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意大利埃特纳火山上裂缝、岩脉和火山喷发的规模分布:对岩浆房体积和喷发潜力的影响。

Size distributions of fractures, dykes, and eruptions on Etna, Italy: Implications for magma-chamber volume and eruption potential.

作者信息

Scudero Salvatore, De Guidi Giorgio, Gudmundsson Agust

机构信息

Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Nazionale Terremoti, Via di Vigna Murata 605, 00143, Rome, Italy.

Department of Biological, Geological and Environmental Sciences - Earth Sciences Section - University of Catania, Corso Italia, 57, 95129, Catania, Italy.

出版信息

Sci Rep. 2019 Mar 11;9(1):4139. doi: 10.1038/s41598-019-40563-0.

DOI:10.1038/s41598-019-40563-0
PMID:30858418
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6412001/
Abstract

The main magma source for eruptions on Etna (Italy) is poorly constrained. Here we use data on the size distributions of volcanic fissures/feeder-dykes, crater cones, dyke thicknesses, and lava flows to estimate the average magma volume flowing out of the chamber during eruptions and the volume of the chamber. For the past four centuries the average magma volume leaving the chamber during each eruption is estimated at 0.064 km. From the theory of poroelasticity the estimated chamber volume is then between 69 and 206 km. For comparison, a sill-like, circular chamber (an oblate ellipsoid) 1 km thick and 14 km in diameter would have a volume of about 154 km. The elastic strain energy stored in the host rock during inflation of such a chamber is about 2.8 × 10 J. Estimating the surface energy of a typical dyke-fracture as about 10 J m, the results suggest that the stored strain energy is sufficient to generate a dyke-fracture with an area of about 28 km. The average strike-dimension of volcanic fissures/feeder-dykes in Etna is about 2.7 km. It follows that the estimated strain energy is sufficient to generate a feeder-dyke with a strike-dimension of 2-3 km and with a dip-dimension as great as 10 km, agreeing with the maximum estimated depth of the magma chamber.

摘要

埃特纳火山(意大利)喷发的主要岩浆源情况不明。在此,我们利用火山裂缝/供浆岩脉、火山口锥、岩脉厚度和熔岩流的尺寸分布数据,来估算喷发期间从岩浆房流出的平均岩浆量以及岩浆房的体积。在过去四个世纪里,每次喷发期间离开岩浆房的平均岩浆量估计为0.064立方千米。根据孔隙弹性理论,估算出的岩浆房体积在69至206立方千米之间。相比之下,一个1千米厚、直径14千米的岩床状圆形岩浆房(扁球体)的体积约为154立方千米。在这样一个岩浆房膨胀过程中,储存在围岩中的弹性应变能约为2.8×10焦耳。将典型岩脉裂缝的表面能估算为约10焦耳/平方米,结果表明储存的应变能足以产生一个面积约为28平方千米的岩脉裂缝。埃特纳火山火山裂缝/供浆岩脉的平均走向尺寸约为2.7千米。由此可见,估算出的应变能足以产生一条走向尺寸为2至3千米、倾向尺寸高达10千米的供浆岩脉,这与岩浆房的最大估算深度相符。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/7e9371dfac37/41598_2019_40563_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/30d3c8b43f2f/41598_2019_40563_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/a0bdc6340237/41598_2019_40563_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/e0f15e441dfe/41598_2019_40563_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/fe22ee09462a/41598_2019_40563_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/7e9371dfac37/41598_2019_40563_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/30d3c8b43f2f/41598_2019_40563_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/a0bdc6340237/41598_2019_40563_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/e0f15e441dfe/41598_2019_40563_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/fe22ee09462a/41598_2019_40563_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e3f8/6412001/7e9371dfac37/41598_2019_40563_Fig5_HTML.jpg

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本文引用的文献

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2
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Emergence of scaling in random networks.随机网络中幂律分布的出现。
冰岛克拉夫拉火山维蒂角砾岩的地层重建:对地热区引发爆发性喷发的喷发前条件的洞察。
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