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                    120  CHAPTER 8



                  the confining layer defining the pressure in the  the gas–pyroclast mixture will be in the range 360–
                                                                      −3
                  trapped gases. The equivalent of the calculations  370 kg m . This is much greater than the density of
                                                                                        −3
                  given in Chapter 7 suggests that for the magmatic  the Earth’s atmosphere, ∼1kgm . However, as the
                  volatile contents of order 1–3 wt% that commonly  mixture accelerates laterally away from the vent, its
                  apply to these evolved magmas, and for carapace  bulk density will rapidly decrease as the gas decom-
                  strengths of a few megapascals, the initial speeds in  presses to atmospheric pressure. The bulk density
                  these kinds of explosions could easily be at least  will become similar to that expected from the dis-
                        −1
                  100ms .                                     integration of a lava dome or lava flow; the values,
                    The fact that this process causes the develop-  obtained from eqn 6.2, range between  ∼3 and
                  ment of a pyroclastic density current, rather than a  ∼20 kg m −3  (Table 8.2), depending on the magma
                  vertical eruption column, must be strongly influ-  volatile content. Even the smallest of these densi-
                  enced by the bulk density of the mixture of gas and  ties, corresponding to a very volatile-rich magma,
                  pyroclasts that is produced by the lava disintegra-  is greater than that of the atmosphere. This ensures
                  tion; it will also be at least partly dictated by the  that a ground-hugging density current is always
                  detailed geometry of the lava body and the location  formed, whether from a pyroclastic fountain or
                  where the disintegration starts. Of course, if the  the disintegration of a dome or lava flow, but clearly
                  erupted lava is connected to hot magma in the  there is the potential for pyroclastic density
                  underlying dike system, it may well be that, as soon  currents to have a wide range of initial particle
                  as the overlying erupted lava is removed, the subja-  concentrations.
                  cent magma explosively erupts upward and forms   As soon as a pyroclastic density current moves
                  a Plinian eruption column (as at Mount St Helens   away from its source, its top begins to entrain the
                  in 1980) or, if this would not be stable, forms a   air above it in the same way that the edge of an
                  pyroclastic fountain. Certainly, numerous examples  eruption column entrains adjacent air. This process
                  have been observed of vertical eruption columns  starts even sooner if the current is fed by a fountain,
                  being produced very shortly after dome collapse  since some mixing with the surrounding atmo-
                  events.                                     sphere must happen on the outer surface of the
                                                              fountain as material descends toward the ground.
                                                              This inclusion of air must decrease the bulk density
                  8.4.3 Ignimbrite emplacement mechanisms
                                                              of the part of the current involved, and so it begins
                  Our understanding of the way pyroclastic density  to cause a density stratification within the current.

                  currents emplace their characteristic deposits has  As part of the interaction between the density cur-
                  advanced enormously over the past two decades,  rent and the overlying air, a mixture of heated air
                  although there are still many details that are not  and volcanic gas elutriates some fraction of the
                  fully understood. One of the most important issues  smallest clasts from the main body of the current to
                  relates to the density of the currents while they are  form a growing convection cloud above it. This is
                  moving and the motions within them – especially  called a co-ignimbrite cloud, or phoenix cloud
                  the extent to which those motions are turbulent   (see Fig. 8.10). These clouds may be carried by the
                  or laminar. These factors control the way clasts are  wind in a quite different direction from that of the
                  deposited on the ground as the current passes a  density current, eventually depositing their small
                  given location.                             clasts to form a characteristic co-ignimbrite ash
                    Because of the way they are formed, the currents  fall deposit.
                  are likely to start out as homogeneous mixtures of   There is another important source of stratifica-
                  gas and pyroclasts, but they may have a wide range  tion within the main body of the density current:
                  of bulk densities. If a current is formed from a   the tendency of clasts to fall through the gas phase.
                  pyroclastic fountain, the analysis described in the  In principle every pyroclast will try to reach its
                  previous section shows that the pressure in the   equilibrium terminal velocity in the gas, which
                  gas emerging from the vent will be 1 to 10 MPa   eqns 8.1 and 8.3 show to be a function of the clast
                  (Table 8.2) and as a result the bulk density of   size and density together with the properties of
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