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                                             PYROCLASTIC FALLS AND PYROCLASTIC DENSITY CURRENTS  115


                 that is a perfect cone. If you take a series of closely  to fall deposits from the convecting eruption
                 spaced horizontal slices through the cone, then the  clouds above Hawaiian eruptions, but little work
                 average of the areas of the top and bottom of a slice,  has been done on this yet.
                 multiplied by the slice thickness, is a good approx-  We now turn our attention to the second family
                 imation to the volume of the slice. In the same   of pyroclastic deposits, those emplaced not by fall-
                 way, the average of the areas of any two isopachs,  out from a high eruption column but rather by flow
                 multiplied by the difference between the deposit   of a mixture of clasts and gas as density currents
                 thicknesses that they represent, is a good approx-  close to the ground.
                 imation to the volume of the deposit between
                 the isopachs. Adding up the contributions from
                                                              8.4 Pyroclastic density currents and
                 all pairs of isopachs gives the total deposit volume.
                                                              their deposits
                 Of course, it is necessary to estimate the loca-
                 tion of the zero-thickness isopach; and the more
                 closely spaced the isopachs the more accurate   The deposits from pyroclastic density currents
                 the volume.                                  include some of the smallest volcanic layers pre-
                   The resulting volume is the volume of the deposit  served in the geological record and also the depos-
                 as it lies on the ground. It is normal to convert this  its from what are undoubtedly the largest-volume
                 to the equivalent volume that it would occupy if all  and most destructive volcanic phenomena on Earth.
                 of the pore space within the pyroclasts and all of  However, they have certain key properties in com-
                 the vacant space between the rather loosely packed  mon which is why they are discussed together.
                 clasts were removed – the so-called dense rock
                 equivalent (DRE) volume. Multiplying the DRE
                                                              8.4.1 Nature of the deposits
                 volume by the density of the solid version of the
                 erupted magma gives the total mass of the deposit.  The three main terms used to describe these depos-
                 These are important adjustments to make, because  its are  ignimbrite,  pyroclastic surge deposit
                 they allow the duration of the eruption to be esti-  and block-and-ash flow deposit, and the magmas
                 mated. This is done by dividing the mass of the  giving rise to them are almost always of evolved
                 deposit by the mass eruption rate derived from  composition. The deposits are dominated by juve-
                 fitting the field data to the curves in Fig. 8.6. The  nile material but commonly also contain  lithic
                 estimate of the duration may not be very accurate  fragments torn from the walls of the dike and vent

                 because, as mentioned earlier, the mass flux may  system feeding the eruption. The juvenile clasts
                 have changed during the eruption, and so the fit to  include intact lapilli and blocks of vesicular pumice,
                 the theoretical curves may not give a good estimate  glassy shards which represent fragments of pumice
                 of the average eruption rate.                clasts which have been broken up, and broken
                                                              pieces of crystals which grew in the magma prior to
                                                              eruption and which were released when pumices
                 8.3.5 Fall deposits: summary
                                                              shattered. Ignimbrites are generally ash-rich and
                 When used on prehistoric eruptions, the kinds   very poorly sorted, forming extensive sheets or
                 of analyses described above, from which we can  fans (Fig. 8.8) that cover large areas, up to tens of
                 estimate magma volatile content, mass eruption  thousands of square kilometers. They bury or
                 rate, eruption cloud height, and wind speed and  drape pre-existing topography and thicken in local
                 direction during the eruption, are best applied to  depressions. Pyroclastic surge deposits are some-
                 the deposits from large Plinian eruptions. This is  what better-sorted than ignimbrites, although still
                 because the large dispersal area of such eruptions  poorly sorted, and show distinct internal stratifica-
                 maximizes the chances of significant amounts   tion (Fig. 8.9). They may occur within or immedi-
                 of the deposit being preserved in the geological  ately adjacent to ignimbrite deposits. Block-and-ash
                 record and exposed for us to examine. There is  flow deposits differ from the other two types in
                 clearly the potential to apply the same methods   generally containing clasts that are less vesicular.
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