Page 377 - Caldera Volcanism Analysis, Modelling and Response
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352                                                         Thomas R. Walter



               1. Introduction

               Large-volume ash-flow eruptions and sporadic cones typically align along the
          circumference of a caldera basin (e.g., Walker, 1984; Lipman, 1997; Cole et al.,
          2005). Studies of caldera structures show that groups of eruption feeder pathways
          form discordant intrusive bodies with near-circular geometries in map view.
          Intrusions along a circle around a volcanic center were described in detail in the
          early twentieth century (Clough et al., 1909); these intrusions are referred to as ring-
          complexes. Ring-complexes are very common for volcanoes with surface expressed
          calderas (Richey, 1935; Smith and Bailey, 1968; Lipman, 1984), and different types
          are distinguished. The geometry of ring-complexes comprise circular or angular,
          inwardly dipping, vertical, and outwardly dipping dikes of variable thickness. These
          can be singular intrusion events or multiple dikes, forming basaltic or silicic sheets.
          Intrusion dynamics of ring-complexes include those that generate their own
          propagating fractures or those that reactivate existing fracture zones. In the latter
          case, the dike may follow predefined faults of regional tectonic and/or volcano-
          tectonic origin.
             In association with collapsed calderas, two main types of ring-complexes can be
          distinguished (see Table 1): inwardly dipping (often 30–451) concentric dikes,
          referred to as cone sheets (Bailey et al., 1924), and near-vertical or often outwardly
          dipping concentric dikes intruded parallel to (or into) the ring-faults, referred to as
          ring-dikes (Anderson, 1936; Billings, 1943). In the mid-1930s, E.M. Anderson
          developed the first mathematical theory for the development of ring-complexes
          (Anderson, 1936); a fluctuating pressure within a deep parabolic magma chamber is
          thought to be responsible for the formation of ring-complexes. The two different
          types of ring-complexes are therefore defined geometrically as well as genetically;
          while cone sheets are thought to form during stages of caldera floor uplift
          (inflation), ring-dikes form during stages of caldera floor subsidence (deflation).
          This work focuses on the different conditions and geometries of ring-dike
          formation related to caldera subsidence.
             Ring-dikes ideally intrude along the ring-fault and form a closed ring; more
          commonly, they only partially intrude into a ring-fracture to form curved or
          segmented dikes (Billings, 1943; Bonin, 1986). Ring-dikes are often only a few
          centimeters or meters thick. However, old eroded caldera system ring-dikes can
          reach massive dimensions, wider than 10 km and more than 0.5 km thick. Classic
          ring-dikes were described for volcanic systems in Scotland; for instance, at Glencoe
          caldera, a deeply eroded caldera with inverted relief, caldera subsidence affects an
          oval-shaped area and activated boundary faults (Clough et al., 1909). Although
          similar mechanisms were applied to most intrusive complexes in the British
          Volcanic Tertiary Province (Richey, 1935), newer studies suggest that some of these
          ring-complexes are lopolithic intrusions associated with inflation and doming
          (O’Driscoll et al., 2006).
             A major difficulty in ring-dike studies is that exposures are usually poor and
          often obscured by sedimentary caldera infill or other intrusive bodies (O’Driscoll
          et al., 2006; Kennedy and Stix, 2007). It has been shown that the geometry of a
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