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Ignimbrite flare-ups and their drivers: A New Zealand perspective

Journal

EARTH-SCIENCE REVIEWS
Volume 162, Issue -, Pages 65-82

Publisher

ELSEVIER
DOI: 10.1016/j.earscirev.2016.09.007

Keywords

Continental arc magmatism; Ignimbrite flare-up; Caldera-forming eruption; Mantle flux; Magmatic-tectonic; Taupo Volcanic Zone

Funding

  1. University of Auckland for Postdoctoral
  2. Mighty River Power

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Ignimbrite flare-ups are periods of intense silicic volcanism characterized by multiple caldera-forming eruptions that together evacuate 10(3) to 10(4) km(3) of magma. Ignimbrite flare-ups of different ages and from different tectonic settings have been well documented; however, in the literature, the distinction between an 'ignimbrite flare-up' and a 'magmatic flare-up' is not always obvious. We argue that the distinction is an important one as magmatic flare-ups do not always necessitate an ignimbrite flare-up, and thus the drivers for both require more investigation. Here we focus our review on the North Island continental arc of New Zealand, which is rarely included in published comparative studies of arc magmatism. Yet, it is well known for its extraordinary production of high-silica rhyolite and intensity of caldera-forming eruptions relative to other active arc systems, and a highly resolved understanding of the subduction plate boundary characterized by a rapidly migrating arc. Much of the present-day geologic footprint of the active part of the arc, the Taupo Volcanic Zone (TVZ), was established in a remarkable ignimbrite flare-up event between similar to 350 and similar to 280 ka. During this time, eight ignimbrite-forming eruptions occurred, evacuating similar to 3000 km(3) of magma, and formed calderas that pepper a 90 x 40 km area. We divide the flare-up into 3 pulses of caldera activity, and track the magmatic input from the build-up to the first pulse, through to the final caldera forming eruption of the last pulse. Based on a comparison between New Zealand and other documented examples worldwide, we propose three ignimbrite flare-up categories based on their longevity and intensity. Most ignimbrite flare-ups last 10(6) to 10(7) years (categories 2 and 1, respectively), erupt magma volumes exceeding 10(4) km(3) and are interpreted to be driven from depth by high mantle flux (i.e. magmatic flare-ups). Here, we draw attention to a new, much shorter time scale flare-up (10(4) to 10(5) years; category 3) as exemplified by the similar to 350 to similar to 280 TVZ example. Using the erupted volumes for several documented flare-ups at the three category timescales, we calculate a mantle input based on published silicic intrusive:extrusive ratios and isotopically derived ratios for basaltic input. Our results show that category 3 ignimbrite flare-up eruption rates typically exceed 10 km(3) kyr(-1), have multiple caldera-forming eruptions, and are defined by mantle input rates that can be sustained through the duration of the ignimbrite flare-up and are at least an order of magnitude above the longer timescale category 1 and 2 ignimbrite flare-ups. For the TVZ, such high ignimbrite productivity over just tens of thousands of years, is related to an efficient feedback loop between high mantle flux and accelerated rifting that together are responsible for a remarkably thin and extended continental crust. We argue, that despite its unique nature relative to other continental arcs, there may be important magmatic-tectonic feedbacks that can be gleaned from the highly resolved record of caldera and ignimbrite volcanism in the TVZ, and applied to studying short timescale ignimbrite flare-ups elsewhere. (C) 2016 Elsevier B.V. All rights reserved.

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