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258                                                            J. Martı ´ et al.


             Guillou-Frottier, 1999). Their conclusion is that the presence of far-field
             stresses can significantly modify the distribution and geometry of faulting.
             Regional extensional stresses shift the locations of the zones of minimal and
             maximal bending stresses, leading to both the formation of multiple faults and
             favouring the occurrence of deep faulting centred over the magma chamber
             roof. As long as the extension continues, fractures develop at a more vertical
             angle and propagate from the centre to the borders to create a wider dispersed
             fault zone.
             In conclusion, results from the available models agree that magma chamber
          geometry and load conditions are the two main controlling factors for ring-fault
          formation and, hence, the generation of collapse calderas. With few exceptions,
          models concur in predicting that sill-like chamber geometries are a necessary
          requirement. In addition, only the satisfaction of specific conditions seems to
          generate a favourable stress field for collapse: tension, regional doming, chamber
          overpressure combined with load increase by erupted products, and chamber
          underpressure.


          3.3. Restrictions and limitations of theoretical models
          Theoretical models contribute important semi-quantitative information comple-
          menting experimental models and field studies. However, as with all models, they
          also have restrictions and limitations that we discuss in this section.
             Similar to the analogue models, numerical models assume, with few exceptions,
          a homogenous crust. It is certainly a gross approximation to nature because country
          rocks are normally heterogeneous in composition and properties. Lithological
          heterogeneities can influence the stress field and the rock strength profile and,
          consequently, the development and propagation of fractures (e.g. Gudmundsson
          and Brenner, 2005).
             One of the main problems of existing models on caldera-collapse-formation
          processes is that fluid dynamics and rock mechanics are, in all cases, uncoupled.
          As mentioned above, in an ideal case, all physical processes should be simulated
          simultaneously, as processes occurring inside the chamber may affect those taking
          place in the country rock and vice versa.
             None of the discussed models succeeds in simulating dyke injection neither
          during collapse nor during tumescence. However, as mentioned before, the
          possibility of dyke injection is important during pre-caldera episodes as it can
          regulate (dis)equilibrium conditions inside the magma chamber. The impossibility
          of simulating dyke injection has further consequences: (i) dyke intrusions may
          significantly modify the physical properties of country rock, for example, its tensile
          or shear strengths, evidently affecting fault nucleation and propagation; and
          (ii) some interpretation of results obtained may be misinterpreted. Whereas some
          authors claim that ring fault or other collapse-controlling structures develop from
          the top of the magma chamber to the surface (e.g. Gray and Monaghan, 2004),
          others state that ring-fault nucleation at depth is not possible as any magma chamber
          rupture would lead to a dyke intrusion (e.g. Gudmundsson, 1998). Of course, these
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