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                    86  CHAPTER 6



                       10       10 2      10 3     10 4      10 5     10 6
                     50                                                  50



                     40                           Bezymianny, 1956       40
                                                                             Fig. 6.7 The relationship between the
                                                                            heights of some observed eruption
                   Plume height (km)  30  Santa Maria, 1902     0.3      30  eruption rates in the eruptions
                                                             1.0
                                                                            plumes and the estimated mass
                                                              0.7
                                                                            producing them. The curves are the
                                                                            results of theoretical calculations and
                                             Hekla, 1947
                                                                            are labeled by the fraction of the heat
                                                                         20
                     20
                                                                            to drive the plume upward. Not all of
                                      Hekla, 1970     Soufriere, 1902       contained in pyroclasts that is available
                                                                            the pyroclast heat is available because
                     10        Fuego, 1971                               10  some is removed by large clasts falling
                         Ngauruhoe,                                         out of the plume. (Adapted from fig. 2
                         1974                                               in Wilson, L., Sparks, R.S.J., Huang,
                                Heimaey, 1973                               T.-C. & Watkins, N.D. (1978) The
                      0                                                  0
                                                                            control of volcanic column heights
                       10        10 2     10 3     10 4      10 5     10 6  by eruption energetics and dynamics.
                                                         –1
                                                       3
                                     Volume eruption rate (m  s )            J. Geophys. Res. 83, 1829–1836.)
                  where H is the plume height in kilometers and M  the match between theory and observation is sur-
                                                          f
                                    −1
                  is the mass flux in kg s .                   prisingly good.
                    A “standard atmosphere” is one that is typical
                  of the whole of the Earth. In practice the thermal
                  structure of the atmosphere varies as a function of  6.6 Fallout of clasts from eruption plumes
                  latitude, longitude, elevation above sea level and
                  season of the year, as well as with the local, short-  Thus far we have largely ignored the fact that the
                  term weather conditions, especially the humidity,  rising eruption plume carries with it magma clasts
                  i.e., the water vapor content. One systematic con-  or clots. This section looks at the fate of the clasts in

                  sequence of this is that, for the same eruption   an eruption plume.
                  conditions, one expects to generate higher plumes
                  at lower latitudes.
                                                              6.6.1 Rise of clasts in an eruption plume
                    Figure 6.7 shows a plot of some observed erup-
                  tion plume heights as a function of the corres-  If you drop an object, it falls through the air under
                  ponding estimated volume eruption rates, with  gravity and accelerates until the gravity force acting
                  three theoretical curves superimposed. One of  downward is balanced by the resisting frictional
                  these assumes that all of the available heat from   drag force of the surrounding air. The clasts in the
                  the magma is used to drive the plume, as in eqn 6.7,  eruption plume are no different from any other
                  and the others assume that either 70% or 30% of the  object: they are also trying to fall under gravity. The
                  heat is lost due to the early fallout of large clasts.  difference in the case of magma clasts is that they
                  There are inevitable uncertainties in the obser-  are also being dragged upwards within a rising gas
                  vations of plume heights and mass fluxes: both  stream. This is true of the clasts both when they are
                  change with time during an eruption, and the erup-  still within the dike system above the fragmentation
                  tion rate estimate involves measuring the amount of  level and when they are being carried upwards in
                  pyroclasts deposited around the vent over a finite  the rising eruption plume above the vent. Thus a
                  time interval, and so it is only ever an average dur-  clast is subject to two competing forces – the force
                  ing part of the eruption. Given all these problems,  of gravity trying to making the clast fall and the drag
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