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Emplacement of channeled flows in subaerial, submarine, simulated, and extraterrestrial environments.

机译:在海底,海底,模拟和外星环境中通道流的位置。

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摘要

Channeled lava flows are observed in a range of volcanic environments including shield volcanoes in Hawai'i, in submarine lava flows along mid-ocean ridges, and on the flanks of volcanoes in the Tharsis Region on Mars. Observations of the final channel morphology are a primary means for interpreting how the lava flow was emplaced, including rheologic properties of the lava, effusion rates, and eruption duration. To better understand the emplacement of lava flows, I performed laboratory simulations using polyethylene glycol wax (PEG). These channeled flows reflect a range of compositions (PEG, basalt, dacite), lengths (centimeters to kilometers), and emplacement durations (minutes to years). I find that all the flows show a downstream change in morphology, consistent with morphologic zones (stable, transitional, zone of dispersed flow, flow toe) described by Lipman and Banks [1987] regardless of scale or composition. Lava channels in the extraterrestrial environments can have greater dimensions than terrestrial flows. One particular channeled lava flow near Ascraeus Mons volcano on Mars is 690 km long. I analyze this Ascraeus Mons flow using high-resolution (4.5 to 32 m/pixel) images from Mars Orbiter Camera (MOC) and Thermal Emissions Imaging System (THEMIS) and elevation data from the Mars Orbiter Laser Altimeter (MOLA). I calculate a minimum effusion rate of 19,000--29,000 m3/s from the Graetz number and durations of ∼100--250 days assuming constant flow rates and a continuous eruption. Textures that form in channeled PEG flows are similar to textures observed in submarine channeled lava flows along the East Pacific Rise (9°--10°N). Channeled PEG flows consistently display the following surface textures in the channel: smooth, folded, lineated, and chaotic, which are analogous to smooth, folded, lineated, and jumbled textures in submarine channels. Observations of the formation of surface textures in the PEG channels are applied to the formation of textures in submarine lava channels. I mapped the surface textures preserved in the final flow morphology of 10 channeled PEG flows and 9 submarine lava channels. (Abstract shortened by UMI.)
机译:在一系列火山环境中观察到窜流的熔岩流,包括夏威夷的盾构火山,沿洋中脊的海底熔岩流以及火星上塔西斯地区的火山侧面。观察最终通道的形态是解释熔岩流如何发生的主要手段,包括熔岩的流变特性,渗出速率和喷发持续时间。为了更好地了解熔岩流的位置,我使用聚乙二醇蜡(PEG)进行了实验室模拟。这些引导流反映了一定范围的成分(PEG,玄武岩、,石),长度(厘米至千米)和进位持续时间(分钟至几年)。我发现所有流动都显示出下游的形态变化,与Lipman和Banks [1987]描述的形态学区域(稳定,过渡,分散流动的区域,流动趾)一致,而不论其规模或组成如何。地外环境中的熔岩通道可能比地面流具有更大的尺寸。火星Ascraeus Mons火山附近的一种特殊的导流熔岩流长690公里。我使用来自火星轨道相机(MOC)和热发射成像系统(THEMIS)的高分辨率图像(来自火星轨道激光测高仪(MOLA)的高程数据)来分析这种Ascraeus Mons流。我假设流量恒定且连续喷发,根据Graetz数和持续时间约100--250天计算出的最小积水速率为19,000--29,000 m3 / s。在通道PEG流中形成的纹理类似于在沿东太平洋上升带(9°--10°N)的海底通道熔岩流中观察到的纹理。引导的PEG流在通道中始终显示以下表面纹理:平滑,折叠,带线和混乱,类似于海底通道的平滑,折叠,带线和混乱的纹理。 PEG通道中表面纹理形成的观察结果被应用于海底熔岩通道中纹理的形成。我绘制了保留在10条通道PEG流和9条海底熔岩通道的最终流动形态中的表面纹理。 (摘要由UMI缩短。)

著录项

  • 作者

    Garry, William Brent.;

  • 作者单位

    State University of New York at Buffalo.;

  • 授予单位 State University of New York at Buffalo.;
  • 学科 Geology.
  • 学位 Ph.D.
  • 年度 2006
  • 页码 255 p.
  • 总页数 255
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 地质学;
  • 关键词

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