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Subsurface mass monitoring at Theistareykir geothermal field, Iceland, using hybrid gravimetry 冰岛Theistareykir地热田地下物质监测,使用混合重力测量
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-04-01 Epub Date: 2026-01-25 DOI: 10.1016/j.jvolgeores.2026.108539
B. Giuliante , U. Riccardi , J. Hinderer , P. Jousset , T. Pivetta , A.K. Mortensen , J.D. Bernard , S. Schröder , C.M. Krawczyk
Understanding underground mass redistribution in geothermal fields is fundamental to assess the harnessing in geothermal reservoir. Here we apply the hybrid gravimetry method at Theistareykir geothermal field (Northern Iceland). We collected absolute and discrete microgravity measurements yearly within the geothermal field at fixed locations jointly with continuously recorded gravity time series with two superconducting gravimeters (SGs). Data acquisition started in 2017 at the onset of the anthropogenic perturbation. We present and interpret the discrete and continuous gravity datasets from 2017 until 2024 in an attempt to characterize fluid redistribution within the subsurface. The hybrid gravimetry dataset reveal a gravity decrease nearby the extraction area with rates of about −20 μGal per year for the 2017–2022 period, that reduces to few μGal per year in the last two years (2023–2024). An increase in gravity is observed towards the injection area (around 5 to 10 μGal per year). Time-lapse gravity maps reveal a localized gravity decrease (with a maximum of −60 μGal), not collocated with the zone of largest extraction and furthermore an additional trendline of gravity increase (+15 μGal) is observed towards the North. The first suggests a possible lower permeability subsurface zone within the geothermal field, the latter, is in accordance with the direction of the fault system that crosses Theistareykir field, suggesting potential underground fluid pathways. From 2023, although extraction and injection rates did not change, we evidence a change in the gravity trends outside the western part of the geothermal field possibly associated with the 2023 magmatic intrusion.
了解地热田地下物质分布是评价地热储层利用的基础。本文将混合重力法应用于冰岛北部的Theistareykir地热田。利用两台超导重力仪(SGs)连续记录重力时间序列,每年在固定地点采集地热场的绝对和离散微重力测量数据。数据采集始于2017年人为扰动开始时。我们展示并解释了从2017年到2024年的离散和连续重力数据集,试图描述地下流体再分布的特征。混合重力数据集显示,在2017-2022年期间,提取区附近的重力下降速度约为- 20 μGal /年,在2023-2024年期间,重力下降速度降至几μGal /年。观察到注射区域的重力增加(每年约5至10 μGal)。时移重力图显示了局部重力下降(最大为- 60 μGal),与最大提取区不重合,并且在北方向观测到额外的重力增加趋势线(+15 μGal)。前者提示地热田中可能存在低渗透率地下带,后者与穿越Theistareykir田的断裂系统方向一致,提示潜在的地下流体通道。从2023年开始,虽然抽注速率没有变化,但地热田西部以外的重力趋势发生了变化,这可能与2023年岩浆侵入有关。
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引用次数: 0
Cracking the crust: Rifting and lateral magma transport at the early Holocene Sveinar-Randarhólar Fissure, NE Iceland 地壳断裂:全新世早期裂陷与横向岩浆搬运Sveinar-Randarhólar冰岛东北部裂缝
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-04-01 Epub Date: 2026-02-04 DOI: 10.1016/j.jvolgeores.2026.108557
Adam Abersteiner , Christoph Beier , Sæmundur A. Halldórsson , Edward W. Marshall , Eemu Ranta , Magnús Á. Sigurgeirsson , Martin Whitehouse , Heejin Jeon
The ∼11 ka Sveinar-Randarhólar Fissure (SRF), located in the neovolcanic Northern Volcanic Rift Zone (NRZ; Central East Iceland), is a ∼ 75 km long, north-south trending fissure comprising of a discontinuous chain of scoria cones and basaltic lava flows distal to any central volcanoes. We report petrography, mineral-glass compositions, whole-rock major and trace elements, Pb-isotopes, and olivine O-isotopes, for 39 scoria and lava samples collected along the fissure, together with analyses of the rhyolitic Askja-Skolli (Askja-S) tephra previously linked to the same eruptive event.
The geochemical uniformity indicates the SRF magma was derived from a compositionally homogeneous reservoir that experienced minimal modification during transport. The geochemical similarity between the SRF and the sub-glacial and early-Holocene eruptive products of the Askja central volcano, combined with their shared rift-axis alignment, supports the magma system beneath Askja as the source. The SRF eruption was likely contemporaneous with the Plinian Askja Skolli event that deposited the Askja-S tephra across distal reaches of the fissure. We suggest that rift initiation released accumulated tectonic stress, driving magma withdrawal from a mid-crustal (∼8–10 km) reservoir beneath Askja. The resulting release of tectonic stress triggered eruption and caldera collapse, which in turn further facilitated lateral magma transport into the SRF. The eruption of the SRF into ice-free and lower-elevation terrain suggests that topographic gradient likely influenced vertical and horizontal magma migration.
The SRF represents one of the longest Holocene fissure eruptions in the NRZ, with lateral magma transport extending ≥135 km. Its timing coincides with rapid deglaciation (∼10–12 ka) in northeast Iceland, when ice unloading and lithospheric rebound enhanced melt production and eruption rates.
