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Magma drainage around rising gas slugs and burst overpressure in Strombolian eruptions: Geophysical Research Abstracts Vol. 13, EGU2011-5904, 2011 EGU General Assembly 2011

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Magma drainage around rising gas slugs and burst overpressure in Strombolian eruptions: Geophysical Research Abstracts Vol. 13, EGU2011-5904, 2011 EGU General Assembly 2011. / Del Bello, Elizabetta; Llewellin, Ed; Taddeucci, Jacopo et al.
2011.

Research output: Contribution to conference - Without ISBN/ISSN Abstract

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@conference{b8833ad6cd3f4ef185ec48a06b10e134,
title = "Magma drainage around rising gas slugs and burst overpressure in Strombolian eruptions: Geophysical Research Abstracts Vol. 13, EGU2011-5904, 2011 EGU General Assembly 2011",
abstract = "Strombolian activity is characterized by the recurrence of mildly-explosive eruptions that are driven by the rise and burst of discrete gas slugs which ascend rapidly through a more-or-less stagnant column of low-viscosity magma.Explosion dynamics and vigour, as observed at the surface, are mainly controlled by the slug{\textquoteright}s overpressure with respect to the ambient pressure. Depth of gas slug formation and the amount of gas in the slug are, in turn, known to influence the slug overpressure at burst.We present a physical model for the development of overpressure within a rising gas slug, which allows the overpressureat burst to be calculated. The model neglects inertial and viscous effects and demonstrates that significantoverpressure may develop even in their absence. Results show that the thickness of the magma film draining aroundthe rising slug exerts a primary control on the development of overpressure: a thicker liquid film (i.e. a more viscousmagma) results in a greater burst overpressure. Film thickness is represented dimensionlessly through thegeometrical parameter A{\textquoteright}, which is the fraction of the conduit section occupied by draining magma in the slugregion. A number of models exist which relate A{\textquoteright} to conduit diameter and liquid viscosity. We test these modelsby performing scaled laboratory experiments on air slugs ascending in cylindrical pipes filled with liquids with arange of viscosities. The best-fit model is used to calculate A{\textquoteright} for the range of non-dimensional flow conditionsexpected in volcanic conduits.We apply our model to calculate burst overpressure of Strombolian eruptions using appropriate volcano-scale parameters. Model outputs are compared with previously published estimates of bursting overpressure derived froma broad dataset of eruptions at Stromboli; our results show that magma-static load and geometrical factors alonecan account for the observed overpressures during slug-driven explosions.",
author = "{Del Bello}, Elizabetta and Ed Llewellin and Jacopo Taddeucci and Piergiorgio Scarlato and Stephen Lane",
year = "2011",
month = apr,
language = "English",

}

RIS

TY - CONF

T1 - Magma drainage around rising gas slugs and burst overpressure in Strombolian eruptions

T2 - Geophysical Research Abstracts Vol. 13, EGU2011-5904, 2011 EGU General Assembly 2011

AU - Del Bello, Elizabetta

AU - Llewellin, Ed

AU - Taddeucci, Jacopo

AU - Scarlato, Piergiorgio

AU - Lane, Stephen

PY - 2011/4

Y1 - 2011/4

N2 - Strombolian activity is characterized by the recurrence of mildly-explosive eruptions that are driven by the rise and burst of discrete gas slugs which ascend rapidly through a more-or-less stagnant column of low-viscosity magma.Explosion dynamics and vigour, as observed at the surface, are mainly controlled by the slug’s overpressure with respect to the ambient pressure. Depth of gas slug formation and the amount of gas in the slug are, in turn, known to influence the slug overpressure at burst.We present a physical model for the development of overpressure within a rising gas slug, which allows the overpressureat burst to be calculated. The model neglects inertial and viscous effects and demonstrates that significantoverpressure may develop even in their absence. Results show that the thickness of the magma film draining aroundthe rising slug exerts a primary control on the development of overpressure: a thicker liquid film (i.e. a more viscousmagma) results in a greater burst overpressure. Film thickness is represented dimensionlessly through thegeometrical parameter A’, which is the fraction of the conduit section occupied by draining magma in the slugregion. A number of models exist which relate A’ to conduit diameter and liquid viscosity. We test these modelsby performing scaled laboratory experiments on air slugs ascending in cylindrical pipes filled with liquids with arange of viscosities. The best-fit model is used to calculate A’ for the range of non-dimensional flow conditionsexpected in volcanic conduits.We apply our model to calculate burst overpressure of Strombolian eruptions using appropriate volcano-scale parameters. Model outputs are compared with previously published estimates of bursting overpressure derived froma broad dataset of eruptions at Stromboli; our results show that magma-static load and geometrical factors alonecan account for the observed overpressures during slug-driven explosions.

AB - Strombolian activity is characterized by the recurrence of mildly-explosive eruptions that are driven by the rise and burst of discrete gas slugs which ascend rapidly through a more-or-less stagnant column of low-viscosity magma.Explosion dynamics and vigour, as observed at the surface, are mainly controlled by the slug’s overpressure with respect to the ambient pressure. Depth of gas slug formation and the amount of gas in the slug are, in turn, known to influence the slug overpressure at burst.We present a physical model for the development of overpressure within a rising gas slug, which allows the overpressureat burst to be calculated. The model neglects inertial and viscous effects and demonstrates that significantoverpressure may develop even in their absence. Results show that the thickness of the magma film draining aroundthe rising slug exerts a primary control on the development of overpressure: a thicker liquid film (i.e. a more viscousmagma) results in a greater burst overpressure. Film thickness is represented dimensionlessly through thegeometrical parameter A’, which is the fraction of the conduit section occupied by draining magma in the slugregion. A number of models exist which relate A’ to conduit diameter and liquid viscosity. We test these modelsby performing scaled laboratory experiments on air slugs ascending in cylindrical pipes filled with liquids with arange of viscosities. The best-fit model is used to calculate A’ for the range of non-dimensional flow conditionsexpected in volcanic conduits.We apply our model to calculate burst overpressure of Strombolian eruptions using appropriate volcano-scale parameters. Model outputs are compared with previously published estimates of bursting overpressure derived froma broad dataset of eruptions at Stromboli; our results show that magma-static load and geometrical factors alonecan account for the observed overpressures during slug-driven explosions.

M3 - Abstract

ER -