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首页> 外文期刊>Journal of Volcanology and Geothermal Research >Variations in eruptive style and depositional processes associated with explosive, phonolitic composition, caldera-forming eruptions: The 151 ka Sutri eruption, Vico Caldera, central Italy
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Variations in eruptive style and depositional processes associated with explosive, phonolitic composition, caldera-forming eruptions: The 151 ka Sutri eruption, Vico Caldera, central Italy

机译:与爆发力,火山岩成分,火山口形成爆发有关的爆发方式和沉积过程的变化:意大利中部维科火山口的151 ka Sutri喷发

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摘要

Vico Volcano in central Italy, experienced a complex eruptive history (419-95 ka). The Vico volcanic edifice was constructed by voluminous (50 km~3) leucitite composition effusive lava flows and minor explosive activity over a 50 ka period (305-258 ka). The summit of the edifice was destroyed during the Sutri eruption (151 ka) that resulted in the formation of the 8 km caldera depression.rnA revised stratigraphy for the eruptive products produced by the Sutri eruption (Sutri Formation) is proposed, based on extensive field observations, detailed stratigraphic logging and petrographic analysis; the Sutri A unit consists of a fallout deposit of limited dispersal; the Sutri B unit consists of a small volume, variably welded pumice-rich ignimbrite; the Sutri C unit is a lithic and spatter clast-rich co-ignimbrite lag-flow breccia; the Sutri D unit is a fines-depleted pumice-rich ignimbrite; Sutri (E1-E3) subunits consist of spatter clast-rich ignimbrite; Sutri E4 (sbx) is a spatter clast-rich co-ignimbrite lag-flow breccia; the Sutri E4 (lsbx) subunit is a lithic, pumice and spatter clast-rich co-ignimbrite lag-flow breccia; the climactic Sutri E5 unit is a variably zeolitised spatter and pumice-rich ignimbrite (with lithic-rich base; Sutri E4 flsbx) to the west). The reconstruction of the Sutri eruption leading up to and including formation of the Vico Caldera based on the new stratigraphy of the Sutri Formation, consists of three distinct phases:rnPhase 1-Initial Plinian activity produced a fallout deposit (Sutri A) deposited to the south, followed by partial eruption column collapse that generated a pyroclastic flow directed to the south/southeast (Sutri B). Vent widening in response to vent-wall rock instabilities and increased magma discharge rate overloaded the eruption column with dense, lithic debris resulting in southward collapse and deposition of a thick co-ignimbrite lag breccia in the deflation zone (Sutri C). A change in dast supply at vent from lithic clast-dominated to pumice clast-dominated produced a fines-depleted ignimbrite, Sutri D (plbx) prior to cessation of activity in the south.rnPhase 2-Shortly following the initial Plinian phase or partially overlapping, decompression of the magma chamber in response to partial magma chamber roof block collapse promoted explosive fragmentation of magma at the base of the conduit (as pumice) and led to the opening of a new vent in the north. Sustained mixing of highly vesiculated, grey pumice clasts and dense, poorly vesiculated, black