Page 367 - Caldera Volcanism Analysis, Modelling and Response
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342                                                       Agust Gudmundsson


          pressure becomes zero or, in fact, in the underpressure model negative. This
          problem follows from Equations (1)–(4) and was discussed in the context of these
          equations. When dealing with petroleum reservoirs and hydraulic fractures injected
          from drill holes, it is normally assumed that the fluid must have pressure in excess of
          the minimum principal compressive stress to keep the hydraulic fracture open at its
          contact with the drill hole (Valko and Economides, 1995; Charlez, 1997; Yew,
          1997). By contrast, in the underpressure model, the dyke fractures are supposed to
          remain open when the magma pressure is less than the minimum principal
          compressive stress. It remains to be explained how magma chambers can behave in
          this way and under what conditions.
             A second problem, not mentioned by Gudmundsson and Nilsen (2006), is the
          shear stress generated in the roof of a supposed-to-be empty magma chamber. For a
          chamber with a top at the depth of 4–5 km, for example, an empty cavity at the
          chamber top would result in a shear stress of at least 50–60 MPa. By contrast, the in
          situ shear strength, twice the tensile strength, is likely to be about 10 MPa or less. In
          fact, driving shear stresses (stress drops) in most earthquakes are 1–10 MPa (Scholz,
          1990). So the following question must be answered: how can the rocks sustain the
          shear stresses necessary for an empty cavity to form at many kilometres depth?
             Perhaps, the most serious problem for the underpressure model, from a general
          volcanological point of view, is the poor correlation between collapse (caldera)
          volume and combined volumes of extrusive and intrusive material leaving the
          chamber during the caldera eruption. For calderas in basaltic edifices the volume
          correspondence is normally poor (Walker, 1988). In fact, the two best-documented
          large caldera collapses in recent decades, that of Fernandina in Galapagos in 1968
          (Filson et al., 1973; Munro and Rowland, 1996) and that of Miyakejima in Japan in
          2000 (Geshi et al., 2002) had hardly any eruptions at all. And even if dykes were
          associated with the volcano-tectonic events leading to these collapses, realistic dyke-
          volume estimates are only fractions of the collapse volumes.
             There exist many other careful estimates showing similar lack of volume
          correspondence (Smith, 1979; Williams and McBirney, 1979). An interesting aspect
          of the lack of volume correspondence is that not only do many calderas subside
          without significant eruption or intrusion, but there are also several large-volume
          explosive eruptions that show no major ring-fault slip at the eruption site (Lavallee
          et al., 2006). For example, an explosive eruption at 1600 AD of the Huaynaputina
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          volcano in Peru produced about 11 km DRE of eruptive materials and unspecified
          volume of intrusive materials. This large explosive eruption was associated with two
          small collapse structures, one about 1 km and the other about 0.6 km in diameter
          (and thus too small to be really classified as calderas), with a combined volume of
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          0.043 km or about 0.4% of the eruptive volume (Lavallee et al., 2006).
             The examples of lack of volume correspondence serve to illustrate the point that
          there is clearly no critical eruptive/intrusive volume depending on the size of the
          chamber that can be regarded as a threshold for ring-fault formation or slip.
          Hundreds of eruptions and dyke injections occur in volcanoes worldwide every
          century, and of greatly varying volumes, but very few result in ring-fault formation
          or slip on existing ring faults. In terms of purely empirical theories of caldera
          formation, such as the underpressure model, it is not easy to account for the rarity
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