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| author | prashantsinalkar | 2017-10-10 12:27:19 +0530 |
|---|---|---|
| committer | prashantsinalkar | 2017-10-10 12:27:19 +0530 |
| commit | 7f60ea012dd2524dae921a2a35adbf7ef21f2bb6 (patch) | |
| tree | dbb9e3ddb5fc829e7c5c7e6be99b2c4ba356132c /534/CH12/EX12.4/12_4_Blackbody_Angular_Radiation.sce | |
| parent | b1f5c3f8d6671b4331cef1dcebdf63b7a43a3a2b (diff) | |
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initial commit / add all books
Diffstat (limited to '534/CH12/EX12.4/12_4_Blackbody_Angular_Radiation.sce')
| -rw-r--r-- | 534/CH12/EX12.4/12_4_Blackbody_Angular_Radiation.sce | 26 |
1 files changed, 26 insertions, 0 deletions
diff --git a/534/CH12/EX12.4/12_4_Blackbody_Angular_Radiation.sce b/534/CH12/EX12.4/12_4_Blackbody_Angular_Radiation.sce new file mode 100644 index 000000000..6015f17bc --- /dev/null +++ b/534/CH12/EX12.4/12_4_Blackbody_Angular_Radiation.sce @@ -0,0 +1,26 @@ +clear;
+clc;
+printf('FUNDAMENTALS OF HEAT AND MASS TRANSFER \n Incropera / Dewitt / Bergman / Lavine \n EXAMPLE 12.4 Page 743 \n')// Example 12.4
+
+// Rate of emission per unit area over all directions between 0 degC and 60 degC and over all wavelengths between wavelengths 2 and 4 micro-m
+
+T = 1500 ;//[K] temperature of surface
+stfncnstt = 5.67*10^-8 ;//[W/m^2.K^4] Stefan-Boltzmann constant
+
+//From Equation 12.26 Black Body Radiation
+Eb = stfncnstt*T^4; //[W/m^2]
+
+//From Table 12.1 as wl1*T = 2*1500 (micro-m.K)
+F02 = .273;
+//From Table 12.1 as wl2*T = 4*1500 (micro-m.K)
+F04 = .738;
+
+//From equation 12.10 and 12.11
+i1 = integrate('2*cos(x)*sin(x)','x',0,%pi/3);
+delE = i1*(F04-F02)*Eb;
+
+printf("\n Rate of emission per unit area over all directions between 0 degC and 60 degC and over all wavelengths between wavelengths 2 micro-m and 4 micro-m = %.1e W/m^2",delE);
+//END
+
+
+
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