Flow through the slit or orifice depends on the distributions of the flux of mass leaving the bounding surfaces. These distributions are found by formulating and solving pairs of integral equations. In the case of the slit, the integral equations are formulated by employing kinetic theory methods, while for the annular orifice the techniques of radiative transfer were used. In addition to exact solutions, closed-form solutions based on an approximate model are derived. Results are presented for a wide range of values of the relevant geometrical parameters.
|Original language||English (US)|
|State||Published - Jan 1 1969|
|Event||Unknown conference - |
Duration: Nov 16 1969 → Nov 21 1969
|Period||11/16/69 → 11/21/69|