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                                                                               MAGMA MIGRATION    33


                 larger, respectively, than the average strain rates  grows sideways along the boundary, which locally
                 elsewhere in the mantle where convection is taking  increases the average strain rate. Also, the crustal
                 place without any melting.                   rocks are cooler than those in the mantle, and
                   The way in which a rock responds to being  therefore closer to their plastic–elastic transition
                 deformed, i.e., its rheology, depends on its compo-  temperature for any given strain rate. Thus both the
                 sition, its temperature, and the strain rate imposed  lower temperature of the overlying rocks and the
                 on it. If the temperature of a given hot rock is   increase in strain rate acting on them will act
                 kept constant and the strain rate applied to it is  together to make the creation of fractures particu-
                 increased, its response eventually changes from  larly likely as a plume head reaches the base of the
                 that of a very viscous liquid, i.e., a plastic solid, to  crust. Note that the increased strain rate applies to
                 that of a brittle elastic solid. Alternately, keeping  the rocks inside the top of the plume as well as to
                 the strain rate constant and decreasing the temper-  the crustal rocks above; thus the process of coales-
                 ature will also trigger the change from plastic to  cence of existing large melt veins into dikes can
                 elastic behavior and initiate fracturing. Diapirically  occur within the plume head itself.
                 rising masses of rock are always moving from hotter
                 into cooler surroundings, and so the onset of frac-
                 turing will occur whenever the rheological bound-  3.4 Dike propagation
                 ary between the plastic and elastic responses of
                 the host rocks is crossed, and this is likely to hap-  Wherever the change from plastic deformation to
                 pen at higher temperatures, and therefore at greater  brittle fracture of rocks occurs, fractures start to
                 depths, for larger, more rapidly rising diapiric bod-  grow from any feature that can concentrate the
                 ies than smaller, slower ones.               stress – this could be a particularly sharp-cornered
                   It is very difficult to predict exactly the condi-  interface between three crystals as described in
                 tions under which elastic to plastic transitions in  section 2.4.2 or some accidental defect in the inter-
                 rock behavior will occur in the Earth because it is  nal structure of a single mineral grain. As soon as a
                 hard to simulate mantle conditions in the laborat-  fracture forms in the crust above a region contain-
                 ory. The problem is not so much in producing the  ing magma, the liquid will start to flow into the
                 required temperatures and pressures but in dealing  fracture to fill the space created. A major property
                 with the time scales. If we are prepared to wait one  of brittle fractures is that the rate at which the sharp
                                  7
                 year, that is ∼3 × 10 s, to conduct an experiment   tip of the fracture can propagate into the unfrac-

                 in which a rock sample is deformed by 100%, i.e.,  tured rock ahead of it is limited only by the speed of
                 compressed to about half its thickness and double  sound in the rock (a sound wave is just a wave of
                 its cross-sectional area, in a high-pressure, high-  deformation of the material in which it is traveling).
                 temperature apparatus in the laboratory, the average  In practice the crack-tip propagation speed is some-
                                        s , which is 30 million
                 strain rate will be ∼3 × 10 −8 −1            what less than the actual sound speed, but it is still
                 times faster than in the mantle. Extrapolations  on the order of a few kilometers per second, and at
                 made across this enormous difference in time scale  first sight it is tempting to predict that dikes should
                 are not very reliable.                       grow at this rate. However, there is a limit to the
                   However, it is clear that the heads of mantle  speed at which magma can flow into a narrow, open-
                 plumes reaching the base of the overlying crust   ing crack. The speed is controlled by the crack width
                 are particularly likely to cause their host rocks to  and the magma viscosity, and also by the widths of
                 fracture. Two factors combine to cause this. First, a  the network of smaller veins that are feeding melt
                 change in bulk composition occurs, with the crust  toward the crack. This magma flow speed will be
                 being less dense than the mantle in general, includ-  very much less than the speed of sound in rock –
                 ing the hot material in the plume. Thus the plume  typically more than a thousand times less. Thus in
                 buoyancy is lost and the top of the plume ceases   practice it is the flow speed of the liquid magma
                 to rise. The material below it continues to rise,   in the narrow veins that determines the speed at
                 however, and the plume head flattens out and  which the dike as a whole can grow upward.
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