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Investigating the connection between superhydrous melts, magma reservoir nucleation and the scarcity of mafic eruptions in post-collisional settings 研究碰撞后超水熔体、岩浆储层成核与基性火山喷发稀少之间的联系
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-01-27 DOI: 10.1016/j.jvolgeores.2026.108542
Alissa Näpflin , Răzvan-Gabriel Popa , Ioan Seghedi , Olivier Bachmann
Magma reservoir emplacement in the brittle upper-crust typically requires prolonged heating to modify host-rock rheology, allowing magma to accumulate rather than erupt. In thermally immature crust, early eruptions are expected to be mafic, yet many volcanic provinces, particularly those with water-rich melts, lack significant initial mafic volcanism, suggesting an alternative trapping mechanism. We investigate this using Caraci volcano (Romania's Apuseni Mountains), a water-rich system that started with relatively differentiated, andesitic eruptions. The first eruptions at Caraci extruded water-rich (5–6 ± 0.35 wt% dissolved H2O) amphibole-plagioclase andesites (890–920 ± 22 °C) stored at water-saturated conditions in the upper-crust (∼2 ± 0.5 kbar). These magmas were associated with superhydrous primitive melts (>6 wt% H₂O), which evolved in a polybaric system (crystallization pressure varying from 2 to 8 ± 0.5 kbar), evidenced by high-Mg amphibole and delayed plagioclase crystallization. These deeper storage melts likely reached water saturation during ascent towards the upper crust, inducing degassing and crystallization, which increased viscosity and enabled stalling in the cold crust, explaining the lack of initial mafic eruptions and providing the efficient trapping mechanism in a thermally immature crust. Progressive drying of the source and generation of less hydrous magmas initiated the eruptions and construction of the stratovolcano, and ultimately terminated the system. As a result, the final eruption extruded somewhat drier (4–4.5 ± 0.35 wt% H2O), hotter (930–960 ± 45 °C) pyroxene-bearing andesites erupted from water-undersaturated storage. This trapping mechanism of water-rich magmas may explain the typical scarcity of mafic volcanism in arc and post-collisional settings.
岩浆储层位于脆弱的上地壳中,通常需要长时间加热来改变宿主岩石的流变性,从而使岩浆积聚而不是喷发。在热不成熟的地壳中,早期喷发预计是基性的,然而许多火山省,特别是那些富含水的熔体,缺乏明显的初始基性火山作用,这表明了另一种圈闭机制。我们使用Caraci火山(罗马尼亚的Apuseni山脉)来研究这一点,这是一个富含水的系统,起源于相对分化的安山岩喷发。Caraci的第一次喷发喷出了富含水(5-6±0.35 wt%溶解水)的角闪斜长安山岩(890-920±22°C),储存在上地壳(~ 2±0.5 kbar)的水饱和条件下。这些岩浆与超水原始熔体(>6 wt% H₂O)有关,在多压系统中演化(结晶压力在2 ~ 8±0.5 kbar之间),以高mg角闪孔和延迟斜长石结晶为证据。这些较深的储存熔体可能在向上地壳上升的过程中达到水饱和,导致脱气和结晶,从而增加了粘度,使冷地壳停滞,解释了最初基性喷发的缺乏,并为热不成熟地壳提供了有效的捕获机制。源区的逐渐干燥和含水岩浆的减少引发了层状火山的喷发和建造,并最终终止了该体系。结果,最后的喷发挤出了相对干燥(4-4.5±0.35 wt% H2O),较热(930-960±45°C)的含辉石安山岩,这些安山岩是从水不饱和的储存中喷发出来的。这种富水岩浆的圈闭机制可以解释弧和碰撞后环境中典型的基性火山活动的缺乏。
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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 : 2026-01-27 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
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 : 2026-01-25 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
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 : 2026-01-23 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":"2026-01-23","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
Hydrous upper mantle facilitated alkali basalt genesis in the Southeastern Carpathians, Romania 罗马尼亚喀尔巴阡山脉东南部含水上地幔有利于碱性玄武岩的形成
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-01-22 DOI: 10.1016/j.jvolgeores.2026.108540
Levente Patkó , Ákos Kővágó , Thomas Pieter Lange , Alexandru Szakács , Monika Huraiová , Márta Berkesi , László Előd Aradi , Szilveszter Gergely , Ábel Szabó , Károly Németh , Csaba Szabó , István János Kovács
This study investigates the structural hydroxyl content in clinopyroxenes from five cumulate xenoliths hosted by alkali basaltic pyroclastic rocks collected from the Perşani Mountains Volcanic Field (southeastern Transylvania, Romania), revealing structural hydroxyl concentrations ranging from 261 to 436 ppm wt. From these measurements, the ‘water’ content of the equilibrium parental alkali basaltic melt was estimated at 1.2 to 2.5 wt%, consistent with global values for alkali basalts. The mantle source ‘water’ content was also determined and resulted to be a ‘water’-rich mantle volume, ranging from 400 to 840 ppm wt. under batch melting and 310 to 660 ppm wt. for fractional melting models. The hydrous signature appears to be linked to the influence of an earlier subduction event, sustained by continued fluid release from remnants of the sinking slab at asthenospheric depths. The findings highlight the crucial influence of ‘water’ in upwelling mantle material, especially in regions affected by slab rollback and detachment, as is the case in the study area of the East Carpathian bend zone, where ‘water’ governs the extent of partial melting and enhances melt generation.
