Page 30 - Aerodynamics for Engineering Students
P. 30

Basic concepts and definitions  13

                 It is often convenient to link the enthalpy or total heat above to the other energy of
               motion, the kinetic energy w; that for unit mass of gas moving with mean velocity Vis
                                                 -   v2
                                                K=-                               (1.16)
                                                     2
                 Thus the total energy flux in the absence of external, tangential surface forces and
               heat conduction becomes
                                       VZ  +
                                       - cp T = cp TO = constant                  (1.17)
                                        2
               where, with  cp invariant,  TO is  the  absolute temperature  when  the  gas is  at rest.
               The quantity cpTo is referred to as the total or stagnation enthalpy. This quantity is an
               important parameter of the equation of the conservation of energy.
                 Applying the first  law  of  thermodynamics to  the  flow  of  non-heat-conducting
               inviscid fluids gives

                                                                                  (1.18)

                  Further, if the flow is unidirectional and cvT = E, Eqn (1.18) becomes, on cancelling
               dt,
                                            dE +pd(i)  = 0                        (1.19)


               but differentiating Eqn (1.10) gives

                                                                                  (1.20)

               Combining Eqns (1.19) and (1.20)
                                                    1
                                               dh = -dp                           (1.21)
                                                    P
               but

                                                                                  (1.22)
                                           R
               which, together with Eqn (1.21), gives the identity

                                            P
                                            *+ypd(j)    =O                        (1.23)
               Integrating gives
                                                 (3
                                        In p + yln  -  = constant

               or
                                                p = kpy                           (1.24)
               which is the isentropic relationship between pressure and density.
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