JOURNAL OF PETROLOGY VOLUME 38 NUMBER 12 PAGES 1635–1644 1997 The Brittle–Ductile Transition in High-Level Granitic Magmas: Material Constraints DONALD B. DINGWELL∗ ¨ BAYERISCHES GEOINSTITUT, UNIVERSITAT BAYREUTH, D-95440 BAYREUTH, GERMANY RECEIVED JANUARY 1997; ACCEPTED AUGUST 1997 Granitic magmas residing at high levels in the continental crust may be subjected to stress transients on a wide range of time-scales. The origins of the stress transients may be internal, deriving from the volume evolution of the magmatic system, or external such as the rapid release of stresses during tectonic and volcanically derived earthquakes. The strain response of the granitic magma is critically dependent upon its viscosity and the magnitude and time-scale of the application or release of the stress. The response of the magma may be either ductile or brittle. Prediction of the expected response of the magma requires an accurate and reliable method for determining the location in temperature and time-scale of the transition of the response of the melt from ductile to brittle by analogy to the glass transition determined by frequency domain relaxation studies. The application of the Maxwell criterion, which treats the magma as a viscoelastic medium in the linear stress–strain regime, provides such a method. Application of this method requires accurate viscosity and elastic modulus data for the magma. The consequence of intersecting the glass transition in a system where the total strains are significant is brittle failure of the melt phase. Here, the material constraints on the brittle–ductile transition of granitic magma are reviewed. The transition of the mechanical response of magma from ductile to brittle behavior can have enormously important consequences for heat, mass and momentum transfer. Despite this observation, and the fact that the lithologies produced both by eruptive and high-level intrusive silicic magmas give clear evidence of both types of deformation, the characterization of this transition and the quantification of the conditions necessary to achieve it are not well understood for magmas. Fluid-saturated granitic magmas residing at high levels in the Earth’s crust can potentially experience the transition from viscous to brittle deformation under a variety of sources of transient stress related to their internal chemical and physical evolution and the external circumstances of their emplacement and/or eruption (Dingwell, 1995). Significant experimental progress towards quantification of the conditions necessary for the transition, and prediction of the material response of the magma to it, has been achieved in the past few years, chiefly in the field of experimental deformation of magma. Here the quantification of the properties of magma which are chiefly responsible for controlling the mechanical response of high-level granitic systems is reviewed. High-level granitic magma is likely to be subject to transient stresses stemming from a variety of internal and external stresses. Those stresses may contain volume and/or shear components. The internal stresses include those stemming from volume changes associated with boiling and crystallization phenomena as well as ascent of the magma as a whole. The external stresses include sources of transient stresses within the crust such as tectonic stresses whose release results in earthquakes and ‘volcanic’ transient stresses where co-eruptive microearthquakes signal transient stress release in or below the volcanic edifice. The combination of silicic melt chemistry and high-level emplacement enhances the probability of brittle response of the magma via at least three of several depth-related factors: (1) at shallow depths, magmatic degassing strongly increases the magma viscosity via dehydration, foaming and crystallization; (2) the reduced temperatures of the magma and host rock enhance ∗Fax: 49 921 55 3769. e-mail: [email protected] Oxford University Press 1997 KEY WORDS: brittle; ductile; glass transition; melt; viscosity INTRODUCTION JOURNAL OF PETROLOGY VOLUME 38 NUMBER 12 DECEMBER 1997 their propensity for brittle response; (3) surface-related tectonically or volcanically generated gravitational instabilities can generate very high unloading strain rates for magma at subvolcanic depths, and magma–water contact in volcanic conduits or at the surface can generate shock waves associated with explosive interactions. VISCOELASTICITY AND THE GLASS TRANSITION IN MAGMA The response of a largely molten (<30% crystals) granitic magma to the application of transient stresses is dominated by the behavior of the melt phase. As such, the most important first step in the quantification of the mechanical response of high-level silicic granitic magmas is an adequate characterization of the glass transition in such magma. Figure 1 illustrates the calorimetric behavior of a granitic melt in the vicinity of the glass transition. The transition from solid-like behavior at lower temperature to liquid-like behavior at higher temperature causes a sharp increase in the derivative thermodynamic