~ 11 ka Sveinar-Randarhólar裂缝(SRF),位于新火山北部火山裂谷带(NRZ;冰岛中部东部),是一个~ 75公里长,南北走向的裂缝,由一个不连续的火山锥链和玄武岩熔岩流组成,远超任何中心火山。我们报告了沿着裂缝收集的39个岩屑和熔岩样本的岩石学、矿物玻璃成分、全岩主要元素和微量元素、pb同位素和橄榄石o同位素,以及先前与同一喷发事件相关的流纹岩askya - skolli (askya - s) tephra的分析。地球化学均匀性表明SRF岩浆来自一个成分均匀的储层,在运输过程中经历了最小的改造。SRF与Askja中央火山冰期下及早全新世喷发产物的地球化学相似性,结合它们共同的裂谷轴走向,支持Askja下岩浆系统为岩浆源。SRF喷发可能与普林尼期Askja Skolli事件同时发生,该事件沉积了Askja- s tephra穿过裂缝的远端。我们认为,裂谷的形成释放了累积的构造应力,促使岩浆从Askja下方的中地壳(~ 8-10公里)储层中撤出。构造应力的释放引发了火山喷发和破火山口崩塌,从而进一步促进了岩浆向SRF的横向输送。SRF在无冰低海拔地区的喷发表明,地形梯度可能影响了岩浆的垂直和水平迁移。SRF代表了NRZ全新世最长的裂缝喷发之一,岩浆横向输送延伸≥135 km。它的时间与冰岛东北部的快速消冰(~ 10-12 ka)一致,当时冰卸载和岩石圈反弹增强了熔体的产生和喷发速度。
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引用次数: 0
Spatiotemporal evolution of ground deformation on Nishinoshima Island (Japan) during 2014–2020: Insights from ALOS-2/PALSAR-2 InSAR 2014-2020年日本西野岛地表变形时空演变:来自ALOS-2/PALSAR-2 InSAR的观测
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-04-01 Epub Date: 2026-02-02 DOI: 10.1016/j.jvolgeores.2026.108544
Yuji Himematsu
The appearance of a new island associated with a volcanic eruption offers an opportunity to investigate spatiotemporal characteristics of topographic evolution. This study examined the spatiotemporal evolution of ground deformation associated with the eruptive episodes on Nishinoshima Island (Japan) from 2013 to 2020 using ALOS-2/PALSAR-2 Interferometric Synthetic Aperture Radar (InSAR). Frequent lava flows during the 2013–2020 eruptive episodes formed a new islet on the southeastern part of the original island, extending its overall area. ALOS-2/PALSAR-2 InSAR during 2014–2020 revealed a line-of-sight (LOS) extension along the side of the lava flows during the eruptive episodes and in the lava-emplaced regions after previous episodes. The LOS extension along the side of the lava flows during the eruptions is interpreted as loading deformation due to lava emplacement. The best-fit loading model suggests that the pressurized extents almost coincide with the region of decorrelation, which aligns with the area emplaced with lava. In contrast, the inferred volume of emplaced lava yields ∼20% of that inferred from DEM difference. In contrast, the post-eruptive LOS extension at the lava-emplaced area is interpreted as thermoelastic deformation. The magnitude of the post-eruptive LOS extension has reached approximately 20 cm since the end of the previous eruptions, while the rate of LOS change has decreased exponentially over time. The best-fit thermoelastic deformation model indicates a heat source located at a depth of approximately 20 m, consistent with the thickness of the emplaced lava from the previous eruptive episode.
与火山爆发相关的新岛屿的出现为研究地形演变的时空特征提供了机会。利用ALOS-2/PALSAR-2干涉合成孔径雷达(InSAR)研究了2013 - 2020年日本西野岛火山喷发期间地面变形的时空演变特征。2013-2020年火山喷发期间频繁的熔岩流在原岛的东南部形成了一个新的小岛,扩大了其整体面积。2014-2020年期间,ALOS-2/PALSAR-2 InSAR探测结果显示,火山喷发期间沿熔岩流一侧和前几次喷发后的熔岩就位区存在视距(LOS)延伸。火山喷发时沿熔岩流一侧的LOS延伸可以解释为熔岩侵位引起的加载变形。最拟合的加载模型表明,压力范围与去相关区基本一致,与熔岩侵位区一致。相比之下,推断出的就位熔岩体积相当于从DEM差异推断出的体积的20%。相比之下,岩浆侵位区爆发后的LOS扩展被解释为热弹性变形。自前几次喷发结束以来,爆发后的LOS扩展幅度已达到约20 cm,而LOS变化速度随时间呈指数级下降。最佳拟合的热弹性变形模型表明,热源位于约20 m的深度,与上一次喷发的就位熔岩厚度一致。
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引用次数: 0
Magmatic processes in the Comei large igneous province: Insights from quantitative plagioclase composition and texture analysis Comei大火成岩省岩浆过程:定量斜长石组成和结构分析的启示
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-04-01 Epub Date: 2026-02-05 DOI: 10.1016/j.jvolgeores.2026.108559
Sheng-Sheng Chen, Ji-Cheng Wang
The Comei Large Igneous Province (CLIP) in the Tethyan Himalaya (southern Tibet) represents a major Cretaceous magmatic event, yet its origin remains debated between a mantle plume versus a passive rift model. While previous geochemical and geochronological studies have been inconclusive, quantitative textural analysis of magmatic rocks can provide critical, independent constraints on eruption dynamics and timescales—key discriminants between these hypotheses. This study focuses on the porphyritic igneous rocks of the Lakang and Sangxiu Formations, whose plagioclase phenocrysts faithfully record pre-eruptive magmatic conditions. We applied Crystal Size Distribution (CSD) analysis to plagioclase populations, supplemented by electron probe microanalysis (EPMA) of crystal zoning and alignment factor (AF) measurements. The CSDs display straight-line segments (S-CSD type) in the large-crystal domain, indicating steady-state growth in a sub-volcanic reservoir. Calculated characteristic lengths (CLs), combined with an appropriate plagioclase growth rate (10−11 mm/s) for this system, yield magma residence times of 729–2124 years. Integrating these timescales with revised volume estimates yields high eruption rates of 0.24–3.1 km3/yr. The textural record is composite: S-CSD segments indicate time-averaged steady-state growth in a sub-volcanic reservoir, whereas complex crystal zoning and CSD inflections attest to frequent, short-term recharge events. This apparent contradiction is resolved by a model where long-term mush stability was punctuated by episodic rejuvenation. This combination—brief storage, high eruption flux, and a record of both steady growth and episodic replenishment—is best explained by a thermally buffered crystal mush system that was periodically rejuvenated. Such high-energy, high-flux dynamics are inconsistent with passive rifting but strongly support a mantle plume origin for the CLIP. This study demonstrates how multi-scale textural analysis can resolve fundamental debates in LIP petrogenesis.
