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                                                                                    LAVA FLOWS   135


                                                  Fractured, no strength
                                                   Brittle but unfractured
                                              Viscoelastic, non-Newtonian


                                                Uncooled Newtonian core
                 Fig. 9.15 Illustration of the changing
                 properties of the lava in a lava flow
                 lobe as a result of the variation of
                 temperature with distance from
                 the flow’s cooling boundaries.


                  formed. It is possible that the single Bingham rheol-  fluid it will flow if given the slightest chance to
                  ogy model is an adequate approximation for these  do so. Under any given set of stresses, it may be
                  features.                                   the brittle-elastic layer, the viscoelastic layer or the
                   However, the realization that the majority of lava  Newtonian layer that controls the apparent rheol-
                  flows contain a very hot central core, at least until  ogy of the flow as a whole. Working out the distri-
                  the time when they stop flowing, implies that there  bution of stresses inside a lava flow unit to decide
                  is no good reason to expect the lava deep in the  how, and if, it will move is a problem that has not
                  channel, which is responsible for the advance of  yet been completely solved.
                  the flow, to have the same properties as the cool
                  lava forming the levées. The cross-sectional profile
                  of a channelized flow is more likely to be as shown  9.6 Lava flow motion
                  in Fig. 9.14b, with the channel containing a layer
                  of lava chilled against the original ground surface,  It is reasonable to assume that, at least in basaltic
                  above which a raft of cooled lava, distorted and  lava flows, the hot lava in the central channel has
                  sheared at its edges where it experiences friction  a negligible yield strength. In that case we can
                  with the stationary levées, is carried along on top   assume that the lava in the central channel can
                  of a Newtonian fluid core.                   be described by just one parameter, its constant
                   The fact that there are very great differences  Newtonian viscosity, η. It can then be shown that
                  between the physical properties of the different  if the lava in the channel has depth d , which we

                                                                                             c
                  parts of a lava flow is central to understanding flow  assume (as is generally true) to be much less than
                  shape and movement. Figure 9.15 illustrates the  the width of the channel, its average flow speed U
                  key facts. The material at the front and sides of a  is given by
                  flow consists, in general, of at least three layers. The
                                                                      2
                  very cool outer layer contains many cracks that  U = (ρ gd sin α)/(3 η)          (9.6)
                                                                      c
                  have formed due to the stresses of cooling, and the
                  presence of the cracks means that this layer has no  as long as the motion of the lava is smooth and
                  strength at all. Inside this is a layer where the lava is  laminar. If the flow speed is large enough, the
                  below its solidus temperature, but has not devel-  motion of the liquid in the channel may become
                  oped a network of interconnecting cracks, so that   disordered and turbulent, in which case the speed
                  it has some brittle strength. Further still from the  is given by
                  surface is a layer that has a temperature above the
                  solidus. This material is viscoelastic and will deform  U = [(2 gd sin α)/f ] 1/2  (9.7)
                                                                       c
                  in a plastic fashion if stressed slowly but, like the
                  brittle layer, will develop cracks if it is stressed   where f is a friction factor equal to about 0.01. It
                  suddenly. Finally the lava furthest from the surface  should be stressed that most of the types of lava
                  is well above its solidus temperature and has no  flow yet observed in eruptions on Earth have been
                  significant strength, so that like any Newtonian  laminar, although carbonatite flows are commonly
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