EAPSI:3-D Numerical Modeling of the 35-40E mid-ocean ridge segment along the Southwest Indian Ridge

EAPSI：西南印度洋中脊 35-40E 洋中脊部分的 3-D 数值模拟

• 批准号: 1414893
• 负责人: Mark Larson
• 金额: $ 0.5万
• 依托单位: Larson Mark O
• 依托单位国家: 美国
• 项目类别: Fellowship Award
• 财政年份: 2014
• 资助国家: 美国
• 起止时间: 2014-06-01 至 2015-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1414893&HistoricalAwards=false
• 关键词: EAPSI; Numerical; Modeling; 35; 40E

Mid-ocean ridges are where a large part of the Earth's volcanism, and significant earthquakes occur. However, the mid-ocean ridges are just the surface expression of the larger convecting mantle system and this mantle is poorly understood. This project aims to explain how the mantle supplies material to the surface of the Earth, and how the mantle moves near the surface. Geodynamic modeling is one of the only ways that currently exists to investigate the mantle processes at mid-ocean ridges and to uncover the geologic history there. Geological observations make modeling more realistic. In this project, the properties of rocks collected from the Southwest Indian Ridge will be compared with many simulated magma compositions, which will then be used to find the properties of the mantle beneath the observed rocks' source. This will grant a better understanding of the ridges in general, as well as hotspot-ridge interaction zones. Collaboration with Dr. Okino's group at the University of Tokyo, will allow for the utilization of novel techniques in order to trace the magma source of the ridge and to explain heterogeneity along the ridge axis.In 2007 and 2009, 35-40 degrees segment of the Southwest Indian Ridge where mantle-derived rocks and geophysical data were collected. This segment is the nearest to the Marion hotspot and is anomalous from other hotspot-ridge regions around the globe in that it experiences a low magma flux, and the rocks have a very different chemical composition from rocks found at other hotspot-ridge regions. COMSOL Multiphysics© will be used for calculation of the physical properties of the segment. MELTS software will be used to forward model the geochemical tracing to infer source geometry and composition and melt pathways. Forward modeling of the gravity and magnetic fields of the produced models using MATLAB will allow us to further constrain the density, depth and geometry of the mantle melt regime, leading to a better understanding of the mantle system as a whole. Incorporating the geochemical, and geophysical data to the model represents a fundamental advancement of the ridge modeling process and combining geodynamic models with observational data. This NSF EAPSI award is funded in collaboration with the Japan Society for the Promotion of Science.

海洋中脊是地球上大部分火山活动和重大地震发生的地方。然而，洋中脊只是更大的对流地幔系统的表面表现，人们对这种地幔知之甚少。这个项目旨在解释地幔如何向地球表面提供物质，以及地幔如何在地表附近移动。地球动力学建模是目前研究洋中脊地幔过程和揭示那里地质历史的唯一方法之一。地质观测使建模更加真实。在这个项目中，从西南印度海岭收集的岩石的性质将与许多模拟的岩浆成分进行比较，然后将用于发现观察到的岩石来源下的地幔的性质。这将使我们更好地了解山脊的总体情况，以及热点-山脊的相互作用区。与东京大学冲野博士的团队合作，将允许利用新技术来追踪山脊的岩浆来源，并解释沿山脊轴线的非均质性。2007年和2009年，在西南印度洋脊35-40度段收集了地幔源岩石和地球物理数据。这部分是离马里恩热点最近的，与全球其他热点-山脊区域不同，因为它经历了较低的岩浆通量，岩石的化学成分与其他热点-山脊区域的岩石非常不同。COMSOL Multiphysics©将用于计算分段的物理特性。将使用melt软件对地球化学示踪进行正演模拟，以推断源的几何形状、成分和熔体路径。利用MATLAB对生成的模型的重力和磁场进行正演建模，将使我们能够进一步约束地幔熔体的密度、深度和几何形状，从而更好地理解整个地幔系统。将地球化学和地球物理资料结合到模型中，是脊模拟过程和地球动力学模型与观测资料相结合的根本进步。NSF EAPSI奖是与日本科学促进会合作资助的。