位于特提斯喜马拉雅(西藏南部)的Comei大火成岩省(CLIP)代表了白垩纪的一次主要岩浆事件,但其起源仍然存在地幔柱与被动裂谷模型之间的争论。虽然以前的地球化学和地质年代学研究没有定论,但对岩浆岩的定量结构分析可以为火山喷发动力学和时间尺度提供关键的独立约束,这是这些假设之间的关键区别。以拉康组和桑秀组的斑岩火成岩为研究对象,其斜长石斑晶真实地记录了喷发前的岩浆条件。我们应用晶体尺寸分布(CSD)分析斜长石种群,辅以电子探针显微分析(EPMA)的晶体分带和取向因子(AF)测量。csd在大晶域中呈直线段(S-CSD型),表明次火山岩储层在稳定状态下发育。计算出的特征长度(CLs),结合适宜的斜长石生长速率(10 ~ 11 mm/s),得出该体系的岩浆停留时间为729 ~ 2124年。将这些时间尺度与修正的体积估计值相结合,可以得出0.24-3.1 km3/年的高喷发率。结构记录是复合的:S-CSD段表明次火山储层的时间平均稳态增长,而复杂的晶体分带和CSD弯曲则证明了频繁的短期充注事件。这个明显的矛盾被一个模型解决了,在这个模型中,长期的糊状稳定被间歇性的恢复所打断。这种组合——短暂的储存,高喷发通量,稳定增长和偶然补充的记录——最好的解释是一个周期性恢复活力的热缓冲晶体糊状系统。这种高能、高通量的动力学与被动裂谷作用不一致,但强烈支持CLIP的地幔柱起源。该研究表明,多尺度结构分析可以解决岩石成因的基本问题。
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引用次数: 0
Reconstruction of the plinian phase of the 7.3 ka “Akahoya” caldera-forming eruption at the Kikai caldera, Japan 日本Kikai火山口7.3 ka“Akahoya”火山口形成喷发的普林尼期重建
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-04-01 Epub Date: 2026-01-23 DOI: 10.1016/j.jvolgeores.2026.108541
Yusuke Haruta , Fukashi Maeno , Yujiro J. Suzuki
<div><div>Most caldera-forming eruptions begin as plinian events. These plinian phases cause magma chamber decompression and result in subsequent caldera collapse and climactic phases characterized by large-scale pyroclastic density currents (PDCs). It is thus essential to understand the eruption sequence and parameters of the plinian phases to constrain the mechanisms of caldera-forming eruption. Here we reconstruct the detailed sequence of the plinian phase of the 7.3 ka caldera-forming eruption (Akahoya eruption) at the Kikai caldera, Japan, based on a geological survey and plume modeling. The proximal facies of the plinian phase deposits indicate that the source vent was located in the western part of the caldera. The eruptive deposits can be divided into seven subunits (Units A0, A1, A2, A3, A4a, A4b, and B) based on their lithofacies. These subunits were further classified into three groups, separated by minor erosive features. The first group comprised an ash fall layer (Unit A0) distributed only in the proximal area within 20 km of the source vent. The second group comprised a pumice fall layer (Unit A1) distributed within 80 km-distance from the Kikai caldera, and overlying PDC or co-PDC fall deposits (Unit A2) distributed in the proximal area. The third group in the proximal area comprised multiple pumice fall layers (Units A3 and A4a) and PDC deposits (Unit B); whilst in the distal area it comprised up to six pumice fall layers intercalated with ash fall layers (Units A4a and A4b). The uppermost pumice fall layers of the third group (Unit A4b) exhibited a more widespread distribution. Based on fall deposit data and plume modeling, eruptive volumes and mass discharge rates (MDRs) were estimated for the three groups to be <span><math><mn>0.0013</mn><mo>−</mo><mn>0.020</mn></math></span> km<sup>3</sup> (first group), <span><math><mn>0.22</mn><mo>−</mo><mn>1.0</mn></math></span> km<sup>3</sup> and <span><math><mn>3.1</mn><mo>×</mo><msup><mn>10</mn><mn>7</mn></msup><mo>−</mo><mn>1.5</mn><mo>×</mo><msup><mn>10</mn><mn>8</mn></msup></math></span> kg/s (second group), and <span><math><mn>5.0</mn><mo>−</mo><mn>14.0</mn></math></span> km<sup>3</sup> and <span><math><mn>5.2</mn><mo>×</mo><msup><mn>10</mn><mn>8</mn></msup><mo>−</mo><mn>2.2</mn><mo>×</mo><msup><mn>10</mn><mn>9</mn></msup><mspace></mspace></math></span>kg/s (third group). The results revealed that the plinian phase of the Akahoya eruption consisted of three eruptive events: Event 1, a small-scale explosive eruption; Event 2, a plinian eruption (MDR up to <span><math><msup><mn>10</mn><mn>8</mn></msup></math></span> kg/s), transitioned into the eruption of small-scale PDCs; Event 3, a large-scale plinian eruption (MDR up to <span><math><msup><mn>10</mn><mn>9</mn></msup></math></span> kg/s) marked by continuous partial column collapses. This eruption sequence is characterized by a gradual increase in eruptive intensity and scale, similar to plinian phases of many caldera-forming erupti