spatter clasts occurred both in the conduit and in the eruption column and subsequent column collapse produced a small volume pyroclastic flow directed to the north, dominated by dense, black spatter clasts (Sutri E1-E3). Phase 3-Sustained eruptive activity continued in the north and increased magma discharge rate likely then resulted in great instability of the magma chamber roof and surrounding wall rocks of the progressively draining magma chamber. The eruption column collapsed radially depositing vast quantities of lithic clasts, spatter clasts and some pumice clasts into the deflation zone as co-ignimbrite lag-flow breccias (Sutri E4 sbx, lsbx), signalling the onset of caldera collapse. Eruption column collapse also produced a radially distributed, pyroclastic flow that deposited a moderate volume ignimbrite (Sutri E5) with a lithic-rich base (Sutri E4 flsbx) at proximal localities in the west. Final caldera collapse occurred shortly following emplacement of Sutri E5 presumably in response to evacuation of the magma chamber and final collapse of the magma chamber roof. We infer from the eruption dynamics that progressive collapse of the magma chamber roof occurred culminating in final climactic and post-eruptive caldera collapse.
机译:意大利中部的维科火山经历了复杂的喷发历史(419-95 ka)。维科火山大厦是由大量的(50 km〜3)白云石组成的涌出熔岩流和较小的爆炸活性(在50 ka的时间段内(305-258 ka))构成的。苏特里火山喷发(151 ka)期间摧毁了大厦的顶峰,导致形成了8 km的火山口凹陷。rn根据广泛的油田范围,提议对苏特里火山喷发(苏特里岩层)产生的喷发物地层进行修订观测,详细的地层测井和岩石学分析; Sutri A装置由分散度有限的沉淀物组成; Sutri B单元由少量,可变焊接的富浮石火成石组成; Sutri C单元是一块片状和飞溅的碎屑丰富的共燃物滞后角砾岩。 Sutri D单元是一种富含细粉的浮石着火物; Sutri(E1-E3)亚基由飞溅丰富的碎屑火成岩组成。 Sutri E4(sbx)是一种飞溅丰富的碎屑共燃滞后角砾岩; Sutri E4(lsbx)亚基是一种由石块,浮石和飞溅组成的富含碎屑的共燃物滞后角砾岩。高海拔的Sutri E5装置是一个可变的沸石飞溅物和浮石富集的火成岩(基石含量丰富; Sutri E4 flsbx位于西侧)。苏特尔火山喷发的重建过程基于新的苏特尔岩层地层,包括维科破火山口的形成,包括三个阶段:阶段1-初始普利尼活动活动产生了沉积物(Sutri A)沉积到南部,然后是部分喷发的柱塌陷,产生了一个热碎屑流,流向南/东南(Sutri B)。火山口因火山岩壁失稳而变宽,岩浆排放速率增加,使喷发柱充满致密的石屑碎屑,导致向南塌陷,并在放气区沉积了厚的共燃滞后角砾岩(Sutri C)。阶段2在最初的Plinian阶段之后不久或部分重叠,在南部停止活动之前,出气口的粪便供应从石块为主的浮石变为浮石为主的浮石产生了细粉状的火成岩Sutri D(plbx)。 ,岩浆室的减压响应部分岩浆室屋顶块塌陷,促进了岩浆在管道底部的爆炸性破碎(如浮石),并导致北部新的通风孔打开。高泡状灰色浮石碎屑和稠密,微泡性差的黑色飞溅碎屑的持续混合在导管和喷发柱中均发生,随后的柱塌陷产生少量的碎屑碎屑流,流向北部,以密集的黑色飞溅碎屑为主(Sutri E1-E3)。 3期持续的喷发活动在北部继续进行,岩浆排放速率增加可能导致岩浆室顶板和逐渐排水的岩浆室周围围岩的巨大不稳定性。喷发柱塌陷成放射状沉积,形成大量的碎屑,飞溅碎屑和一些浮石碎屑,作为共着火的滞后角砾岩(Sutri E4 sbx,lsbx)进入放气区域,表明火山口塌陷的开始。喷发柱的塌陷也产生了放射状分布的火山碎屑流,在西部近端沉积了中等体积的火成岩(Sutri E5),其上有富含岩性的碱(Sutri E4 flsbx)。 Sutri E5放置后不久,最终破火山口坍塌发生,可能是由于岩浆室的撤离和岩浆室屋顶的最终塌陷。我们从喷发动力学中推断,岩浆室屋顶的逐渐塌陷最终导致了最终的高潮和喷发后的火山口塌陷。

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  • 来源
    《Journal of Volcanology and Geothermal Research 》 |2009年第4期| 225-255| 共31页
  • 作者单位

    School of Geosciences, P.O Box 28E, Monash University, Clayton, Victoria 3800, Australia School of Geosciences, P.O Box 28E, Monash University, Clayton, Victoria 3800, Australia;

    School of Geosciences, P.O Box 28E, Monash University, Clayton, Victoria 3800, Australia;

    Dipartimento di Scienze Geologiche, Universita di Roma Tre, S. Lgo Leonardo Murialdo, 00146 Roma, Italy;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    caldera; ignimbrite; plinian; phonolite; pyroclastic flow;

    机译:破火山口;着火普林尼安石火山碎屑流;

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