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                                                                                    LAVA FLOWS   127


                                                              (although still high enough to cause the explosive
                                                              activity of course) so that the speeds of the clots
                                                              leaving the vent are not too large. “In sufficient
                                                              numbers” implies that the mass eruption rate from
                                                              the vent is high; this has two effects. First, if there
                                                              is a large mass flux there will be a large number of
                                                              clots in flight at any one time and so they form
                                                              a dense cloud, with clasts on the outside shielding
                                                              those near the middle from being able to “see” the
                                                              sky and radiate away their heat. Second, with a
                                                              large mass flux each clot that lands on the ground
                                                              will be buried by the later-arriving clots more
                  Fig. 9.3 A rhyolite flow forming the ∼80 m high Novarupta
                                                              quickly, again conserving its heat. When the accu-
                  dome marking the site of the vent for the June 1912
                                                              mulation rate of hot clasts is large enough they
                  eruption in Alaska that emplaced the Valley of Ten
                  Thousand Smokes ignimbrite. (Photograph taken by   completely merge together, the slightly cooled
                  T. Miller, courtesy U.S. Geological Survey.)  outer skins of the clots being reheated by the hot
                                                              interiors as heat is shared by conduction, and the
                 9.2 Origin of lava flows                      whole assemblage moves downhill away from the
                                                              vent as a rootless lava flow (Fig. 9.4). The tem-
                 The simplest way that a lava flow can form is when  perature of such a flow may be only a few kelvins to
                 magma overflows from a volcanic vent onto the   a very few tens of kelvins less than that of a flow
                 surrounding surface and moves downhill under  formed directly by effusion from a vent.
                 gravity. We have seen that most magmas exsolve  It is very common for basaltic magmas erupting
                 volatiles as they approach the surface, and thus  as fire-fountains to form rootless lava flows as part
                 should not be surprised to find that most active lava  of a spectrum of features. If clots lose almost no
                 flows contain significant numbers of volcanic gas  heat, and coalescence is complete, a flow forms. If
                 bubbles which, after the flow has cooled and atmo-  clots lose rather more heat, their skins may reach
                 spheric air has replaced the original gas in the inter-  a high enough temperature, after heat sharing with
                 connected bubbles, are quite vesicular. We know  the interiors, to weld together, but the interiors
                 from the evidence in Chapter 5 that the high juve-  may then be too cool to deform significantly and so

                 nile volatile content of many magmas has the poten-  no flow occurs; instead a welded spatter rampart
                 tial to make them erupt explosively. If the magmas  forms (Fig. 9.5). Finally, if too much heat is lost in
                 erupt on the deep ocean floor on Earth, the pres-  flight, the clots accumulate as a warm but un-
                 sure of the overlying water greatly reduces the  welded scoria deposit (Fig. 9.6). Figure 9.7 shows
                 amount of gas that can exsolve, and so many of  qualitatively how the combinations of magma volatile
                 these magmas behave as though they had a low  content and mass flux through the vent control this
                 volatile content and do not erupt explosively.  range of possible features.
                   However, even when volatile-rich magmas erupt  In principle the same range of processes can occur
                 subaerially, there is still a way that lava flows can be  in more evolved magmas. However, in dacitic
                 formed. All that is required is that at least some of  magmas it is not common for the combinations
                 the clots of fragmented magma ejected through the  of volatile content and eruption rate to favor this.
                 vent into a fire-fountain or into the base of an erup-  Rhyolitic magmas, on the other hand, are much
                 tion column should fall back to the ground near the  more likely to erupt at high mass fluxes and,
                 vent sufficiently quickly and in sufficient numbers.  because of high volatile contents, very explosively.
                 “Sufficiently quickly” is important so that the clots  The resulting great efficiency of magma fragmenta-
                 do not have time to cool much while they are in  tion causes the average sizes of the pumice clasts
                 flight. Short travel times are encouraged by the  that are formed to be small which, together with
                 magma having a relatively low volatile content  the high mass flux, makes the jet of clasts and gas
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