From 7f60ea012dd2524dae921a2a35adbf7ef21f2bb6 Mon Sep 17 00:00:00 2001 From: prashantsinalkar Date: Tue, 10 Oct 2017 12:27:19 +0530 Subject: initial commit / add all books --- 534/CH12/EX12.5/12_5_Diffuse_emitter.sce | 45 ++++++++++++++++++++++++++++++++ 1 file changed, 45 insertions(+) create mode 100644 534/CH12/EX12.5/12_5_Diffuse_emitter.sce (limited to '534/CH12/EX12.5/12_5_Diffuse_emitter.sce') diff --git a/534/CH12/EX12.5/12_5_Diffuse_emitter.sce b/534/CH12/EX12.5/12_5_Diffuse_emitter.sce new file mode 100644 index 000000000..8d2f40319 --- /dev/null +++ b/534/CH12/EX12.5/12_5_Diffuse_emitter.sce @@ -0,0 +1,45 @@ +clear; +clc; +printf('FUNDAMENTALS OF HEAT AND MASS TRANSFER \n Incropera / Dewitt / Bergman / Lavine \n EXAMPLE 12.5 Page 748 \n')// Example 12.5 + +// Total hemispherical emissivity +// Total emissive Power +// Wavelength at which spectral emissive power will be maximum + +T = 1600 ;//[K] temperature of surface +wl1 = 2 ;//[micro-m] wavelength 1 +wl2 = 5 ;//[micro-m] wavelength 2 +stfncnstt = 5.67*10^-8; //[W/m^2.K^4] Stefan-Boltzmann constant +// From the given graph of emissivities +e1 = .4; +e2 = .8; +//From Equation 12.26 Black Body Radiation +Eb = stfncnstt*T^4; //[W/m^2] + +//Solution (A) +//From Table 12.1 as wl1*T = 2*1600 (micro-m.K) +F02 = .318; +//From Table 12.1 as wl2*T = 5*1600 (micro-m.K) +F05 = .856; +//From Equation 12.36 +e = e1*F02 + e2*[F05 - F02]; + +//Solution (B) +//From equation 12.35 +E = e*Eb; + +//Solution (C) +//For maximum condition Using Weins Law +consttmax = 2898 ;//[micro-m.K] +wlmax = consttmax/T; + +//equation 12.32 with Table 12.1 +E1 = %pi*e1*.722*10^-4*stfncnstt*T^5; + +E2 = %pi*e2*.706*10^-4*stfncnstt*T^5; + +printf("\n (a) Total hemispherical emissivity = %.3f \n (b) Total emissive Power = %i kW/m^2 \n (c) Emissive Power at wavelength 2micro-m is greater than Emissive power at maximum wavelength \n i.e. %.1f kW/m^2 > %.1f kW/m^2 \n Thus, Peak emission occurs at %i micro-m",e,E/1000,E2/1000,E1/1000,wl1); +//END + + + -- cgit