properties of the melt such as heat capacity and expansivity as relaxation modes involving the polyanionic network structure of the melt are activated by self-diffusion with increasing temperature (Dingwell, 1990). The zone of mixed response between the glassy and liquid regimes corresponds to a partially relaxed viscoelastic response of the system. The significance of the glass transition for the mechanical response of magma lies in the aforementioned phrases ‘solid-like’ and ‘liquid-like’ behavior. Simply put, the liquid-like response of the melt to the application of stresses is entirely viscous or ductile whereas the solidlike response is entirely elastic at small strains (i.e. in the linear stress–strain regime) but brittle at the higher strains commonly encountered in magmas in nature. It should be noted that the width of the zone of hysteresis between the fully glassy and fully liquid responses of the melt (Fig. 1) is on the order of several tens of degrees. Translated through the temperature dependence of viscosity, this width corresponds to several log units of viscosity, which in turn implies that the viscoelastic response of the melt can span several log units of strain rate in nature. The experimental deformation of melts at low strain and variable strain rate demonstrates clearly the width of the zone of viscoelastic response in silicate melts (Dingwell & Webb, 1990; Webb & Dingwell, 1995). Such viscoelasticity data, expressed as the real (strain is in phase with the applied stress) and imaginary (strain is out of phase with the applied stress) components of the viscoelastic response of a calc-alkaline rhyolite to the application of torsional stresses, are illustrated in Fig. 2. The width of the peak corresponding to the out-of-phase component of deformation indicates the width of the Fig. 1. Variation of heat capacity, C p, as a function of temperature. The glass transition expresses itself as a sharp increase in the derivative thermodynamic properties of the melt phase. An example of such a derivative property is the heat capacity. At low temperatures the heat capacity values correspond to the solid-like or glassy response of the melt phase to temperature changes. The melt structure responds in a disequilibrium fashion to temperature changes whereby the vibrational component of the melt entropy can vary in thermal equilibrium, but the configurational component of the entropy does not. This is because the self-diffusion of the cations and anions is required by the mechanism of structural reorganization or relaxation to higher-temperature equilibrium states. The diffusivity provides a kinetic threshold which must be overcome on a specific time-scale of heating rate before metastable equilibrium can be achieved. At temperatures higher than the glass transition such a metastable equilibrium, involving both vibrational and configurational components of structural change with temperature, is achieved. The addition of the configurational component of the heat capacity to its glassy component at T g generates much higher metastable liquid values of the derivative property. The portion of the derivative property curves near the glass transition temperature is transient, and is path dependent in nature. The form of the curve in this interval depends on material properties, the heating rate and (in the case of heating) on the thermal history (and thus the quenched-in structure) of the glass. Data for a haplogranitic melt with added B2O3 redrawn from Knoche et al. (1992). viscoelastic response of a rhyolite in the linear stress–strain regime. This result demonstrates that viscoelastic response of a melt can be expected to be 2 log units of strain rate slower that the relaxation strain rate calculated by using the Maxwell relation (s=g/M), where s is the relaxation time, g the viscosity and M the elastic modulus. NON-NEWTONIAN FLOW AND BRITTLE FAILURE This onset of the viscoelastic response of the melt phase has a corresponding phenomenon in nonlinear experiments where the deformation of the melt is no longer independent of the deformation rate and the strains reach much higher values, similar to those anticipated in magmas in nature. Experiments to define the onset of the non-Newtonian rheological response of the melt phase have been conducted using a variety of deformation 1636 DINGWELL BRITTLE–DUCTILE TRANSITION IN GRANITIC MAGMAS onset of non-Newtonian rheology and ultimate brittle failure of the melt can be accessed through the predicted relaxation time or strain rate of the Maxwell relation via incorporation of the constant offset noted above. PARAMETERIZATION—NEWTONIAN VISCOSITIES Fig. 2. The viscoelastic response of a dry calc-alkaline rhyolitic melt. The sample of remelted, bubble- and crystal-free obsidian was subjected to torsional stresses in the frequency (x) range of mHz to kHz and the viscoelastic response to the forced oscillations was recorded. Here, the shear modulus is plotted against the frequency (normalized to the shear relaxation time) of the applied torsional stress. The growth of the imaginary or ‘out-of-phase’ component of the stress–strain relationship indicates the onset of significant mixed (viscous + elastic), partially relaxed strain response to the applied stress. The width of the range of the observable imaginary component is several log units in frequency or strain rate. This width translates through the activation energy of the shear stress relaxation time into a width, at a constant frequency, of several tens of degrees Celsius. These experiments are performed under conditions of variable strain rate but very low total strains, with the result that elastic strains or energy storage, rather than brittle failure, are the consequence. Nevertheless, the location of the onset of elastic response in time–temperature space is a fairly accurate indicator of the conditions necessary for the material in question to exhibit nonNewtonian flow and brittle failure in corresponding nonlinear time domain experiments (see Fig. 3). Redrawn from Webb (1992). geometries (Li & Uhlmann, 1970; Simmons et al., 1982; Hessenkemper & Bru¨ckner, 1988; Webb & Dingwell, 1990), and all yield the fundamental type of response illustrated here in Fig. 3. The strain-rate-independent viscosity of the melt encountered at low strain rates begins to deviate from this Newtonian behavior at a characteristic strain rate ~3·5 log units slower than the relaxation strain rate calculated from the Maxwell relation. The consequence of this breakdown of the Newtonian flow of the melt is that the apparent viscosity decreases with increasing strain rate, in a phenomenon known as shear thinning. The melt cannot shear thin indefinitely and with sustained application of stress the melt eventually ‘breaks’ or fails at a point where the microscopically accumulated strain defects have weakened the tensile strength of the melt to a value less than the applied stress. Despite the small difference between the onset of significant elastic response of the melt phase in the linear regime and the onset of non-Newtonian rheology in the nonlinear regime, the two events appear to be closely coupled and are generated by the same fundamental phenomenon, the inability of the melt to relax on the time-scale of the deformation. Thus the prediction of the The necessary inputs for the application of the Maxwell criterion to the prediction of the onset of non-Newtonian rheology are viscosity and elastic modulus data. Comparison of longitudinal wave propagation data from ultrasonic studies and shear viscosity data from concentric cylinder viscometry confirms that the shear viscosity and volume viscosities of silicate melts are similar in magnitude. Therefore a sufficiently general description of the P–T–X dependence of the shear viscosity should suffice for fulfilling the viscosity data needed as input. Until recently, the database for shear viscosities of rhyolitic melts was not complete enough to justify a general model because of the strongly nonlinear dependence of viscosity on water content and reciprocal absolute temperature. Recent experimental improvements have now largely filled in the gap of observations (Dingwell et al., 1996a, 1996b; Richet et al., 1996) for the previously under-investigated, high-viscosity region, with the result that Hess & Dingwell (1996) were able to provide a nonArrhenian model for melt viscosity. Figure 4 illustrates the essential features of the model predictions. The addition of water generates the well-known nonlinear decrease of viscosity vs added water content and an increasingly nonArrhenian dependence of the viscosity on temperature. Both features exert strong controls on the predicted viscosities and only now is it possible to model the rheological consequences of degassing of rhyolitic melts to a reasonable degree of accuracy. For example, at a strain rate of 10–1·5 s–1, a calc-alkaline rhyolite containing 2 wt % water would experience the onset of non-Newtonian behavior at a temperature of 800°C. Many high-level granites may evolve to the situation where several relatively incompatible elements which are normally present at trace levels in granitic magmas achieve minor or even major element concentration levels of 0·5 to several weight percent in the melt phase. Figure 5 illustrates that several of these elements can also influence significantly the viscosity of the melt phase. Predictive models are generally not yet available to incorporate the combined effects of water and these other elements. As a general rule, the effects of combinations of enriched elements on the viscosity of the melt phase are not expected to be nonlinear or nonadditive. One example is the combined influence of boron and water on the viscosity of a granitic melt (Fig. 6). Interestingly, the viscoelastic response of the melt (see below), although 1637 JOURNAL OF PETROLOGY VOLUME 38 NUMBER 12 DECEMBER 1997 Fig. 3. shifted to much lower temperature by the addition of components such as boron, phosphorus or fluorine, does not appear to vary in internal character in the partially relaxed region (Fig. 7). By analogy, we can conclude that the onset and path of