342 RADIATIVE HEAT TRANSFER
12.4 Consider a particle cloud of fixed-size particles (radius a) contained between parallel plates 0 ≤x≤L=1 m.
The volume fraction of particles is fv(x)=f0+ ∆ f(x/L), and their temperature is T(x)=T0+ ∆T(x/L), where
∆f/f0= ∆T/T0=1, f0=1%, T0=500 K. Assuming the particle size to be a=500 µm, and made of a
material with a gray hemispherical emittance of ǫλ=0.7, show that the large-particle approximation may be
used for the infrared. Calculate the local, spectral absorption and scattering coefficients. Determine the local
Planck-mean extinction coefficient as well as the total optical thickness of the slab (based on the Planck-mean).
Solution
With temperatures ranging between 500 K and 1000 K, the Planck function Ibλis substantial in the wavelength
range 2.2µm< λ < 19 µm (i.e., the range between f(λT)min ≃0.1 and f(λT)max ≃0.9 from Appendix C).
so that the large particle limit applies.
κλ=ǫλπa2NT=ǫλ
1−ǫλ
σsλ=0.7
0.3×0.045(1+ξ)=0.105(1+ξ) cm−1.
The local Planck-mean extinction coefficient is found from equation (12.32) as
βP=π
βλIbλdλ=βλ,