大多数形成火山口的喷发都是从普林尼期事件开始的。这些平期引起岩浆室减压,并导致随后的破火山口崩塌和以大规模火山碎屑密度流(PDCs)为特征的气候期。因此,了解普林尼期的喷发顺序和喷发参数是制约火山口形成机制的必要条件。本文基于地质调查和羽流模拟,重建了日本Kikai火山口7.3 ka火山口形成喷发(Akahoya喷发)的普林尼期的详细序列。顺层相沉积的近端相表明,烃源喷口位于破火山口的西部。根据其岩相特征,可将其划分为7个亚单元(A0、A1、A2、A3、A4a、A4b、B)。这些亚基进一步划分为3组,以较小的侵蚀特征为界。第一组由一个灰落层(单位A0)组成,仅分布在源喷口20公里内的近端区域。第二组由分布在Kikai破火山口80 km范围内的浮石落层(A1单元)和分布在近端区域的上覆PDC或co-PDC落层(A2单元)组成。第三组在近端由多个浮石落层(单元A3和单元A4a)和PDC矿床(单元B)组成;而在远端区域,它由多达六个浮石坠落层和火山灰坠落层相互穿插(单元A4a和A4b)。第三组(A4b单元)最上层浮石落层分布更为广泛。根据沉积资料和羽流模拟,估计3组的喷发体积和质量排放速率(MDRs)分别为0.0013 ~ 0.020 km3(第一组)、0.22 ~ 1.0 km3和3.1×107−1.5×108 kg/s(第二组)和5.0 ~ 14.0 km3和5.2×108−2.2×109kg/s(第三组)。结果表明,阿卡霍亚火山喷发的普林尼期由3次喷发事件组成:事件1为小规模的爆发性喷发;事件2,普林尼喷发(MDR高达108 kg/s),转变为小规模pdc喷发;事件3,大规模的普林尼火山喷发(MDR高达109 kg/s),标志着连续的部分柱崩塌。该喷发序列的特点是喷发强度和规模逐渐增加,与许多形成火山口的喷发的普林尼期相似。据估计,顺层沉降体的岩浆总量为1.0 ~ 4.0 km3。这一数值明显小于其他具有类似火山口规模的形成火山口喷发的普林尼期岩浆体积。接近阿卡霍亚火山喷发岩浆库破火山口崩塌开始的理论岩浆退出阈值。结果表明,阿卡霍亚火山喷发的火山口塌陷是由相对较小的岩浆室减压引起的,该火山喷发发生在普林尼期和喷发暂停之后。
{"title":"Reconstruction of the plinian phase of the 7.3 ka “Akahoya” caldera-forming eruption at the Kikai caldera, Japan","authors":"Yusuke Haruta ,&nbsp;Fukashi Maeno ,&nbsp;Yujiro J. Suzuki","doi":"10.1016/j.jvolgeores.2026.108541","DOIUrl":"10.1016/j.jvolgeores.2026.108541","url":null,"abstract":"&lt;div&gt;&lt;div&gt;Most caldera-forming eruptions begin as plinian events. These plinian phases cause magma chamber decompression and result in subsequent caldera collapse and climactic phases characterized by large-scale pyroclastic density currents (PDCs). It is thus essential to understand the eruption sequence and parameters of the plinian phases to constrain the mechanisms of caldera-forming eruption. Here we reconstruct the detailed sequence of the plinian phase of the 7.3 ka caldera-forming eruption (Akahoya eruption) at the Kikai caldera, Japan, based on a geological survey and plume modeling. The proximal facies of the plinian phase deposits indicate that the source vent was located in the western part of the caldera. The eruptive deposits can be divided into seven subunits (Units A0, A1, A2, A3, A4a, A4b, and B) based on their lithofacies. These subunits were further classified into three groups, separated by minor erosive features. The first group comprised an ash fall layer (Unit A0) distributed only in the proximal area within 20 km of the source vent. The second group comprised a pumice fall layer (Unit A1) distributed within 80 km-distance from the Kikai caldera, and overlying PDC or co-PDC fall deposits (Unit A2) distributed in the proximal area. The third group in the proximal area comprised multiple pumice fall layers (Units A3 and A4a) and PDC deposits (Unit B); whilst in the distal area it comprised up to six pumice fall layers intercalated with ash fall layers (Units A4a and A4b). The uppermost pumice fall layers of the third group (Unit A4b) exhibited a more widespread distribution. Based on fall deposit data and plume modeling, eruptive volumes and mass discharge rates (MDRs) were estimated for the three groups to be &lt;span&gt;&lt;math&gt;&lt;mn&gt;0.0013&lt;/mn&gt;&lt;mo&gt;−&lt;/mo&gt;&lt;mn&gt;0.020&lt;/mn&gt;&lt;/math&gt;&lt;/span&gt; km&lt;sup&gt;3&lt;/sup&gt; (first group), &lt;span&gt;&lt;math&gt;&lt;mn&gt;0.22&lt;/mn&gt;&lt;mo&gt;−&lt;/mo&gt;&lt;mn&gt;1.0&lt;/mn&gt;&lt;/math&gt;&lt;/span&gt; km&lt;sup&gt;3&lt;/sup&gt; and &lt;span&gt;&lt;math&gt;&lt;mn&gt;3.1&lt;/mn&gt;&lt;mo&gt;×&lt;/mo&gt;&lt;msup&gt;&lt;mn&gt;10&lt;/mn&gt;&lt;mn&gt;7&lt;/mn&gt;&lt;/msup&gt;&lt;mo&gt;−&lt;/mo&gt;&lt;mn&gt;1.5&lt;/mn&gt;&lt;mo&gt;×&lt;/mo&gt;&lt;msup&gt;&lt;mn&gt;10&lt;/mn&gt;&lt;mn&gt;8&lt;/mn&gt;&lt;/msup&gt;&lt;/math&gt;&lt;/span&gt; kg/s (second group), and &lt;span&gt;&lt;math&gt;&lt;mn&gt;5.0&lt;/mn&gt;&lt;mo&gt;−&lt;/mo&gt;&lt;mn&gt;14.0&lt;/mn&gt;&lt;/math&gt;&lt;/span&gt; km&lt;sup&gt;3&lt;/sup&gt; and &lt;span&gt;&lt;math&gt;&lt;mn&gt;5.2&lt;/mn&gt;&lt;mo&gt;×&lt;/mo&gt;&lt;msup&gt;&lt;mn&gt;10&lt;/mn&gt;&lt;mn&gt;8&lt;/mn&gt;&lt;/msup&gt;&lt;mo&gt;−&lt;/mo&gt;&lt;mn&gt;2.2&lt;/mn&gt;&lt;mo&gt;×&lt;/mo&gt;&lt;msup&gt;&lt;mn&gt;10&lt;/mn&gt;&lt;mn&gt;9&lt;/mn&gt;&lt;/msup&gt;&lt;mspace&gt;&lt;/mspace&gt;&lt;/math&gt;&lt;/span&gt;kg/s (third group). The results revealed that the plinian phase of the Akahoya eruption consisted of three eruptive events: Event 1, a small-scale explosive eruption; Event 2, a plinian eruption (MDR up to &lt;span&gt;&lt;math&gt;&lt;msup&gt;&lt;mn&gt;10&lt;/mn&gt;&lt;mn&gt;8&lt;/mn&gt;&lt;/msup&gt;&lt;/math&gt;&lt;/span&gt; kg/s), transitioned into the eruption of small-scale PDCs; Event 3, a large-scale plinian