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Numerical analysis of conditions necessary for near-surface snow metamorphism.

机译:近地表雪变质必要条件的数值分析。

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摘要

Faceted snow crystals develop at or near the snow surface due to temperature gradients. After burial, snow avalanches regularly fail on these layers. Generally, surface hoar deposits when the snow surface is cooler than the surrounding environment; near-surface facets form when the subsurface is warmed by solar radiation and the surface is cooled by radiative, convective, and latent heat exchange.;Field research stations were established that included daily observations and meteorological data. In two seasons, 14 surface hoar and 26 near-surface facet events were recorded. Statistical analysis of the surface hoar events indicated three factors that were related to surface hoar growth: incoming long-wave radiation, snow surface temperature, and relative humidity. The ideal conditions for each of these parameters were 190--270 W/m 2, -22 to -11°C, and 45--80%, respectively. For near-surface facet formation, long- and short-wave radiation and relative humidity were statistically linked to the events. The ideal conditions for these parameters ranged from 380--710 W/m2, 210--240 W/m2, and 23--67%, respectively.;Using a thermal model, sensitivity analysis, and Monte Carlo simulations the conditions that lead to facet formation were explored. Based on computed mass-flux, the formation of surface hoar was mainly driven by changes in long-wave radiation, air temperature, wind velocity, and relative humidity. From these terms graphical tools were developed to predict surface hoar; the numerical results matched reasonably well with the field observations. Based on the presence of a specific temperature gradient understood to lead to near-surface facets, three terms were determined to be the most in uential: density, thermal conductivity, and incoming long-wave radiation. Using these terms, albedo, and incoming short-wave radiation---a requirement for radiation-recrystallization---a means for predicting the presence of near-surface facets was presented.;The physical and analytical data presented indicates that incoming long-wave radiation is the most influential parameter governing the conditions that lead to surface hoar and near-surface facet growth. The analysis suggests that snow with low density and high thermal conductivity may be conducive to the formation of near-surface facets.
机译:由于温度梯度,在雪表面处或附近会形成多面雪晶体。埋葬后,雪崩经常在这些层上失败。通常,当雪面温度低于周围环境时,会形成表层灰浆。当地下被太阳辐射加热并通过辐射,对流和潜热交换使表面冷却时,形成近地表小面。;建立了包括每日观测和气象数据的野外研究站。在两个季节中,记录了14次表面灰白事件和26次近表面小面事件。地表灰浆事件的统计分析表明与地表灰浆生长有关的三个因素:入射长波辐射,雪地表温度和相对湿度。每个参数的理想条件分别为190--270 W / m 2,-22至-11°C和45--80%。对于近地表小面的形成,长波和短波辐射以及相对湿度在统计上与事件有关。这些参数的理想条件分别为380--710 W / m2、210--240 W / m2和23--67%.;使用热模型,灵敏度分析和Monte Carlo模拟可以得出导致探索小面的形成。基于计算的质量通量,地表灰白的形成主要是由长波辐射,空气温度,风速和相对湿度的变化驱动的。根据这些术语,开发了图形工具来预测表面起泡。数值结果与现场观测结果吻合得很好。根据特定的温度梯度(可导致近表面小平面)的存在,确定以下三个项的电势最大:密度,导热率和入射长波辐射。使用这些术语,反照率和入射短波辐射-辐射重结晶的要求-提出了一种预测近表面刻面存在的方法。;所提供的物理和分析数据表明,入射长波-波辐射是控制导致表面白化和近表面小面生长的条件的最具影响力的参数。分析表明,低密度和高导热率的积雪可能有助于形成近地表小面。

著录项

  • 作者

    Slaughter, Andrew Edward.;

  • 作者单位

    Montana State University.;

  • 授予单位 Montana State University.;
  • 学科 Engineering Civil.;Atmospheric Sciences.
  • 学位 Ph.D.
  • 年度 2010
  • 页码 603 p.
  • 总页数 603
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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