non-Newtonian viscosity in these specialized granitic melts will be unaffected except in the sense that the temperature at which they occur will be shifted. CHEMICAL AND PHYSICAL INFLUENCES ON VISCOELASTICITY High-level granite magmas, in a volatile-saturated state, are complex geo-materials consisting of significant volume fractions of suspended crystals and vesicles. The influence of the physical incorporation of these phases on the rheology and glass transition of rhyolitic melts is illustrated in Fig. 8, where frequency domain data for the viscoelastic response of a rhyolitic melt with spherical crystals and vesicles are compared. As was the case for chemically induced shifts of the rheology, there are no changes in the internal structure of the partially relaxed behavior, but the temperature shifts because of the inclusion of crystals and bubbles are considerable. These results corroborate time domain studies of the viscosity of crystal and bubble suspensions, and indicate that the physical influences of suspended bubbles and crystals up to contents of 30 vol. % can shift the viscosity by up to a log unit. Under the rapid application of pressure or shear stress perturbations to be expected to result from transient stresses in high-level granitic magmas, the bubbles suspended in the vesicular magma may not have sufficient time to respond by viscous deformation of their shape as was the case in Fig. 8. In such a situation, the bubbles 1638 DINGWELL BRITTLE–DUCTILE TRANSITION IN GRANITIC MAGMAS Fig. 3. The non-Newtonian response of a dry calc-alkaline rhyolitic melt, a calc-alkaline andesite, a tholeiitic basalt and a synthetic nephelinite. The sample of remelted, bubble- and crystal-free obsidian was subjected to longitudinal stresses over a range of strain rates and the onset of non-Newtonian response to the longitudinal stresses was recorded. The deviation of the response of the melt from a constant ratio of stress to strain-rate or apparent viscosity indicates a partially unrelaxed response of the melt to the applied strain. The difference in time-scale between the onset of the non-Newtonian response and the calculated relaxation time of the melt phase is ~3·5 log units. This is slightly larger than the prediction that would be made from the width of the relaxation peak in Fig. 2, but the approximation that the onset of the non-Newtonian response of the melt phase can be scaled by a constant offset to the calculated relaxation time of the melt remains valid. Thus the viscosity of the melt, the time-scale of the deformation and the temperature of the system govern the onset of unrelaxed response and non-Newtonian flow of the melt phase. Redrawn from Webb & Dingwell (1990). are likely to contribute to a viscosity increase which can be modeled in a similar fashion to equations used for crystal suspensions [e.g. the Stokes–Einstein equation and derivative formulations; see Dingwell et al. (1993) for a review]. Torsional deformation experiments of the type discussed above yield shear modulus data in the mHz to kHz region which are comparable in magnitude. The influence of water on the elastic moduli of rhyolitic or granitic melts is not well known. It is unlikely, however, to lead to a shift in values of the elastic moduli outside of the bounds presented above. ELASTIC MODULI The predictive power of the Maxwell criterion for viscoelastic response of the liquid phase also requires an adequate description of the unrelaxed elastic moduli of the melt phase. Experimental measurements of the longitudinal modulus of silicate melts using MHz ultrasonic techniques yield moduli that vary with melt compositions within the relatively tight bounds of 3–30 GPa. MAGMA STRENGTH Given the relatively good constraints on the prediction of non-Newtonian rheology and eventual brittle failure of the melt phase provided above, we now turn to the consideration of the strength or failure criteria for these melts. The strength of complex materials such as magmas 1639 JOURNAL OF PETROLOGY VOLUME 38 NUMBER 12 DECEMBER 1997 Fig. 4. Parameterization of the dependence of the relaxed Newtonian shear viscosity of calc-alkaline rhyolitic melts on water content and temperature. The influence of pressure on the viscosity of hydrous calc-alkaline rhyolites can be neglected up to pressures of several kilobars. (a) illustrates the influence of water content on the viscosity of the melt for a series of isotherms. The extremely nonlinear decrease of the melt viscosity with increasing water content has been parameterized by an exponential function. (b) illustrates the temperature dependence of the viscosity of hydrous calc-alkaline rhyolitic melts at a series of compositions with constant water content. The significant curvature of the dependence of melt viscosity on the reciprocal absolute temperature has been parameterized using a Tamann–Vogel–Fulcher, reduced temperature fit. Using this parameterization of the dependence of viscosity on water content and temperature, the onset of non-Newtonian flow, leading to brittle failure, can be predicted in time–temperature