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                 8              Pyroclastic falls and



                                pyroclastic density currents

















                 8.1 Introduction
                                                              8.2.1 Fallout from the rising eruption column
                 Chapter 6 discussed the upward transport of clasts  Chapter 6 explained that an eruption column can
                 in eruption columns, their eventual release from  be divided into three regions: the gas-thrust region,
                 such columns, and the factors that may cause  the convective region and the umbrella region. The
                 columns to become unstable, leading to pyroclastic  width of an eruption column increases with height
                 fountaining that feeds pyroclastic density currents.  in the gas-thrust and convective regions, becoming
                 This chapter looks in more detail at all of these   even wider in the umbrella region, where it com-
                 processes and at the mechanisms of emplacement  monly spreads preferentially downwind (Fig. 6.5).
                 of the resulting deposits.                   Figure 8.1 shows the same eruption column seen
                                                              from directly upwind of the vent. In the gas-thrust
                                                              and convective regions the expansion in the erup-
                 8.2 Fallout of clasts from eruption columns  tion column is caused by the entrainment and heat-
                                                              ing of air from the surrounding atmosphere. The
                 Chapter 6 showed how the terminal velocity of a
                 clast within the eruption column, which is a func-
                 tion of its radius, density, and shape, largely deter-

                 mines the height above the vent to which it can be
                 carried. The general pattern is for the largest clasts                Umbrella Region
                 to fall out from lower levels with smaller clasts
                 being carried to greater heights. The exact height
                 reached by a clast of given size and type, however,
                 depends on the eruption conditions, as discussed                      Convective Region
                 further below, and the location at which it lands
                 depends on the state of the atmosphere, especially
                 the wind. The distribution of fallen pyroclasts                        Gas-Thrust or
                 on the ground can be used to infer at least some                       Inertial Region
                 of the properties of the eruption that produced
                 them. This is particularly important for volcanoes              Vent
                 that erupt very explosively, but do so only very
                                                              Fig. 8.1 A Plinian eruption cloud viewed from upwind of
                 rarely (perhaps at intervals of tens to hundreds of
                                                              the vent. The progressively greater lateral spreading of
                 thousands of years), because it means that the prod-
                                                              the cloud continues for most of its rise, but eventually
                 ucts of prehistoric eruptions can be analyzed in
                                                              incorporation of air that brings with it the momentum of the
                 order to gain some idea of what to expect in the  wind causes the top of the cloud to be carried away in the
                 future.                                      downwind direction and spreading becomes negligible.
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