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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 /3831/CH16/EX16.2/Ex16_2.sce | |
| parent | b1f5c3f8d6671b4331cef1dcebdf63b7a43a3a2b (diff) | |
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initial commit / add all books
Diffstat (limited to '3831/CH16/EX16.2/Ex16_2.sce')
| -rw-r--r-- | 3831/CH16/EX16.2/Ex16_2.sce | 16 |
1 files changed, 16 insertions, 0 deletions
diff --git a/3831/CH16/EX16.2/Ex16_2.sce b/3831/CH16/EX16.2/Ex16_2.sce new file mode 100644 index 000000000..7f40f256f --- /dev/null +++ b/3831/CH16/EX16.2/Ex16_2.sce @@ -0,0 +1,16 @@ +// Example 16_2
+clc;funcprot(0);
+// Given data
+T=20+273.15;// K
+V=25.0;// m/s
+k=1.40;// The specific heat ratio
+p=0.101;// MPa
+g_c=1;// The gravitational constant
+c_p=1.004;// kJ/kg.K
+R=0.286;// kJ/kg.K
+
+// Solution
+p_os=p*(1+((V^2/1000)/(2*g_c*c_p*T)))^(k/(k-1));// The isentropic stagnation pressure in MPa
+rho=(p*10^3)/(R*T);// kg/m^3
+rho_os=rho*(1+((V^2/1000)/(2*g_c*c_p*T)))^(1/(k-1));// The isentropic stagnation density in kg/m^3
+printf("\nThe isentropic stagnation pressure,p_os=%0.4f MPa \nThe isentropic stagnation density,rho_os=%1.4f kg/m^3",p_os,rho_os);
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