利用自然样品、实验和热力学模型评估岩浆储存深度的有效性——以美国NM的Valles Caldera为例

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Magdalen A. Grismer, Laura E. Waters, Gordon M. Moore, Gabriela A. Farfan
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引用次数: 0

摘要

岩浆储量的估计通常是通过自然样品中的矿物组合、实验和热力学模型(例如熔融体)来进行的,每种方法都有局限性。在这里,我们比较了每一种方法,以评估它们在估计崩塌后的储存条件方面的效用,来自Valles Caldera, NM(美国)的两长石高硅流纹岩(hsr)。我们重点研究了Valle Grande高铁,这些高铁已知整个岩石、玻璃成分、结晶度和储存条件(~ 750-770°C;∼130 - 165 MPa)。平衡实验与样品岩石学确定的岩浆储存条件重叠,其玻璃和矿物成分与自然样品中的玻璃和矿物成分相匹配,表明斑晶组合准确地记录了喷发前的条件。rmelt再现了天然样品和实验的不同方面,但通常确认存储条件(751-758°C;塌陷后高硅流纹岩岩石学记录。rmelt在±5°C,压力>;125 MPa下再现实验确定的相进曲线。在125 MPa以下,rmelt对实验石英、水晶石和斜长石的稳定性预测过高。我们将rmelt地热气压计应用于玻璃山黑曜岩(双长石高铁),以评估rmelt、实验和Valle Grande高铁之间一致性的可能原因。rmelt地热气压计将玻璃山黑曜岩的温度高估了50-77°C,并可能低估了压力。rmelt预测这两种HSRS的共饱和温度为~ 750°C。我们发现rmelt恢复了Valle Grande HSRS的储存温度和压力,因为它们的温度为~ 750°C,含有<;30%的总结晶度,接近平衡,储存在>; MPa。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Efficacy of Assessing Magmatic Storage Depth Using Natural Samples, Experiments and Thermodynamic Models: A Case Study From Valles Caldera, NM (USA)

Efficacy of Assessing Magmatic Storage Depth Using Natural Samples, Experiments and Thermodynamic Models: A Case Study From Valles Caldera, NM (USA)

Estimates of magmatic storage are typically made using mineral assemblages in natural samples, experiments and thermodynamic models (e.g., MELTS), where each method has limitations. Here, we compare each of these methods to assess their utility in estimating storage conditions for post-collapse, two-feldspar high-silica rhyolites (HSRs) sourced from Valles Caldera, NM (USA). We focus on the Valle Grande HSRs, which have known whole rock, glass compositions, crystallinities and storage conditions (∼750–770°C; ∼130–165 MPa). Equilibrium experiments that overlap with magmatic storage conditions determined from sample petrology have glass and mineral compositions that match those in the natural samples, suggesting that the phenocryst assemblage is accurately recording pre-eruptive conditions. RMELTS reproduces differing aspects of the natural samples and experiments, but generally confirm storage conditions (751–758°C; 179–215 MPa) recorded by the petrology of the post-collapse high-silica rhyolites. RMELTS reproduces the experimentally determined phase-in curves within ±5°C, at pressures >125 MPa. Below 125 MPa, RMELTS overpredicts the stability of the experimental quartz, sanidine and anorthoclase. We apply the RMELTS geothermobarometer to the Glass Mountain obsidians (two-feldspar HSRs) to evaluate possible reasons for the agreement between RMELTS, experiments, and Valle Grande HSRs. The RMELTS geothermobarometer overpredicts the Glass Mountain obsidians' temperatures by 50–77°C, and likely underpredicts pressures. RMELTS predicts a common co-saturation temperature of ∼750°C for these two HSRS. We find that RMELTS recovers the storage temperature and pressures for Valle Grande HSRS because they have temperatures of ∼750°C, contain <30% total crystallinity, are near equilibrium and are stored at >125 MPa.

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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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