Page 299 - Dust Explosions in the Process Industries
P. 299

268  Dust Explosions in the Process Industries


             4.2.2
             DIFFERENCES BETWEEN FLAMES IN  PREMIXED GAS
             AND IN DUST CLOUDS


             Leuschke (1965) pointed out some characteristicdifferences between a laminar, premixed
             gas flame and a laminar dust flame. One important difference is that the reaction zone
             in the dust cloud is considerably thicker than in the gas, irrespectiveof the type of dust,
             and on the order of at least 10-100  mm. When discussingthis feature of the dust flame,
             Cassel(l964) distinguished between two types of flames. The first, the Nusselt type, is
             controlledby diffusion of oxygen to the surface of individual, solid particles, where the
             heterogeneous chemical reaction takes place. In the second type, the volatile flame, the
             rate of gasification,pyrolysis, or devolatilizationis the controlling process and the chem-
             ical reaction takes place mainly in the homogeneous gas phase. In Nusselt-type flames,
             the greater thickness of the combustionzone, compared with that of premixed gas flames,
             results from the slower rate of molecular diffusion, compared to diffusion in premixed,
             homogeneous gases. In the volatile flame type, the greater flame thickness is due to the
             preheating zone, where volatiles or pyrolysis gases are driven out of the particles ahead
             of the flame. When mixed with air, these gases and vapors burn almost as a premixed
             gas. The combustion of  the remaining solid char particles occurs subsequently at a
             slower rate in the tail of the flame, and therefore the volatile flame in clouds of coals and
             organic dusts is also in fact coupled to a Nusselt-type flame.
               In metals, low melting-pointmaterials may oxidize in the vapor phase, but due to the
             oxide film around each particle, this does not result in a homogeneous metal vapor/air
             flame. Because of the large heat of combustionper mole of O2for example, of aluminum
             and magnesium dust compared with organic dusts, the temperature of the burning par-
             ticles is very high and thermal radiation plays a central role in the transfer of heat in the
             combustion wave. Radiative heat transfer is also supposed to play a role in coal dust
             flames. However, because the thermal radiation is proportional to the fourth power of
             the temperature, the role of thermal radiation in coal dust flames is less important than
             in, for example, aluminum and magnesium dust flames. Radiative heat transfer in dust
             flames is a complex process, and it is of  interest to note that Elsner, Koneke, and
             Weinspach (1988) investigated the solid particle emissivity in dust clouds as a function
             of dust cloud thickness, specific surface area of  the particles, dust concentration, and
             absorption and scatter coefficients. Experiments were conducted with fluidized bed ash
             and quartz sand. Good agreement was found between the experiments and a theoretical
             equation.
               Leuschke (1965) conducted an illustrative series of experiments demonstrating the
             importance of radiative heat transfer in metal dust flames, using the experimental setup
             illustrated in Figure 4.8. Two transient dust clouds were generated simultaneouslyon the
             two sides of  a double-glass window, one being ignited immediately by a gas flame. It
             was then observed whether the radiation from the burning cloud was able to ignite the
             other cloud.
               Table 4.2, summarizing the results, shows that only the flames of Zr, Ti, AI, and Mg
             produced sufficient radiation to ignite the other cloud. Ignition of  graphite was not
             accomplishedat all, in agreement with the inability of graphite dust clouds to propagate
             a self-sustained flame in air at normal temperature and pressure. The reason why the gas
   294   295   296   297   298   299   300   301   302   303   304