本研究调查了从perani山脉火山场(罗马尼亚特兰西瓦尼亚东南部)收集的由碱玄武质火山碎屑岩携带的5个累积包体中斜辉石中结构羟基的含量,揭示了结构羟基的浓度范围为261至436 ppm wt。从这些测量结果中,平衡母碱玄武质熔体的“水”含量估计为1.2至2.5 wt%,与碱玄武岩的全球值一致。还确定了地幔源“水”含量,并得出了一个“水”丰富的地幔体积,在批量熔融模式下为400至840ppm,在部分熔融模式下为310至660 ppm。含水特征似乎与早期俯冲事件的影响有关,由软流层深处下沉的板块残余物持续释放的流体维持。研究结果强调了“水”对上涌地幔物质的重要影响,特别是在受板块回滚和分离影响的地区,就像在东喀尔巴阡弯曲带的研究区域一样,“水”控制着部分熔融的程度,并增强了熔体的产生。
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引用次数: 0
The nucleation and growth of mixed H2O–CO2 bubbles in magmas 岩浆中混合H2O-CO2气泡的成核与生长
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-01-19 DOI: 10.1016/j.jvolgeores.2026.108538
Patrick Sullivan , Edward W. Llewellin , Fabian B. Wadsworth , Simone Colucci , Halim Kusumaatmaja
Volcanic eruptions are driven by the nucleation and growth of gas bubbles that form when volatile species dissolved in magma become supersaturated. Previous models for bubble growth have focussed on H2O; however, CO2 also plays a fundamental role in the nucleation and growth of gas bubbles. Here, we develop a numerical model to explore the nucleation and growth of bubbles containing both H2O and CO2 in magma of arbitrary composition. Nucleation is modelled as a Poisson process using classical nucleation theory with composition-appropriate solubility models for the mixed H2O–CO2 fluid. We find that CO2 dramatically increases the depth of bubble nucleation compared with H2O-only systems; for a case-study rhyolite (Krafla, Iceland) CO2 increases nucleation depth from 130 m (H2O-only) to 760 m if CO2 is included (a factor of 6 increase in nucleation pressure); for a case-study basalt (Fagradalsfjall, Iceland), nucleation occurs at 13 km depth if CO2 is included, but does not occur at all if H2O is the only volatile species. Post-nucleation growth of the bubbles is investigated by extending a ‘shell model’ to include CO2 as well as H2O. The species are coupled via a mixed equation-of-state for the gas phase, introducing a co-dependence on their solubility that allows H2O to exsolve at greater depth when CO2 is present. As a result, exsolution of a small volume of CO2 can trigger the exsolution of a much larger volume of H2O, driving rapid, disequilibrium bubble growth. Our findings show that accounting for mixed H2O–CO2 volatile compositions is essential for accurate modelling of magma ascent and eruption dynamics.
火山爆发是由气泡的成核和增长驱动的,当岩浆中的挥发性物质变得过饱和时,气泡就会形成。以前的气泡增长模型主要关注H2O;然而,二氧化碳在气泡的成核和生长中也起着重要作用。在这里,我们建立了一个数值模型来探索在任意成分的岩浆中含有H2O和CO2的气泡的成核和生长。成核是一个泊松过程建模使用经典成核理论与组成适当的溶解度模型的混合H2O-CO2流体。我们发现,与纯h2o体系相比,CO2显著增加了气泡成核的深度;以冰岛Krafla流纹岩为例,CO2使成核深度从130 m(仅含h2o)增加到760 m(含CO2时,成核压力增加了6倍);以玄武岩(冰岛Fagradalsfjall)为例,如果含二氧化碳,则在13公里深度发生成核,但如果只有H2O是挥发性物质,则根本不发生成核。通过扩展“壳模型”来包括CO2和H2O,研究了气泡的成核后生长。这两种物质通过气相的混合状态方程耦合,引入了它们的溶解度的共同依赖,当CO2存在时,H2O可以在更大的深度溶解。因此,少量CO2的析出会引发大量H2O的析出,从而导致气泡快速、不平衡地生长。我们的研究结果表明,考虑混合的H2O-CO2挥发成分对于精确模拟岩浆上升和喷发动力学至关重要。
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引用次数: 0
Investigating the seismic structure of shallow magmatic conduits: Insights from the Salina Island (southern Italy) 研究浅层岩浆导管的地震结构:来自萨利纳岛(意大利南部)的见解
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-01-19 DOI: 10.1016/j.jvolgeores.2026.108536
I. Granados-Chavarría , F. Di Luccio , M. Calò , D. Famiani , M. Lupi , M. Palano , G. Ventura
The plumbing systems of closely spaced individual volcanoes and volcanic fields may be very complex due to the interaction (or not) of different magma storage zones and magma pathways at variable depths. Ambient noise tomography unveils the shallow seismic structure of Salina Island (Southern Italy), which is characterized by 6 proximal and partly overlapping volcanoes developed between 244 and 15.6 ka. We use two months of continuous data from 40 nodal stations deployed in 2023 at uneven interstation distances. This seismic array yields tomographic maps down to 1.5 km depth in which the geometry of the volcano flank collapses and shallower plumbing systems of eruptive fissures are clearly imaged. Shear wave velocity maps reveal the main structures and deposits of the ‘twin’ stratovolcanoes of Monte dei Porri, to the west, and Monte Fossa delle Felci, to the east. High velocity anomalies beneath these volcanoes become less pronounced at ∼200 m b.s.l. revealing the transition from submarine to subaerial lava flows. 3D images of the eastward dipping subcircular conduits below the main volcanoes suggest that the deep feeding system is located offshore to the east.