space. Reproduced after Hess & Dingwell (1996). Fig. 5. The individual influence of a variety of chemical components commonly enriched in certain granitic and related magmatic to magmatohydrothermal lithologies on viscosity. These data give an indication of the relative viscosities to be expected in the hydrous equivalent melts; however, the combined influence of water and excess secondary components such as those illustrated here has not yet been sufficiently investigated to generate a predictive model. The fact that the influence of water is the greatest and that the viscosities of mixtures in silicate melts are in general highly nonlinear means that simple additions of the viscosity influences of the individual components on the viscosity of a hydrous highly specialized granitic melt will probably significantly overestimate the viscosity. More data are needed. Reproduced after Dingwell et al. (1997). 1640 DINGWELL BRITTLE–DUCTILE TRANSITION IN GRANITIC MAGMAS Fig. 6. The influence on viscosity (portrayed as an isokom temperature) of the combination of boron and water added to the composition of a calc-alkaline granitic melt. The curve of the combined influence of boron and water was generated for this specific case by considering the combined influence of (H2O + B2O3)/6. Such a combination cannot be generalized and the roots of its empirical success lie in the structural interaction of water and boron in this granite melt. Specific interaction of other elements with water and each other are likely to require other parameterizations. Reproduced after Romano et al. (1996). is highly under-investigated. There are, however, several starting points from which we can begin to build an appraisal of magma strength, and these are summarized below and in Table 1. We are interested primarily in tensile strength because in complex geo-materials this is likely to have a value considerably lower than either the shear or compressive strength. The theoretical limit of the tensile strength of the melt phase may be taken as its elastic modulus, here the tensile or Young’s modulus. For a pure melt the unrelaxed Young’s modulus has a value of the same order of magnitude as the equivalent (unrelaxed) shear and bulk moduli (i.e. several tens of GPa; Bansal & Doremus, 1986). In practice, melts never reach these levels of cohesion and their tensile breaking strength is 2–3 log units lower. Fiber elongation experiments on the nonNewtonian flow of rhyolite indicate a tensile strength of the shear thinned liquid of ~108·5 Pa (Webb & Dingwell, 1990). The fibers employed in those experiments were annealed at temperatures slightly above the glass transition to a fully relaxed state and subsequently subjected to tensile stresses that were large enough to drive their Fig. 7. The influence of chemistry on the viscoelasticity of granitic melts is illustrated with the examples of additions of several weight percent of the components B2O3, P2O5 and F2O–1 to a calc-alkaline granitic melt. Each of the components shifts the temperature of the onset of the viscoelastic behavior considerably through the influence on the relaxed shear viscosity. Apart from this shift in the onset temperature, the viscoelastic response of the melt is little influenced by the addition of these components despite their probably significant influence on melt structure. On the basis of the results presented here, no significant influence on the viscoelastic response, and, by analogy, the onset of nonNewtonian flow in nonlinear processes, is expected with the addition of water to these melts, apart from the temperature shift caused by the shift of the relaxed shear viscosity. G/G x represents the ratio of the real and imaginary components of the shear modulus to the value at infinite frequency. Redrawn from Bagdassarov et al. (1993). 1641 JOURNAL OF PETROLOGY VOLUME 38 NUMBER 12 DECEMBER 1997 Fig. 8. The physical influence of bubbles (a) and bubbles + crystals (b) on the viscoelastic response (the shear modulus, G) of a rhyolitic melt. The presence of bubbles in the rhyolitic melt decreases the viscosity by up to 1 log unit in the frequency range investigated. The viscoelastic region is shifted accordingly. The addition of crystals to the bubble suspension increases the viscosity by a similar amount and again the viscoelastic region is shifted accordingly. The primary influence on the viscoelastic response of the rhyolitic melt is through the influence on the shear viscosity up to the levels of crystals and bubbles illustrated here in the investigated frequency region. Nonlinear flow of vesicular and highly crystalline rhyolitic melts may generate distinct rheological response. The labels 9/9, 16/16 and 40/40 correspond to the crystallinity/porosity of the individual samples. Redrawn from Bagdassarov & Dingwell (1993) and Bagdassarov et al. (1994). (See Figs 2 and 7 for definitions of the plotted variables.) rheological response into the non-Newtonian regime outlined above. Because the fiber breakage occurred after a period of significant deformation via non-Newtonian flow, the microstructure of the melt phase must have recorded a cumulative record of the non-Newtonian deformation which would presumably lead to weakening of the fiber. The application of stresses in those experiments was at a relatively low strain rate and it is possible that crystal- and bubble-free rhyolitic melts in nature, when rapidly exposed to a transient stress, could exhibit slightly stronger behavior. The experimental evidence to date indicates that no significant compositional dependence of the tensile strength of the melt phase is to be expected. 