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Rapid remobilization of magmatic crystals kept in cold storasre

机译:冷藏的岩浆晶体的快速移动

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摘要

The processes involved in the formation and storage of magma within the Earth's upper crust are of fundamental importance to volcanology. Many volcanic eruptions, including some of the largest, result from the eruption of components stored for tens to hundreds of thousands of years before eruption. Although the physical conditions of magma storage and remobilization are of paramount importance for understanding volcanic processes, they remain relatively poorly known. Eruptions of crystal-rich magma are often suggested to require the mobilization of magma stored at near-solidus conditions; however, accumulation of significant eruptible magma volumes has also been argued to require extended storage of magma at higher temperatures. What has been lacking in this debate is clear observational evidence linking the thermal (and therefore physical) conditions within a magma reservoir to timescales of storage-that is, thermal histories. Here we present a method of constraining such thermal histories by combining timescales derived from uranium-series disequilibria, crystal sizes and trace-element zoning in crystals. At Mount Hood (Oregon, USA), only a small fraction of the total magma storage duration (at most 12 per cent and probably much less than 1 per cent) has been spent at temperatures above the critical crystallinity (40-50 per cent) at which magma is easily mobilized. Partial data sets for other volcanoes also suggest that similar conditions of magma storage are widespread and therefore that rapid mobilization of magmas stored at near-solidus temperatures is common. Magma storage at low temperatures indicates that, although thermobarometry calculations based on mineral compositions may record the conditions of crystallization, they are unlikely to reflect the conditions of most of the time that the magma is stored. Our results also suggest that largely liquid magma bodies that can be imaged geophysically will be ephemeral features and therefore their detection could indicate imminent eruption.
机译:地球上地壳内岩浆的形成和储存所涉及的过程对火山学至关重要。许多火山喷发,包括一些最大的火山喷发,是由于在喷发前储存了数万至数十万年的成分喷发而引起的。尽管岩浆储存和迁移的物理条件对于理解火山过程极为重要,但对它们的了解仍然相对较少。通常认为,富含晶体的岩浆爆发需要动员储存在接近固相线状态的岩浆。然而,也有人认为大量可爆发的岩浆体积的积累需要在更高的温度下扩展岩浆的储存。这场辩论缺乏的是清晰的观测证据,将岩浆储层中的热(以及物理)条件与储藏的时间尺度即热历史联系起来。在这里,我们提出了一种通过结合从铀系列不平衡,晶体尺寸和晶体中的痕量元素分带得出的时间尺度来限制这种热历史的方法。在胡德山(美国俄勒冈州),岩浆总储藏时间的一小部分(至多12%,可能远低于1%)花费在高于临界结晶度(40-50%)的温度下岩浆很容易动员。其他火山的部分数据集也表明,类似的岩浆储存条件已广泛存在,因此,在接近固相线温度的情况下,迅速移动岩浆是很普遍的。低温下的岩浆储存表明,尽管基于矿物成分的热压法计算可能会记录结晶条件,但它们不太可能反映岩浆存储大部分时间的条件。我们的研究结果还表明,可以通过地球物理成像的很大程度上为液体的岩浆体将是短暂的特征,因此对其进行检测可能表明即将爆发。

著录项

  • 来源
    《Nature》 |2014年第7489期|480-483|共4页
  • 作者单位

    Department of Earth and Planetary Sciences, University of California, Davis, One Shields Avenue, Davis, California 95616, USA;

    College of Earth, Ocean and Atmospheric Sciences, 104 Ocean Administration, Oregon State University, Corvallis, Oregon 97331, USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);美国《化学文摘》(CA);
  • 原文格式 PDF
  • 正文语种 eng
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  • 入库时间 2022-08-18 02:52:58

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