eruption (MDR up to &lt;span&gt;&lt;math&gt;&lt;msup&gt;&lt;mn&gt;10&lt;/mn&gt;&lt;mn&gt;9&lt;/mn&gt;&lt;/msup&gt;&lt;/math&gt;&lt;/span&gt; kg/s) marked by continuous partial column collapses. This eruption sequence is characterized by a gradual increase in eruptive intensity and scale, similar to plinian phases of many caldera-forming erupti","PeriodicalId":54753,"journal":{"name":"Journal of Volcanology and Geothermal Research","volume":"472 ","pages":"Article 108541"},"PeriodicalIF":2.3,"publicationDate":"2026-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146190951","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Modelled versus tracked ballistic trajectories of volcanic bombs at Stromboli (Italy) 意大利斯特隆博利火山炸弹弹道轨迹的模拟与追踪
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-04-01 Epub Date: 2026-01-27 DOI: 10.1016/j.jvolgeores.2026.108543
A. Sork , L. Watson , B. Kennedy , R.H. Fitzgerald , J. Taddeucci , M. Sellier , P. Scarlato , E. Del Bello , T. Ricci
Validation for computational modelling of volcanic ballistic projectiles (VBPs) has often been accomplished by replication of field-surveyed VBP distributions. However, a range of ejection parameters can result in the same impact location, with differing impact energies and therefore hazard implications. Ballistic hazard models must accurately represent the whole trajectory to better estimate ballistic energy and interpret eruption dynamics.
We examine model performance by directly measuring Strombolian VBP ejection parameters and trajectories from high-speed video and comparing with modelled trajectories using the same parameters. We illustrate the effects of velocity and size on drag. We synthesize and investigate different methods by which the Reynolds number (Re) - drag coefficient (CD) relationship is incorporated into models and how this affects modelling results. Our computational model allows for application of different existing Re-CD methods and direct comparison to tracked trajectories on the metrics of impact distance and peak height.
Even with validated ejection parameters and appropriate Re-CD relationships, the model rarely accurately reproduces both height and distance within a 5% threshold. The most common scenario is model overestimation of both metrics. The gas jet is the largest factor contributing to this discrepancy. Significant slowing of VBPs in excess of gravity is observed while bombs are rising (and within the gas jet radius) but not while falling. Slowing in the gas jet is potentially caused by friction with ash and lapilli, surface temperature effects, or other fluid dynamics effects.
火山弹道弹丸(VBPs)计算模型的验证通常是通过复制现场测量的VBP分布来完成的。然而,一系列的弹射参数可能导致相同的撞击位置,具有不同的撞击能量,从而产生危险。为了更好地估计弹道能量和解释喷发动力学,弹道危险模型必须准确地表示整个轨迹。我们通过直接测量高速视频中的Strombolian VBP弹射参数和轨迹,并与使用相同参数的建模轨迹进行比较,来检验模型的性能。我们说明了速度和尺寸对阻力的影响。我们综合和研究了将雷诺数(Re) -阻力系数(CD)关系纳入模型的不同方法,以及这对建模结果的影响。我们的计算模型允许应用不同的现有Re-CD方法,并根据撞击距离和峰值高度的指标直接比较跟踪轨迹。即使有有效的弹射参数和适当的Re-CD关系,该模型也很难在5%的阈值内准确地再现高度和距离。最常见的情况是模型对两个度量的高估。燃气喷射是造成这种差异的最大因素。在超过重力的情况下,当炸弹上升时(以及在气体喷射半径内),可观察到VBPs的显著减速,而在下降时则没有。气体喷射的减速可能是由于与灰和石蜡的摩擦、表面温度效应或其他流体动力学效应造成的。
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引用次数: 0
Granophyric crystallization within the Gomez Tuff, the world's largest pantelleritic ignimbrite, Davis Mountains, Trans-Pecos Texas 戈麦斯凝灰岩中的花岗植物结晶,世界上最大的泛辉质火成岩,戴维斯山脉,跨佩科斯德克萨斯州
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-01 Epub Date: 2026-01-12 DOI: 10.1016/j.jvolgeores.2025.108527
Don F. Parker , John C. White , Kevin Urbanczyk
The Gomez Tuff was erupted ∼37 Ma as an explosive component of widespread silicic lava (“flood rhyolite”). The Gomez eruption covered an area > 4000 km2, with an estimated dense rock equivalent volume of ∼220 km3, making it the largest known pantelleritic ignimbrite. The eruption formed a ∼18 × 24 km-diameter caldera, within which the ignimbrite ponded to thicknesses approaching 500 m. Estimated water content (∼1.9 wt%) of the erupting magma was relatively low, favoring eruption of dense pyroclastic flows over pyroclastic falls. Within thicker sections of the tuff, rheomorphic flow created flow banding, large folds and ramp structures. Granophyric crystallization (af, cpx, aenig, amph, qz) destroyed the fragmental nature of the tuff, except for abundant lithic inclusions.