1642 DINGWELL BRITTLE–DUCTILE TRANSITION IN GRANITIC MAGMAS Table 1: Strength estimates for magma Material Strength (Pa) Method Theory (T) or Source experiment (E) Silicate melt 1010 Elastic moduli T 1 Rhyolitic melt 108·5 Fiber failure E 2 Hydrous vesicular melt 106·5 Decrepitation E 3 Dome lava 106·5 Curvature T 4 Dome lava 106·5 Fragmentation E 5 1, Bansal & Doremus (1986); 2, Webb & Dingwell (1990); 3, Romano et al. (1996); 4, Mungall (1995); 5, Alidibirov & Dingwell (1996a). The presence of other phases in a granitic magma will in general contribute to a lowering of the tensile strength via the production of spatial variations in the strength of the bulk phase, which, in turn, generate spatial stress inhomogeneities in the stress field of the magma. Thus the magma is likely to develop stress concentrations locally whose relaxation may impose failure conditions on adjacent areas of the magma. Most crystalline phases possess a relatively high strength in comparison with that of the melt phase. Vesicles of fluid phases have, of course, negligible internal tensile strengths but their nucleation and growth may lead to compositional gradients in the liquid envelope surrounding each vesicle. Water concentration gradients generated during the diffusioncontrolled growth of bubbles in a water-saturated rhyolitic magma, for example, can lead to significant local spatial variations in the rheology of the melt phase, thus generating the possibility of stress concentration near the bubble surfaces. Very few experimental data are currently available to quantify these effects in detail. The case for a vesicular magma with water-filled vesicles has been experimentally addressed by Romano et al. (1996), who demonstrated clearly, on the basis of the decrepitation pressures of fluid inclusions in glasses, that the effective tensile strength of hydrous granitic melts containing vesicles can be as low as 2 log units less than that obtained for bubble-free melts. Mungall et al. (1996) modeled those observations in terms of the volume stresses distributed throughout the melt phase during rapid cooling of the vesicular magma. Water concentration gradients in vesicular magma cause significant shifts in the rheology of the melt and create volume stresses via the influence of water on the molar volume of the melt. Mungall et al. (1996) concluded that tensile ‘gradient’ stresses in the immediate vicinity of the vesicles could be generated that would be large enough to overcome the tensile strength of the melt phase locally. In many volcanic dome magmas the geometry of the vesicles is extremely tortuous, far from the sub-spherical geometry of the experiments described above. In such materials, the local embayments of high curvature will lead to stress concentrations which should further weaken the magma as a result of purely geometrical constraints (Mungall, 1995). In addition, if the crystal and vesicle volume fractions of a magma come into intimate contact, separated perhaps only by a thin film wetting of the melt phase, then the strength of the magma may also be adversely affected (Proussevitch et al., 1993). The subjection of magmatic samples to well-controlled transient stresses has recently been placed on a much more systematic experimental basis by the development of the so-called ‘fragmentation’ bomb (Alidibirov & Dingwell, 1996a, 1996b). This device is capable of subjecting magma samples, mechanically equilibrated under pressures up to 200 bars and temperatures up to 950°C, to stress transients that overcome the tensile strength of the magma. Experimental series in which the magnitude of the stress transient is systematically varied reveal that highly crystalline and vesiculated magma dome samples have characteristic tensile strengths in the range of 106−107 Pa. Experiments in which the vesicularity and crystallinity of the magma are systematically varied are at present under way. If the response of the magma is entirely brittle then the question arises as to the quantification of the production of surfaces during deformation. A number of formulations exist for the quantification of the brittle response of materials (Cook & Pharr, 1990). These include, for example, the so-called ‘fracture toughness’. A sampling of hydrous natural rhyolites has been studied by Gerth & Schnapp (1996). The systematic investigation of fracture toughness for magmatic geomaterials has not yet been initiated. This remains an important research goal for the future. 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