Page 480 - Bird R.B. Transport phenomena
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460  Chapter 15  Macroscopic Balances for Nonisothermal Systems

                                                                   Fig. 15.3-2.  The mixing  of two ideal  gas
                                                                   streams.








                                                       Plane 2






       EXAMPLE   15.3-2    Two steady, turbulent streams  of  the same ideal gas  flowing  at different  velocities, tempera-
                           tures, and pressures  are  mixed  as  shown  in  Fig.  15.3-2. Calculate the velocity, temperature,
      Mixing  of  Two  Ideal  and pressure of the resulting stream.
      Gas  Streams
                           SOLUTION
                           The fluid  behavior in this example is more complex than that for  the incompressible, isother-
                           mal  situation discussed  in Example  7.6-2, because here changes  in density  and temperature
                           may  be  important. We  need  to use  the steady-state  macroscopic energy  balance, Eq. 15.2-3,
                           and  the ideal  gas  equation  of  state, in addition to the mass  and  momentum balances.  With
                           these exceptions, we proceed as in Example 7.6-2.
                               We  choose the inlet planes (la and lb) to be cross sections at which the fluids  first  begin
                           to  mix.  The outlet plane  (2) is  taken  far  enough downstream that complete mixing  has oc-
                           curred. As  in Example 7.6-2 we  assume  flat  velocity  profiles,  negligible  shear stresses  on the
                           pipe wall, and no changes in the potential energy.  In addition, we  neglect the changes in the
                           heat capacity  of the fluid  and assume adiabatic operation. We  now write the following  equa-
                           tions for this system with two entry ports and one exit port:
                           Mass:                             =  м? 1я  +  w }b                  (15.3-6)
                           Momentum:           v 2 w 2  +  p 2 S 2  =  }a  +  p ]a S u  +  v }b w ]b  +  p lb S lb  (15.3-7)
                           Energy:  w [C (T  -  T )  + \v\\ = wJC (T  -  T )  + \v\ ]  + w [C (T  -  T )  + \v] \  (15.3-8)
                                    2  p  2  nf          p  la   ref    a   }b  p  U)  ref   b
                           Equation of state:              Pi  =  P RT /M                       (15.3-9)
                                                                2
                                                                   2
                           In this set of equations we know all the quantities at la  and lb, and the four unknowns are p 2/
                           T , p , and v . T  is the reference temperature for  the enthalpy. By multiplying  Eq. 15.3-6 by
                               2
                                        ref
                            2
                                     2
                           C T  and adding the result to Eq. 15.3-8 we get
                            p  ref
                                            w [C T 2  + &}  =                    Ш             (15.3-10)
                                               p
                                             2
                           The right sides  of  Eqs. 15.3-6, 7, and  10 contain known quantities and we designate them by
                           w, P, and  £,  respectively.  Note  that  w, P, and  E are  not  independent,  because  the  pressure,
                           temperature,  and  density  of each inlet stream  must be related  by the equation  of state.
                               We now solve Eq. 15.3-7 for v 2 and eliminate p 2 by using the ideal gas law. In addition  we
                           write w 2 as p 2v 2S 2. This gives
                                                               RT 2  __P
                                                                                               (15.3-11)
                                                            2
                                                               Mv 2  w
                           This equation  can be solved  for  T 2, which is inserted  into Eq. 15.3-10 to give
                                                 *-\*£x)lW                                     (15.3-12)
                                                                     y+    W
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