beta r_1 \right) - C_1, I_1\left( \beta r_1 \right) \right].

The efficiency ηf of an annular fin is the ratio of its heat loss to the heat loss of a similar isothermal fin:

: \eta_f = \frac{ \displaystyle \frac{2 r_1}{\beta}, K_1\left( \beta r_1 \right), I_1\left( \beta r_2 \right)

• I_1\left( \beta r_1 \right), K_1\left( \beta r_2 \right)} { r_2^2
• r_1^2, K_0\left( \beta r_1 \right), I_1\left( \beta r_2 \right)

•     I_0\left( \beta r_1 \right)\, K_1\left( \beta r_2 \right)}.
  

References

• {{cite book | url-access = limited