Gomez phenocryst assemblages include alkali feldspar (Or3639) and quartz ± fayalite, with minor hedenbergite, ilmenite and apatite. Magmatic conditions previously deduced from these assemblages assuming P = 2 kbar, a magmatic temperature of ∼750 °C from phase equilibria and not using fayalite in the calculations indicated a temperature range of ∼870 to 750 °C, with oxygen fugacity (ΔFMQ ∼ −1.92) below the NNO buffer (Parker and White, 2008). Alternative calculations suggest ranges of 855 to 766 °C, assuming fayalite stable in all samples, and 900 to 700 °C, assuming aenigmatite was stable in lieu of fayalite. The calculations assuming neither fayalite nor aenigmatite was stable as a phenocryst are preferred, as fayalite was only observed in two samples and aenigmatite was not observed as a phenocryst in any sample.
The original Peralkalinity Index (P·I.) was likely ∼1.3. During granophyric crystallization (at ∼687 °C) in thick sections of the tuff, groundmass feldspar increased its iron content and became more potassic, driving glass and calculated groundmass compositions to ∼1.48. In the final stages of crystallization, groundmass pyroxene approached stoichiometric aegirine and arfvedsonite became less magnesian and more sodic, suggesting that the P·I. of the final crystallizing glass neared 1.8, judging from comparison to the Type 1 Green Tuff of Pantelleria.
We model the Gomez magma chamber as an extensive sill, in which pantelleritic magma accumulated above a reservoir of trachytic magma. Eruption of the ignimbrite efficiently drained the evolved magma, allowing the eruption of trachyte lava, which subsequently filled the caldera.
戈麦斯凝灰岩是作为广泛分布的硅熔岩(“洪水流纹岩”)的爆炸性成分喷发的~ 37 Ma。戈麦斯火山喷发覆盖了4000平方公里的面积,估计其致密岩石当量体积约为220平方公里,使其成为已知最大的泛辉质火成岩。火山喷发形成了一个直径约18 × 24公里的火山口,火山口内的火成岩沉积厚度接近500米。喷发岩浆的估计含水量(~ 1.9 wt%)相对较低,有利于密集火山碎屑流而不是火山碎屑瀑布的喷发。在较厚的凝灰岩剖面内,流变流动形成了流带、大褶皱和斜坡构造。花岗岩结晶(af, cpx, aenig, amph, qz)破坏了凝灰岩的破碎性质,但含有丰富的岩屑包裹体。戈麦斯斑晶组合包括碱长石(Or36-39)和石英±费长石,少量含钙长石、钛铁矿和磷灰石。先前从这些组合中推断出的岩浆条件假设P = 2 kbar,从相平衡中得出的岩浆温度为~ 750°C,在计算中没有使用费亚利石,表明温度范围为~ 870至750°C,氧逸度(ΔFMQ ~ 1.92)低于NNO缓冲层(Parker和White, 2008)。另一种计算方法认为温度范围在855到766°C之间,假设所有样品中都有稳定的铁晶石,而900到700°C之间,假设铁晶石是稳定的而不是铁晶石。假设费耶利石和奥谜石都不是稳定的斑晶的计算是优选的,因为费耶利石只在两个样品中观察到,而奥谜石没有在任何样品中观察到作为斑晶。原始过碱度指数(P·i)可能为~ 1.3。在凝灰岩厚剖面的花岗岩结晶过程中(在~ 687°C),地长石的铁含量增加,钾含量增加,驱动玻璃和计算的地长石成分达到~ 1.48。在结晶的最后阶段,地质体辉石趋向于化学计量氮化,而到达的辉石镁质变少,钠质变多,表明P·I。与panteleria的1型绿凝灰岩相比,最终结晶玻璃的温度接近1.8。我们将戈麦斯岩浆房建模为一个广泛的岩床,其中泛长质岩浆积聚在粗质岩浆储层之上。火成岩的喷发有效地排干了演化的岩浆,使得粗枝状熔岩得以喷发,这些熔岩随后充满了火山口。
{"title":"Granophyric crystallization within the Gomez Tuff, the world's largest pantelleritic ignimbrite, Davis Mountains, Trans-Pecos Texas","authors":"Don F. Parker ,&nbsp;John C. White ,&nbsp;Kevin Urbanczyk","doi":"10.1016/j.jvolgeores.2025.108527","DOIUrl":"10.1016/j.jvolgeores.2025.108527","url":null,"abstract":"<div><div>The Gomez Tuff was erupted ∼37 Ma as an explosive component of widespread silicic lava (“flood rhyolite”). The Gomez eruption covered an area &gt; 4000 km<sup>2</sup>, with an estimated dense rock equivalent volume of ∼220 km<sup>3</sup>, making it the largest known pantelleritic ignimbrite. The eruption formed a ∼18 × 24 km-diameter caldera, within which the ignimbrite ponded to thicknesses approaching 500 m. Estimated water content (∼1.9 wt%) of the erupting magma was relatively low, favoring eruption of dense pyroclastic flows over pyroclastic falls. Within thicker sections of the tuff, rheomorphic flow created flow banding, large folds and ramp structures. Granophyric crystallization (af, cpx, aenig, amph, qz) destroyed the fragmental nature of the tuff, except for abundant lithic inclusions.</div><div>Gomez phenocryst assemblages include alkali feldspar (Or<sub>36</sub><sub>–</sub><sub>39</sub>) and quartz ± fayalite, with minor hedenbergite, ilmenite and apatite. Magmatic conditions previously deduced from these assemblages assuming <em>P</em> = 2 kbar, a magmatic temperature of ∼750 °C from phase equilibria and not using fayalite in the calculations indicated a temperature range of ∼870 to 750 °C, with oxygen fugacity (ΔFMQ ∼ −1.92) below the NNO buffer (<span><span>Parker and White, 2008</span></span>). Alternative calculations suggest ranges of 855 to 766 °C, assuming fayalite stable in all samples, and 900 to 700 °C, assuming aenigmatite was stable in lieu of fayalite. The calculations assuming neither fayalite nor aenigmatite was stable as a phenocryst are preferred, as fayalite was only observed in two samples and aenigmatite was not observed as a phenocryst in any sample.</div><div>The original Peralkalinity Index (P·I.) was likely ∼1.3. During granophyric crystallization (at ∼687 °C) in thick sections of the tuff, groundmass feldspar increased its iron content and became more potassic, driving glass and calculated groundmass compositions to ∼1.48. In the final stages of crystallization, groundmass pyroxene approached stoichiometric aegirine and arfvedsonite became less magnesian and more sodic, suggesting that the P·I. of the final crystallizing glass neared 1.8, judging from comparison to the Type 1 Green Tuff of Pantelleria.</div><div>We model the Gomez magma chamber as an extensive sill, in which pantelleritic magma accumulated above a reservoir of trachytic magma. Eruption of the ignimbrite efficiently drained the evolved magma, allowing the eruption of trachyte lava, which subsequently filled the caldera.</div></div>","PeriodicalId":54753,"journal":{"name":"Journal of Volcanology and Geothermal Research","volume":"471 ","pages":"Article 108527"},"PeriodicalIF":2.3,"publicationDate":"2026-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145979052","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Hyperspectral imaging, mineralogy, and degassing: Exploring the volcanic hydrothermal system of Red Crater, Tongariro, Aotearoa New Zealand 高光谱成像、矿物学和脱气:探索红火山口的火山热液系统,汤加里罗,奥特阿瓦新西兰
