Magma compressibility and the missing source for some dike intrusions

  • Eleonora Rivalta
    Department of Physics University of Bologna Bologna Italy.
  • Paul Segall
    Department of Geophysics Stanford University Stanford California USA.

書誌事項

公開日
2008-02
権利情報
  • http://onlinelibrary.wiley.com/termsAndConditions#vor
DOI
  • 10.1029/2007gl032521
公開者
American Geophysical Union (AGU)

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説明

<jats:p>Dike intrusions are often accompanied by localized deflation, interpreted as depressurizing magma chambers feeding the dike. In some cases the inferred volume decrease is a factor of 4 or 5 less than the volume increase of the dike. Here we explore whether this discrepancy can be explained by compressibility of the magma combined with the fact that cracks are much more compliant than equidimensional magma chambers. If pressure changes are small, the magma compressibility <jats:italic>β</jats:italic><jats:sub><jats:italic>m</jats:italic></jats:sub> is constant, and the dike ends up in hydrostatic equilibrium with an ellipsoidal magma chamber at the same depth, the ratio <jats:italic>r</jats:italic><jats:sub><jats:italic>V</jats:italic></jats:sub> of the volume of the crack to the volume lost by the chamber is <jats:italic>r</jats:italic><jats:sub><jats:italic>V</jats:italic></jats:sub> = 1 + 4<jats:italic>μβ</jats:italic><jats:sub><jats:italic>m</jats:italic></jats:sub>/3 > 1, where <jats:italic>μ</jats:italic> is the host rock rigidity. For gas poor magmas, <jats:italic>β</jats:italic><jats:sub><jats:italic>m</jats:italic></jats:sub> = 0.6–2 · 10<jats:sup>−10</jats:sup> Pa<jats:sup>−1</jats:sup> and <jats:italic>μ</jats:italic> = 3–25 GPa, we find 1.2 < <jats:italic>r</jats:italic><jats:sub><jats:italic>V</jats:italic></jats:sub> < 7.7. Large changes in magma compressibility due to gas exsolution increase <jats:italic>r</jats:italic><jats:sub><jats:italic>V</jats:italic></jats:sub>.</jats:p>

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