School of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK.
Science. 2017 Mar 24;355(6331). doi: 10.1126/science.aag3055.
Volcanoes are an expression of their underlying magmatic systems. Over the past three decades, the classical focus on upper crustal magma chambers has expanded to consider magmatic processes throughout the crust. A transcrustal perspective must balance slow (plate tectonic) rates of melt generation and segregation in the lower crust with new evidence for rapid melt accumulation in the upper crust before many volcanic eruptions. Reconciling these observations is engendering active debate about the physical state, spatial distribution, and longevity of melt in the crust. Here we review evidence for transcrustal magmatic systems and highlight physical processes that might affect the growth and stability of melt-rich layers, focusing particularly on conditions that cause them to destabilize, ascend, and accumulate in voluminous but ephemeral shallow magma chambers.
火山是其下潜在岩浆系统的表现。在过去的三十年中,人们对上层地壳岩浆房的经典关注已经扩展到考虑整个地壳的岩浆过程。地壳的跨壳视角必须平衡低速(板块构造)的熔体生成和分异速率与许多火山爆发前在上地壳中快速熔体积累的新证据。协调这些观察结果引发了关于地壳中熔体的物理状态、空间分布和寿命的激烈辩论。在这里,我们回顾了跨壳岩浆系统的证据,并强调了可能影响富含熔体层生长和稳定性的物理过程,特别关注导致它们失稳、上升和在大量但短暂的浅层岩浆房中积累的条件。