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-01 Epub Date: 2026-01-15 DOI: 10.1016/j.jvolgeores.2026.108535
Daniel Sturgess , Gabor Kereszturi , Agnes Mazot , Rachelle Sanchez , Antonio M. Álvarez-Valero , Vladyslav Zakharovskyi
Hydrothermal alteration on volcanoes can compromise the strength and permeability of the host rock, contributing to flank collapses (e.g., Te Maari, 2012) and phreatic eruptions (e.g., Whakaari, 2019). Alteration processes occur at volcanoes hosting hydrothermal systems, where hot, acidic fluid flow is driven by a supply of magmatic heat and gas inputs, resulting in the dissolution of primary minerals and the deposition of secondary assemblages. We investigated hydrothermal alteration at Red Crater, Tongariro, Aotearoa New Zealand, using a combination of laboratory and airborne hyperspectral imaging, mineralogical, and geochemical techniques. Two distinct alteration styles were identified: (1) advanced argillic alteration, characterised by amorphous silica, kaolinite, and alunite, primarily focused at the Red Crater scoria cone, and (2) silicification at Oturere and the Emerald Lakes. The distribution of these units was mapped using supervised image classification of airborne hyperspectral data. Textural and isotopic analyses suggest acid-sulphate alteration is primarily driven by the oxidation of rising H2S in a steam-heated environment. Red Crater hosts four main regions of heightened degassing, coinciding with geothermal surface features and hydrothermal alteration deposits, with 26.2 ±1.5 t/d of CO2 emissions and an H2S flux of 131.1 g/m2/d. This study presents a conceptual model of hydrothermal alteration processes at Red Crater. Our mapping of alteration and degassing can indicate areas of potential future hazards, and may support simulations assessing flank instability, improving hazard assessment at this active vent.
火山上的热液蚀变会损害宿主岩石的强度和渗透性,导致侧翼崩塌(例如,Te Maari, 2012)和潜水喷发(例如,Whakaari, 2019)。蚀变过程发生在拥有热液系统的火山上,岩浆热量和气体的输入驱动了热酸性流体的流动,导致原生矿物的溶解和次生组合的沉积。我们利用实验室和航空高光谱成像、矿物学和地球化学技术相结合的方法,研究了新西兰汤加里罗红色陨石坑的热液蚀变。发现了两种不同的蚀变类型:(1)晚期泥质蚀变,以无定形二氧化硅、高岭石和明矾石为特征,主要集中在Red Crater的岩屑锥;(2)Oturere和Emerald Lakes的硅化作用。利用机载高光谱数据的监督图像分类绘制了这些单元的分布。结构和同位素分析表明,酸性硫酸盐的变化主要是由蒸汽加热环境中上升的H2S氧化引起的。赤坑主要有4个脱气强化区,与地热地表特征和热液蚀变矿床相吻合,CO2排放量为26.2±1.5 t/d, H2S通量为131.1 g/m2/d。本文提出了红火山口热液蚀变过程的概念模型。我们绘制的蚀变和脱气图可以指出未来潜在的危险区域,并可能支持评估侧翼不稳定性的模拟,从而改进该活跃喷口的危险评估。
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引用次数: 0
Unravelling the volcanic history of the Campanian Plain: A detailed study of mid-distance successions between 40 and 130 ka 揭示坎帕尼亚平原的火山史:40 - 130 ka中程序列的详细研究
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-01 Epub Date: 2026-01-05 DOI: 10.1016/j.jvolgeores.2026.108531
F. Totaro , P. Petrosino , I. Arienzo , M.A. Di Vito , M. Petrelli , B.R. Jicha , M. D'Antonio
The effectiveness of tephrochronology in reconstructing past events at high resolution relies heavily on accurate knowledge of the eruptive history of volcanic sources. For the Campanian Plain, southern Italy, distal and ultra-distal tephra archives provide detailed geochemical and chronological records of its complex volcanism. In contrast, proximal studies often depend on whole-rock geochemistry from outcrops that are frequently incomplete due to erosion or burial, limiting direct comparisons with glass-based datasets from distal sites. However, mid-distance buried successions offer a crucial archive, preserving volcanic layers often absent in proximal settings. This study investigates two mid-distance successions retrieved from boreholes—Camaldoli della Torre (CdT) and San Marco Evangelista (SME)—and selected samples from the distal San Gregorio Magno (SGM) core covering the 130–40 ka interval. All three boreholes are located in the Campania region (Italy). Through a multi-method analytical approach, including major and trace elements, Sr-Nd isotopes, and new 40Ar/39Ar dating, we characterize key tephra layers and identify previously unrecognized correlations to widespread Mediterranean tephra markers. Additionally, we evaluate the potential of using whole-rock geochemical data for correlation with glass compositions from distal sites, in order to assess whether such comparisons can be reliably employed in tephrostratigraphic studies. Our findings highlight the pivotal role of buried successions in reconstructing a more complete volcanic record revealing the additional occurrences of key Mediterranean tephra markers.
