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                    106  CHAPTER 8



















                                                                             Fig. 8.2 A Plinian eruption cloud
                                                                            viewed obliquely from a direction
                                                                            at right-angles to the direction of the
                                                                            wind. A clast released from the edge
                                                                            of the cloud is carried downwind from
                                                                            its release point and travels a distance
                                                                            that depends on the wind speed and
                                                                            its terminal fall velocity.



                  entrainment in the gas-thrust region is dominated  mass flux) can be used to predict the shape of the
                  by momentum transfer, and an analysis by a pioneer  eruption column and the height to which a clast of
                  of fluid mechanics named Prandtl showed that this  a given size and density will be carried. Then if the
                  should cause the edge of the eruption column to  speed at which the clast will fall and the speed of
                  expand at a rate of one unit sideways for every eight  the wind are known, it is possible to predict where
                  units of height gained. This pattern is close to what  on the ground any given clast should land (Fig. 8.2).
                  has been seen in historic eruptions, especially if an  The smaller the clast, the greater the height to
                  allowance is made for the fact that the bulk density  which it is carried above the vent and thus, because
                  of the erupting jet of clasts and volcanic gas is  the column expands with height, the greater the
                  greater than the density of the surrounding atmo-  cross-wind distance it will land from the vent; also,

                  sphere. Higher up the eruption column, as discussed  the greater the wind speed, the greater the down-
                  in Chapter 6, things become more complicated   wind distance it will land. This description suggests
                  due to the expansion of entrained air, as a result of  that there should be a unique relationship between
                  both heating by pyroclasts and the decreasing atmo-  clast size and position in the final deposit. Unfor-
                  spheric pressure. The spreading rate increases, and  tunately things are a little more complicated,
                  as a general approximation one can think of the   because at any given height in an eruption column
                  lateral expansion rate as being 1 in 8 for the first  a range of particle sizes will be released. The largest
                  quarter of the plume height, 1 in 4 for the second  clast will, of course, be the one that is just sup-
                  quarter, 1 in 2 for the third quarter, and 1 in 1, i.e.,  ported in the column by the rising gases at that
                  a spreading angle of 45° from the vertical, near the  height; but there will also be many smaller clasts
                  start of the umbrella region (Fig. 8.1).    that would normally be carried to greater heights
                    A clast will only fall out from the eruption col-  but that happen to be moved by turbulence to the
                  umn if it is carried to the edge of the column. Once  edge of the column where the upward velocity is
                  it is released, it will be carried along by the wind,  much smaller as the column grades into the bulk of
                  but this will only move it in the direction of the  the atmosphere, and some of these smaller clasts
                  wind. Using the theoretical models of eruption  will be released as well. This means that at every
                  cloud development described in Chapter 6, the erup-  location a pyroclastic fall deposit will contain a
                  tion conditions (magma gas content and erupted  range of grain sizes.
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