Page 243 - Dust Explosions in the Process Industries
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Generation of Explosible Dust Clouds  2 15
















                                            Figure 3.1 2  Scanning electron micrograph single
                                            lycopodium  particle  showing  the  rough  surface
                                            topography.


      3.5.2
      DRAG ON A PARTICLE IN GENERAL

      Figure 3.10 covers the terminal settling velocities of the particle sizes of primary inter-
      est in relation to dust explosion problems, and as shown, Stokes' laminar theory applies
      over most of the range. However, in many situations in industry and particularly during
      dust explosions, general inertia forces may dominate the gravity force, and other flow
      regimes may be of primary interest. The Reynolds number of the particle is an impor-
      tant indicator of the flow regime. The Reynolds number for a particle of diameter  x trav-
      eling in a gas is defined as

                                                                             (3.14)


      where pp is the density of the gas, vIe1 is the relative velocity between the particle and
      the gas, and p is the viscosity of the gas. The drag coefficient C4 is another important
      parameter. It is the ratio between the drag force acting on the pmcle and the product of
      the cross-sectional area of the particle and the dynamic pressure acting on that area. For
      laminar flow conditions (Stokes' range),

           24
      c  =-                                                                  (3.15)
           Re
      The change of the drag coefficient C,  as Reynolds number increases is shown in Figure 3.13
      for three different particle shapes.
        According to Haider and Levenspiel (1989) one can find more than 30 equations in
      the literature that relate the drag coefficient  C,  to the Reynolds number for spherical par-
      ticles falling at their terminal velocities. They also give more recent experimental data
      confirming that Figure 3.13 is adequate for isometric particles of  sphericities Q, of
      0.7-1.0,  where @ is defined as the ratio of the surface area of a sphere having the same
      volume as the particle to the actual surface area of the particle. For disks of lower Q,
      values, in the range 0.2-0.02,  the C,  at a given Re are higher, by a factor on the order
      of  10, than that shown by the curve in Figure 3.13.
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