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                    136  CHAPTER 9



                  turbulent, and some low-viscosity basaltic flows,  reaching it must have flowed even further from the
                  especially when flowing down very steep slopes or  vent and so the wave of cooling will have advanced
                  over cliffs, are locally turbulent. Also, there is every  further into it causing a larger fraction of it to have
                  reason to think that many of the extremely low-  cooled. This means that the yield strength of the
                  viscosity  komatiite flows that were much more  levée material will increase with distance from the
                  common in the Earth’s early history flowed in a very  vent and the flow will get thicker. Meanwhile
                  turbulent fashion, and we see evidence for tur-  the continuing penetration of the cooling effects
                  bulent lava motion on the Moon and Mars, as  means that, even though the core of the flow is still
                  described in Chapter 13.                    very hot, less of its thickness is hot enough to
                    Now that we can relate the speed of a flow to its  deform easily, and so its advance speed slows
                  depth, we are in a position to establish the final   down. The width of the channel is thus forced to
                  relationship that determines the geometry of a lava  change, usually in the direction of getting wider, so
                  flow. This is the requirement that, as long as the  that the flux of lava from the vent is still accommo-
                  mass of lava being erupted from the vent every   dated by the flow. Finally all of this process must go
                  second, M , does not change, the same flux of lava  on even though the flow may be advancing down
                          f
                  must be flowing at every point in the flow. The flux  the flank of a volcano, on which the ground slope
                  is the product of the cross-sectional area of the   varies with distance from the vent. And further-
                  flow and the flow speed, and the area is the depth  more, it is quite possible that there are changing
                  of lava in the channel multiplied by the channel  conditions in the magma reservoir supplying the
                  width, w . Thus we have                     vent which mean that the erupted mass flux also
                         c
                                                              changes with time.
                  M = ρ w d U                          (9.8)
                   f     c  c
                  and although all three of  w ,  d , and  U may be  9.7 Lengths of lava flows
                                         c  c
                  changing (and even ρ may change a little if some of
                  the gas bubbles in the flow burst and collapse), they  It will be clear from the above description that ana-
                  must do so in such a way that the product of all four  lyzing the motion of lava flows, and predicting how
                  quantities remains constant.                they will evolve as they advance down the slopes of
                    The implication of these equations can be sum-  a volcano, is not easy. One important property of
                  marized as follows. Lava is erupted from a vent   flows does seem to be fairly predictable, however,

                  with a given viscosity and a negligible (or at least  and this is the maximum distance to which a single
                  very small) yield strength. It flows downslope, and  cooling-limited flow unit can travel. Recall eqn 9.1
                  immediately begins to cool at its upper and lower  that described the depth to which cooling can
                  edges. The cool material on the top surface of the  penetrate a flow. It might be expected that when
                  flow is carried to the front, falls onto the ground  most of the thickness of a flow was cooled it would
                  and is pushed sideways to form a levée on either  stop moving. To investigate this we take the ratio
                  side of the central channel. The partly solidified  between the cooling depth and some characteristic
                  levée material behaves as a Bingham plastic with a  thickness scale of the flow. The number that is used
                  yield strength that determines the levée width and  is called the equivalent diameter of the flow, d ,
                                                                                                      e
                  thickness. The core of hot material in the central  and it is defined as four times the cross-sectional
                  channel behaves as a Newtonian fluid and pushes  area of the flowing lava divided by its wetted
                  the levées aside until the combination of the width  perimeter. The reason for this definition can be
                  of the channel, the flow speed of the lava, and the  explained as follows.
                  depth of the lava can just accommodate the flux  Imagine lava flowing in a lava tube that has a
                  coming from the vent. The simplest situation is one  circular cross-section with radius r. Then its cross-
                                                                             2
                  in which the depth of lava in the channel is just  sectional area is πr and, if the lava completely fills
                  equal to the depth of the inner edge of the levées.  it, all of the perimeter is wetted by the lava, so the
                  As the front of the flow advances, the material  wetted perimeter is 2πr. Then d is equal to four
                                                                                         e
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