Magma chamber recharge at Vesuvius in the century prior to the eruption of A.D. 79

  1. D.J. Morgan1,
  2. S. Blake2,
  3. N.W. Rogers2,
  4. B. De Vivo3,
  5. G. Rolandi3 and
  6. J.P. Davidson4
  1. 1Department of Earth Sciences, Open University, Walton Hall, Milton Keynes MK7 6AA, UK; Department of Earth Sciences, University of Durham, Durham DH1 3LE, UK; and LGCA, Université Joseph Fourier, 38400 Saint Martin D'Hères, France
  2. 2Department of Earth Sciences, Open University, Walton Hall, Milton Keynes MK7 6AA, UK
  3. 3Departimento di Scienze della Terra, Università di Napoli “Federico II”, Via Mezzacannone 8, 80314 Napoli, Italy
  4. 4Department of Earth Sciences, University of Durham, Durham DH1 3LE, UK

    Abstract

    Evaluating volcanic hazards requires knowledge of the processes that trigger eruptions and the nature and timing of geophysical signals related to these processes. One approach to addressing this need is to link geophysically observable signals (e.g., those related to seismic, aeromagnetic, inflationary, or degassing processes) to pre-eruptive magmatic events deduced (in hindsight) from studies of erupted magmas. Here we present data on sanidine crystals from the A.D. 79 eruption of Vesuvius that show abrupt changes in Ba concentration caused by magma chamber recharge events prior to eruption. These changes have been degraded by diffusion during the time interval between recharge and eruption, and we have determined the length of this time interval by modeling the measured Ba concentration gradients. The results identify three distinct recharge events in the century before the eruption, the most recent occurring ∼20 yr beforehand.

    Footnotes

      • Accepted 15 May 2006.
      • Received 27 January 2006.
      • Revision received 12 May 2006.
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