由于不同的岩浆储存带和岩浆通道在不同深度的相互作用(或不相互作用),间隔紧密的单个火山和火山场的管道系统可能非常复杂。环境噪声层析成像揭示了Salina岛(意大利南部)的浅层地震结构,其特征是在244 - 15.6 ka之间发育了6个近部和部分重叠的火山。我们使用了2023年部署的40个节点站在不均匀站间距离上的两个月连续数据。这个地震阵列产生了1.5公里深度的层析成像图,其中火山侧面塌陷的几何形状和较浅的喷发裂缝管道系统被清晰地成像。横波速度图揭示了位于西面的Monte dei Porri和东面的Monte Fossa delle Felci的“孪生”层状火山的主要结构和沉积物。这些火山下面的高速异常在~ 200m b.s.l.变得不那么明显,揭示了从海底到陆上熔岩流的转变。主要火山下方向东倾斜的次圆形管道的三维图像表明,深层补给系统位于东部近海。
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引用次数: 0
An analog experiment showing varying shapes of pyroclasts by including crystals and bubbles 模拟实验显示了火山碎屑的不同形状,包括晶体和气泡
IF 2.3 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-01-17 DOI: 10.1016/j.jvolgeores.2026.108534
Sayaka Oda, Atsuko Namiki
Low-viscosity basaltic and basaltic andesitic magmas form pyroclastic materials with various shapes, such as scoria, volcanic ash, and Pele’s hair, through fracturing. Brittle fracture of low-viscosity magma is unlikely. Instead, fluid dynamical deformation during the eruption may cause the magma to tear off. The various morphologies of pyroclast shapes should be determined by their deformation history. High crystallinity in magma increases its effective viscosity, potentially enabling brittle-like fracture. To understand how the shape of pyroclastic material produced by low-viscosity magma is determined, we conducted uniaxial extension experiments using a magma analog mixture of liquid, solid, and gas phases. Our experiments demonstrate that fluids with a high solid particle fraction (>0.3) tend to tear off at a small strain, thereby generating a rough fracture surface. The solid particles were undeformable, and a high particle fraction reduced the thickness of the deformable liquid region. Thin liquid films are easily disrupted, and thus a small strain can break the entire fluid. In contrast, a particle-free bubbly fluid generates thin threads. Bubbles can coalesce to create a large bubble and deform. Vertically elongated bubbles split the fluid in the longitudinal direction, forming threads. The former mechanism may generate the irregularly shaped scoriae, and the latter forms Pele’s hair. Our experimental results indicate that suspended crystals and bubbles in magma affect not only the physical properties of magma but also the fracture manner, thereby determining the shapes of pyroclasts.
低粘度玄武岩和玄武岩安山岩岩浆通过压裂形成各种形状的火山碎屑物质,如矿渣、火山灰和贝利的头发。低粘度岩浆不太可能发生脆性断裂。相反,喷发过程中的流体动力变形可能会导致岩浆脱落。火山碎屑形状的各种形态应由其变形历史决定。岩浆的高结晶度增加了它的有效粘度,可能导致脆性断裂。为了了解低粘度岩浆产生的火山碎屑物质的形状是如何确定的,我们使用液体、固体和气体相的岩浆模拟混合物进行了单轴伸展实验。我们的实验表明,高固体颗粒分数(>0.3)的流体倾向于在小应变下撕裂,从而产生粗糙的断口表面。固体颗粒是不可变形的,高颗粒含量减少了可变形的液体区域的厚度。薄的液体薄膜很容易被破坏,因此一个小的应变可以破坏整个流体。相反,无颗粒的气泡流体会产生细线。气泡可以合并形成一个大气泡并变形。垂直拉长的气泡在纵向上分裂流体,形成螺纹。前者的机制可能产生不规则形状的疤痕,后者形成贝利的头发。实验结果表明,岩浆中的悬浮晶体和气泡不仅影响岩浆的物理性质,而且影响破裂方式,从而决定火山碎屑的形状。
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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 : 2026-01-15 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
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 : 2026-01-12 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。
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引用次数: 0
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Journal of Volcanology and Geothermal Research
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