V31B-3023
Eruption cycles in a basaltic andesite system: insights from numerical modeling

Wednesday, 16 December 2015
Poster Hall (Moscone South)
Amanda B Clarke, Arizona State University, School of Earth & Space Exploration, Tempe, AZ, United States, Jean-Francois Smekens, Arizona State University, Tempe, AZ, United States and Mattia De' Michieli Vitturi, Istituto Nazionale di Geofisica e Vulcanolgia, Sezione di Pisa, Pisa, Italy
Abstract:
Persistently active explosive volcanoes are characterized by short explosive bursts, which often occur at periodic intervals numerous times per day, spanning years to decades. Many of these systems present relatively evolved compositions (andesite to rhyolite), and their cyclic activity has been the subject of extensive work (e.g., Soufriere Hills Volcano, Montserrat). However, the same periodic behavior can also be observed at open systems of more mafic compositions, such as Semeru in Indonesia or Karymsky in Kamchatka for example. In this work, we use DOMEFLOW, a 1D transient numerical model of magma ascent, to identify the conditions that lead to and control periodic eruptions in basaltic andesite systems, where the viscosity of the liquid phase can be drastically lower. Periodic behavior occurs for a very narrow range of conditions, for which the mass balance between magma flux and open-system gas escape repeatedly generates a viscous plug, pressurizes the magma beneath the plug, and then explosively disrupts it. The characteristic timescale and magnitude of the eruptive cycles are controlled by the overall viscosity of the magmatic mixture, with higher viscosities leading to longer cycles and lower flow rates at the top of the conduit. Cyclic eruptions in basaltic andesite systems are observed for higher crystal contents, smaller conduit radii, and over a wider range of chamber pressures than the andesitic system, all of which are the direct consequence of a decrease in viscosity of the melt phase, and in turn in the intensity of the viscous forces generated by the system. Results suggest that periodicity can exist in more mafic systems with relatively lower chamber pressures than andesite and rhyolite systems, and may explain why more mafic magmas sometimes remain active for decades.