埃特纳火山基于全球导航卫星系统的长期变形(意大利)

Mimmo Palano , Stefano Calcaterra , Piera Gambino , Benedetto Porfidia , Federica Sparacino
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引用次数: 1

摘要

我们通过考虑2004.42-2018.95期间收集的密集GNSS数据集,估计了埃特纳火山的长期速度场。为了正确地将火山变形与背景构造变形隔离开来,我们使用了32个主要位于西西里岛西北部和东南部的台站,定义了一个新的局部参考系(称为MERF23)。计算的长期速度场很好地突出了西北翼和东部翼之间的对比模式。西北翼的特点是总体呈放射状,变形较小,主要与调查期间发生的通货膨胀和通货紧缩有关。东侧的特征是强烈的向海运动,速度从Pernicana断层(北部边界)的~60 mm/yr到Aci-Trezza断层(南部边界)的约29 mm/yr不等,这清楚地表明,到目前为止,侧翼不稳定仍然是埃特纳山的主要变形类型。还探测到沿火山外围基底的小型收缩,以及小型隆起;这两种模式都归功于不同过程的同时作用,如局部和区域构造以及长期岩浆隆起。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
GNSS-based long-term deformation at Mount Etna volcano (Italy)

We estimated a long-term velocity field for Mount Etna volcano by taking into account a dense GNSS dataset collected during the 2004.42 - 2018.95 period. To properly isolate the volcanic deformation from the background tectonic one, we defined a new local reference frame (termed MERF23) by using 32 stations mainly located in north-western and south-eastern Sicily. The computed long-term velocity field well highlights contrasting patterns between the north-western flank and the eastern one. The north-western flank was characterized by a general radial pattern with small deformations, mainly related to inflation and deflation episodes occurred during the investigated period. The eastern flank was characterized by a vigorous seaward motion, with rates ranging from ∼60 mm/yr on the Pernicana fault (northern boundary) to ∼29 mm/yr along the Aci Trezza fault (southern boundary), clearly evidencing as flank instability remains by far the predominant type of deformation at Mount Etna. A small contraction along the peripheral base of the volcano, coupled with a small uplift has been also detected; both patterns lend credit to the concurrent action of different processes as local and regional tectonics as well as long-term magmatic doming.

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