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Formation and dynamics of magma reservoirs

Research output: Contribution to journalArticle

Original languageEnglish
Article number20190019
Number of pages30
JournalPhilosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
Volume377
Issue number2139
Early online date7 Jan 2019
DOIs
DateAccepted/In press - 25 Oct 2018
DateE-pub ahead of print - 7 Jan 2019
DatePublished (current) - 7 Jan 2019

Abstract

The emerging concept of a magma reservoir is one in which regions containing melt extend from the source of magma generation to the surface. The reservoir may contain regions of very low fraction intergranular melt, partially molten rock (mush) and melt lenses (or magma chambers) containing high melt fraction eruptible magma, as well as pockets of exsolved magmatic fluids. The various parts of the system may be separated by sub-solidus rock or be connected and continuous. Magma reservoirs and their wall rocks span a vast array of rheological properties, covering as much as 25 orders of magnitude from high viscosity, sub-solidus crustal rocks to magmatic fluids. Timescales of processes within magma reservoirs range from very slow melt and fluid segregation within mush and magma chambers and deformation of surrounding host rocks to very rapid development of magma and fluid instability, transport and eruption. Developing a comprehensive model of these systems is a grand challenge that will require close collaboration between modellers, geophysicists, geochemists, geologists, volcanologists and petrologists.

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    Rights statement: This is the author accepted manuscript (AAM). The final published version (version of record) is available online via the Royal Society at https://royalsocietypublishing.org/doi/10.1098/rsta.2018.0019 . Please refer to any applicable terms of use of the publisher.

    Accepted author manuscript, 5 MB, PDF document

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