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                    72  CHAPTER 5









                                                                             Fig. 5.7 A sequence of four frames
                                                                             extracted from a movie showing the
                                                                             rise of magma in a vent on Kilauea
                                                                             volcano, Hawai’I, during an episode of
                                                                             gas pistoning. In frames (a) to (c) the
                                                                             accumulation of gas beneath the lava
                                                                             crust causes the lava crust to rise
                                                                             progressively higher in the vent. In
                                                                             frame (d) the gas has escaped from
                                                                             beneath the lava crust by tearing the
                                                                             crust apart in a minor explosion and
                                                                             the level of the lava in the vent has
                                                                             fallen. (Photography by Tim Orr,
                                                                             Hawaiian Volcano Observatory,
                                                                             courtesy of the U.S. Geological
                                                                             Survey.)


                  the overlying magma, whereas in 5000 seconds it  with higher initial gas contents and with lower rise
                  will rise 50 m. Thus, during rise of magma over a  speeds. Higher gas contents lead to larger bubbles
                  given distance, the slower rising magma allows the  because the bubbles start to form at deeper levels
                  bubbles to travel further relative to their starting  (supersaturation occurs at deeper levels) and thus
                  position in the magma. The further bubbles are able  the bubbles grow more by decompression during
                  to rise through the magma, the greater the oppor-  ascent. Smaller rise speeds lead to bigger bubbles
                  tunity for collision with other bubbles and there-  because the bubbles have more time to grow by
                  fore for coalescence. In the extreme, the magma  diffusion during ascent. For bubbles in basaltic
                                                                                                  −1
                  itself may be stationary and the bubbles rise up  magmas rising at speeds greater than 1 m s , the
                  through it to reach the surface of a lava pond in the  maximum size that the bubbles reach is typically

                  vent. Ascent of the bubbles through such magma  between 1 and 10 mm and essentially no bubble
                                                                                                     −1
                  gives the initially largest bubbles the greatest pos-  coalescence occurs. At rise speeds less than 1 m s ,
                  sible opportunity for overtaking smaller bubbles  although the total gas content still influences bub-
                  and reaching the runaway stage in which single,  ble size, coalescence is the dominant factor deter-
                  large bubbles form, filling the entire dike or con-  mining the final bubble size – the slower the rise
                  duit. In basaltic magmas this effect can manifest  speed the greater the final size of the bubble. When
                  itself in vigorous  Strombolian explosions or in  bubble growth is controlled by coalescence, bub-
                  more gentle “gas pistoning” (Fig. 5.7). These styles  bles in basaltic magmas can grow to sizes greater
                  of eruption are discussed in detail in Chapter 7.  than 1 m.
                    Figure 5.8 shows the influence of rise speed on  Figure 5.8 shows one specific example of how
                  bubble growth for two different magma gas con-  bubble growth is influenced by rise speed in a
                  tents (the amount of gas initially dissolved in the  basaltic magma. In the case illustrated, the critical
                  magma at depth) in a basaltic magma that does not  rise speed determining whether or not coalescence
                                                                               −1
                  become supersaturated. The graph shows that at  occurs is about 1 m s . The value of this critical rise
                  magma rise speeds of greater than 1 m s −1  the final  speed varies as a function of magma gas content
                  size reached by a bubble by the time it is erupted  and magma viscosity. At larger gas contents the crit-
                  depends linearly on the rise speed and also on the  ical rise speed is greater. This is because, as long as
                  total gas content. Bubbles grow larger in magmas  supersaturation does not become important, in
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