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                    124  CHAPTER 8



                  • Pyroclastic density currents are fast-moving,  Walker, G.P.L. & Croasdale, R. (1971) Two Plinian-
                    ground-hugging clouds of very hot clasts and gas  type eruptions in the Azores. J. Geol. Soc. London
                    that flow like liquids. They contain a very wide  127, 17–55.
                    range of clast sizes. Their speeds can be at least  Wilson, L. & Walker, G.P.L. (1987) Explosive volcanic
                    100ms −1  and their travel distance can be many  eruptions – VI. Ejecta dispersal in Plinian eruptions:
                    tens of kilometers. Although they mainly flow  controls of eruption conditions and atmospheric
                    along valley floors, these speeds imply that they  properties. Geophys. J. Roy. Astron. Soc. 89, 657–
                    can climb over topographic obstacles in their  79.
                    paths a few hundred meters high if there is
                    no way to flow around.                     PYROCLASTIC DENSITY CURRENTS
                  • Smaller scale pyroclastic density currents can
                                                              Branney, M.J. & Kokelaar, P. (1992) A re-appraisal of
                    occur when only part of an eruption column
                                                                ignimbrite emplacement: progressive aggradation
                    collapses, or when a volcanic dome or lava flow
                                                                and changes from particulate to nonparticulate flow
                    becomes unstable and disintegrates into pyro-
                                                                during emplacement of high-grade ignimbrite. Bull.
                    clasts and released gas. These travel to smaller
                                                                Volcanol. 54, 504–20.
                    distances, although still at high speeds. A pyro-
                                                              Branney, M.J. & Kokelaar, P. (2002) Pyroclastic Density
                    clastic surge can form when the upper, more
                                                                Currents and the Sedimentation of Ignimbrites.
                    dilute, part of a pyroclastic density current be-
                                                                Memoir 27, Geological Society Publishing House,
                    comes detached from the lower, denser part
                                                                Bath, 143 pp.
                    when the flow meets an obstacle.           Burgisser, A. & Bergantz, G.W. (2002) Reconciling
                  • As they travel, pyroclastic density currents  pyroclastic flow and surge: the multiphase physics
                    deposit pyroclasts on the ground. The deposits  of pyroclastic density currents. Earth Planet. Sci.
                    from large pyroclastic density currents dominated  Lett. 202, 405–18.
                    by grain flow, called ignimbrites, tend to be mas-  Bursik, M.I. & Woods, A.W. (1996) The dynamics and
                    sive, whereas surge deposits formed from more  thermodynamics of large ash flows. Bull. Volcanol.
                    dilute currents exhibit internal stratification.  58, 175–93.
                  • The fronts and tops of pyroclastic density cur-  Druitt, T.H. (1998) Pyroclastic density currents. In The
                    rents can incorporate air which is strongly  Physics of Explosive Volcanic Eruptions (Eds J.S.
                    heated and rises above the body of the density  Gilbert & R.S.J. Sparks), pp. 145–92. Special Publica-
                    current, carrying small clasts up with it to form a  tion 145, Geological Society Publishing House, Bath.

                    co-ignimbrite or phoenix cloud which can itself  Levine, A.H. & Kieffer, S.W. (1991) Hydraulics of
                    generate a fine-grained fall deposit.        the August 7, 1980, pyroclastic flow at Mount
                                                                St. Helens, Washington. Geology 19, 1121–4.
                                                              Neri, A. & Macedonio, G. (1998) Numerical simulation
                  8.6 Further reading                           of collapsing volcanic columns with particles of two
                                                                sizes. J. Geophys. Res. 101, 8153–74.
                                                              Sparks, R.S.J., Wilson, L. & Hulme, G. (1978) Theore-
                  TEPHRA DISPERSAL IN STEADY ERUPTIONS
                                                                tical modelling of the generation, movement and
                  Carey, S. & Sparks, R.S.J. (1986) Quantitative models  emplacement of pyroclastic flows by column col-
                   of the fallout and dispersal of tephra from volcanic  lapse. J. Geophys. Res. 83, 1727–39.
                   eruption columns. Bull. Volcanol. 48, 109–25.  Wilson, C.J.N. (1984) The role of fluidization in the
                  Sparks, R.S.J. (1986) The dimensions and dynamics   emplacement of pyroclastic flows, 2: experimen-
                    of volcanic eruption columns. Bull. Volcanol. 48,  tal results and their interpretation.  J. Volcanol.
                   3–15.                                        Geotherm. Res. 20, 55–84.
                  Sparks, R.S.J., Bursik, M.I., Ablay, G., Thomas, R.M.E.   Wilson, L. & Head, J.W. (1981) Morphology and
                   & Carey, S.N. (1992) Sedimentation of tephra by   rheology of pyroclastic flows and their deposits,
                   volcanic plumes. Part 2: controls on thickness   and guidelines for future observations. In The 1980
                   and grain size variations of tephra fall deposits.   Eruptions of Mount St. Helens, Washington.
                   Bull. Volcanol. 54, 685–95.                  U.S.Geol. Surv. Prof. Pap. 1250, 513–24.
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