Converging-diverging nozzle Solution: First off all, I have to specify that I prefer to work in SI units. I don’t think that it is a problem to convert the SI units in English-American ones. C A B VA VB VC B A C a) The inlet conditions are the standard atmospheric conditions, which means pA 1.013 bar 1.013 105 N/m 2 TA 288 K ( 15C) (1) From here, we can get the density at inlet station, by applying the ideal gas law: A pA R TA (2) where R = the gas constant (in our case, this is the air thermodynamic constant). The general formula for computing the gas constant is the following: R M (3) where = the universal gas constant, which is = 8.314 kJ/kmol.K M = the molecular weight of the gas, which is M = 29 kg/kmol (for air) As a result, the air constant will be: 8.314 R 0.2867 kJ/kg.K 286.7 J/kg.K 29 Introducing the numerical values in (2), we get the following: A 1.013 105 1.227 kg/m 3 286.7 288 (4) The speed at station (A) is VA = 380 ft/s = 115.8 m/s and the cross area of section A-A is AA 2 DA 4 (5) where DA = 5” = 5x25.4 = 127 mm = 0.127 m. By replacing in equation (5), we will have the following: AA 0.1272 0.0127 m2 ( 19.63 in2 ) 4 (6) Now, we are able to compute the air mass flow through the nozzle, by using the formula: M a A AAVA M a 1.227 0.0127 115.8 1.804 kg/s ( 3.977 lbm/s) (7) (8) b) In order to compute the velocities at stations (B) and (C), we will apply the mass flow conservation law: M A M B M C A AAVA B ABVB C ACVC We can compute easily the cross section areas at stations (B) and (C): DB 2" 2 25.4 50.8 mm 0.0508 m DC 6" 6 25.4 152.4 mm 0.1524 m 2 DB 0.05082 0.002 m2 ( 3.14 in2 ) 4 4 AC DC2 0.15242 0.0182 m2 ( 28.27 in2 ) 4 4 AB The densities at stations (B) and (C) are: 0.4536 B 0.060 lbm/ft 3 0.060 kg/m 3 0.961kg/m 3 3 0.3048 0.4536 C 0.050 lbm/ft 3 0.050 kg/m 3 0.801kg/m 3 3 0.3048 By using (8) and (10), one yields: M a 1.804 VB 938.6 m/s ( 3079.4 ft/s) B AB 0.961 0.002 M a 1.804 VC 123.7 m/s ( 405.8 ft/s) C AC 0.801 0.0182 (9) (10) c) The pressure at station (B) will be computed, using the ideal gas law: pB BR TB (11) where TB 30.5F 5 30.5 32 0.83C - 0.83 273 272.17 K 9 pB 0.961 286.7 272.17 0.75 105 N/m 2 0.75 bar (12) (13) In order to compute the pressure at station (C), we will apply the isentropic law: pB Bk pC pC pB C B Ck k (14) where k = adiabatic exponent: k cp cV = 1.4 for air (15) 1.4 0.801 pC 0.75 0.581bar 0.961 d) The potential energy is a result of gravity or other fields, which are not present in our problem. Therefore, the potential energy will be neglected in the energetic balance. If we denote h* h V2 p V2 u 2 2 (16) we obtain the total enthalpy, thus the energy conservation law leads to: h* const. (17) So, if we compute the total enthalpy, we can apply the above equation (16) and find out all kinds of energies involved in the process. h* h V2 V2 k V2 c pT RT 2 2 k 1 2 (18) where cp = specific heat at constant pressure and h h0 c pT h0 kR T k 1 h0 = a reference value, which usually is taken zero. (19) For station (A) we will have the following: h* 1 .4 115.82 286.7 288 295698 J/kg 295.7 kJ/kg 1 .4 1 2 VA2 115.82 295.7 289 kJ/kg 2 2 103 VB2 938.62 hB h * 295.7 144.8 kJ/kg 2 2 103 (The enthalpy can be negative, since it is a relative feature, depending on a reference level of the total enthalpy, which in our case, was taken as zero) V2 123.72 hC h * C 295.7 288 kJ/kg 2 2 103 The kinetic energies (for one mass flow unit) are: VA2 115.82 ek , A 6704.8 J/kg 6.7 kJ/kg 2 2 V 2 938.62 ek ,B B 440485 J/kg 440.5 kJ/kg 2 2 V 2 123.72 ek ,C C 7650.8 J/kg 7.7 kJ/kg 2 2 From (16), the specific internal energy values will be: p 1.013 105 1 u A hA A 289 3 206.4 kJ/kg A 1.227 10 hA h * uB hB pB 0.75 105 1 144.8 222.8 kJ/kg B 0.961 103 uC hC pC 0.581 105 1 288 3 215.5 kJ/kg C 0.801 10 Final remark: The above results are specific features; if we want to calculate absolute features, we have to multiply with the actual mass flow rate. I hope this is the answer that you are looking for. (20)