地表年代学在高分辨率重建过去事件方面的有效性在很大程度上依赖于对火山源喷发历史的准确认识。对于意大利南部的坎帕尼亚平原,远端和超远端tephra档案提供了其复杂火山活动的详细地球化学和年代学记录。相比之下,近端研究往往依赖于露头的全岩石地球化学,由于侵蚀或埋藏,露头往往不完整,限制了与远端地点基于玻璃的数据集的直接比较。然而,中距离的埋藏序列提供了一个重要的档案,保存了在近端环境中经常缺失的火山层。本研究调查了camaldoli della Torre (CdT)和San Marco Evangelista (SME)两个井中序列,并选择了覆盖130-40 ka区间的San Gregorio Magno (SGM)远端岩心样本。这三个井眼都位于意大利坎帕尼亚地区。通过多方法分析方法,包括主要元素和微量元素,Sr-Nd同位素,以及新的40Ar/39Ar测年,我们表征了关键的tephra层,并确定了以前未被认识到的与广泛分布的地中海tephra标记的相关性。此外,我们评估了使用全岩地球化学数据与远端地点的玻璃成分进行对比的潜力,以评估这种比较是否可以可靠地用于地层研究。我们的发现强调了埋藏序列在重建更完整的火山记录方面的关键作用,揭示了地中海关键火山标志的额外出现。
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引用次数: 0
Reconstruction of the eruptive processes and new 40Ar/39Ar dating of Plio-Pleistocene monogenetic volcanism in the Folded Middle Atlas (Northern Morocco). Implications of eruption style variation with climate changes 褶皱中阿特拉斯(摩洛哥北部)上新世-更新世单成因火山喷发过程重建及40Ar/39Ar新定年气候变化对火山喷发样式变化的影响
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-01 Epub Date: 2026-01-07 DOI: 10.1016/j.jvolgeores.2026.108530
Said Haidatte , Károly Németh , Abdelilah Fekkak , Hind El Hachimi , El Houcine El Haous , Omar Outaaoui , Michele Lustrino
During the Plio-Pleistocene, several individual monogenetic volcanoes were emplaced in the Folded Middle Atlas region in Central Morocco. These eruptions are primarily concentrated on anticlinal ridges and are structured by a network of NNE-SSW-oriented faults, inherited from Alpine or older tectonic phases. This study investigates three Pleistocene (2.5-0.8 Ma) small scoria cones and one partially preserved maar, here dated with 40Ar/39Ar geochronology to 0.281 Ma, indicating the youngest hydrovolcanic eruption of this area.
The temporal distribution and morphological diversity of volcanic edifices in northern Africa during the Plio-Pleistocene are inferred to be closely associated with paleoclimatic fluctuations, which alternated between arid and humid phases. Strombolian explosive eruptions created scoria cones primarily during arid periods, facilitating magmatic outgassing with minimal interaction between magma and the water table. In contrast, hydrovolcanic eruptions were promoted by wetter climatic conditions, which were susceptible to interaction between upwelling magma and surface water or shallow aquifers.
Scoria cones consist of pyroclastic deposits of varying grain sizes, including scoriaceous pyroclasts such as small portions of coarse ash lapilli and volcanic bombs with different morphologies. Their last eruptive activity phases are typically represented by thin lava flows, indicating a gradual shift to Hawaiian-type mild explosive dynamics. Conversely, maar formations are characterized by ejecta deposits from phreatomagmatic explosions, indicating rapid interaction between magma and varying volumes of external water, likely occurring during a single eruptive event.
在上新世-更新世期间,摩洛哥中部褶皱的中阿特拉斯地区有几座独立的单生火山。这些喷发主要集中在背斜脊上,由北北东-西南向断裂网络构造,继承自阿尔卑斯或更古老的构造阶段。本研究考察了3个更新世(2.5 ~ 0.8 Ma)小火山锥和1个部分保存的火山泥,其40Ar/39Ar年代学测定值为0.281 Ma,为该区最年轻的水火山喷发。推断北非地区上新世—更新世火山结构的时间分布和形态多样性与古气候的干湿交替波动密切相关。斯特龙堡火山爆发主要在干旱时期产生了火山渣锥,促进了岩浆和地下水位之间最小的相互作用。相比之下,湿润的气候条件促进了水火山爆发,这些气候条件容易受到上涌岩浆与地表水或浅层含水层相互作用的影响。火山渣锥由不同粒度的火山碎屑沉积物组成,包括火山渣质火山碎屑,如一小部分粗灰石和不同形态的火山弹。它们最后的喷发活动阶段通常以稀薄的熔岩流为代表,表明逐渐转向夏威夷式的温和爆炸动力学。相反,maar地层的特征是由火山喷发的喷出物沉积物,表明岩浆和不同体积的外部水之间的快速相互作用,可能发生在一次喷发事件中。
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引用次数: 0
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Journal of Volcanology and Geothermal Research
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