Understanding seismogenic processes in the Southern Calabrian Arc: a geodynamic perspective

M. Tiberti, P. Vannoli, U. Fracassi, P. Burrato, V. Kastelic, G. Valensise
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引用次数: 19

Abstract

For any scientist working in seismotectonics, the Calabrian Arc represents the most challenging area of Italy. Lying on top of a subduction zone, it is characterised by a complex geological structure largely inherited from the early stages of the collision between the Africa and Eurasia plates. The current and extremely vigorous seismogenic processes, although generated by a mechanism driven by the subduction, are no longer a direct consequence of plate convergence. About one fourth of the largest Italian earthquakes concentrates in a narrow strip of land (roughly 200×70 km) corresponding to the administrative region of Calabria. The present-day seismicity, both shallow and deep, provides little help in detecting the most insidious seismogenic structures, nor does the available record of GPS-detected strains. In addition to its fierce seismicity, the Calabrian Arc also experiences uplift at rates that are the largest in Italy, thus suggesting that active tectonic processes are faster here than elsewhere in the country. Calabrian earthquakes are strong yet inherently elusive, and even the largest of those that have occurred over the past two centuries do not appear to have caused unambiguous surface faulting. The identified active structures are not sufficient to explain in full the historical seismicity record, suggesting that some of the main seismogenic sources still lie unidentified, for instance in the offshore. As a result, the seismogenic processes of Calabria have been the object of a lively debate at least over the past three decades. In this work we propose to use the current geodynamic framework of the Calabrian Arc as a guidance to resolve the ambiguities that concern the identification of the presumed known seismogenic sources, and to identify those as yet totally unknown. Our proposed scheme is consistent with the location of the largest earthquakes, the recent evolution of the regions affected by seismogenic faulting, and the predictions of current evolutionary models of the crust overlying a W-dipping subduction zone.
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了解南卡拉布里亚弧的孕震过程:地球动力学视角
对于任何从事地震构造学研究的科学家来说,卡拉布里亚弧代表着意大利最具挑战性的地区。它位于俯冲带的顶部,其特点是复杂的地质结构,很大程度上继承了非洲板块和欧亚板块碰撞的早期阶段。当前和极其强烈的孕震过程,虽然是由俯冲驱动的机制产生的,但不再是板块收敛的直接结果。大约四分之一的意大利最大地震集中在与卡拉布里亚行政区域相对应的狭长地带(大约200×70公里)。当今的地震活动性,无论是浅层还是深层,都无法帮助我们探测到最隐蔽的发震构造,gps探测到的菌株的现有记录也是如此。除了剧烈的地震活动外,卡拉布里亚弧的隆起速度也是意大利最大的,这表明这里的活跃构造过程比意大利其他地方要快。卡拉布里亚地震很强烈,但本质上难以捉摸,即使是过去两个世纪发生的最大地震,似乎也没有造成明确的地表断层。已确定的活动构造不足以全面解释历史地震活动记录,这表明一些主要的孕震源仍未被确定,例如在近海。因此,至少在过去的三十年里,卡拉布里亚的孕震过程一直是激烈争论的对象。在这项工作中,我们建议使用卡拉布里亚弧的当前地球动力学框架作为指导,以解决涉及识别假定已知孕震源的模糊性,并识别那些尚未完全未知的孕震源。我们提出的方案与最大地震的位置、发震断裂影响区域的近期演化以及当前w向俯冲带上地壳演化模型的预测相一致。
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