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A comparative planetological study of particle speed and concentration during aeolian saltation.

机译:风沙盐化过程中粒子速度和浓度的比较行星学研究。

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摘要

Aeolian gradation is important on any planetary surface possessing loose particulate material and winds of sufficient strength to initiate motion. The mode of aeolian transport with the greatest potential for geologic alteration is saltation, where sand-sized particles bounce along the surface. The goals of this dissertation are to: determine the relative contributions of particle concentration and particle speed to saltation flux for a wide range of environmental conditions, extrapolate the saltation flux predictions of previous investigators to non-terrestrial conditions, determine the range of environmental conditions over which those predictions remain valid, and assess the nature and consequences of aeolian activity on other planets.; Flux predictions developed for terrestrial saltation were found to be valid for a narrower range of wind speeds on Mars and Venus than in the terrestrial case. On Mars, low atmospheric density impairs the full development of saltation; on Venus, particle trajectories are so small that mid-air collisions readily impede, or choke, saltation. Actual saltation flux can be several orders of magnitude less than predicted, due to these and other environmental factors. The height of the zone of aeolian abrasion of surface materials is inversely proportional to the atmospheric density and the intensity of abrasion. The spectrum of particle speeds and the trajectory heights in the saltation cloud are controlled by surface conditions; particle size, shape, and density and wind speed. The particle speed distribution is more complex than previously supposed, particularly for particles that are relatively large and dense. Particle speed and flux distribution above the surface profoundly affects both the style and rate of small-scale aeolian erosion and bedform development. The onset of choking conditions in the saltation cloud can be considered to be a change in flow regimes, analogous to the change in flow regimes in water from that producing rippled bedforms to that producing plane beds.
机译:在任何具有松散的颗粒物质和具有足够强度以发起运动的风的行星表面上,风积梯度都很重要。地质变化潜力最大的风沙运输方式是盐化,其中沙粒沿着表面反弹。本文的目的是:确定在各种环境条件下颗粒浓度和颗粒速度对盐分通量的相对贡献,将先前研究人员的盐分通量预测推算到非陆地条件下,确定环境条件在这些预测中哪些保持有效,并评估风能活动在其他行星上的性质和后果?与陆相情况相比,火星和金星的风速范围更窄,因此针对陆盐形成的通量预测被发现是有效的。在火星上,低的大气密度会破坏盐分的充分发展。在金星上,粒子的轨迹是如此之小,以至空中碰撞很容易阻止或阻塞盐分。由于这些和其他环境因素,实际的盐分通量可能比预期的少几个数量级。表面材料的风蚀磨损区的高度与大气密度和磨蚀强度成反比。盐雾云中的粒子速度谱和轨迹高度受表面条件控制。粒径,形状,密度和风速。粒子速度分布比以前想象的要复杂,特别是对于相对较大和密集的粒子。表面上的粒子速度和通量分布深刻地影响着小规模风蚀和床形发育的样式和速度。盐雾云中窒息条件的发生可以认为是流态的变化,类似于水中的流态从产生波纹状床状床到平面床的变化。

著录项

  • 作者

    Williams, Steven Hamilton.;

  • 作者单位

    Arizona State University.;

  • 授予单位 Arizona State University.;
  • 学科 Geology.; Physics Astronomy and Astrophysics.
  • 学位 Ph.D.
  • 年度 1987
  • 页码 170 p.
  • 总页数 170
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 地质学;天文学;
  • 关键词

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