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Analysis of planetary boundary layer wind and thermodynamic structures over Great Bear Lake during varying synoptic-scale regimes.

机译:分析不同天气尺度下大熊湖的行星边界层风和热力结构。

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摘要

Surface observations, lake evaporation data and upper-air soundings were collected in a special data-collection effort during the months of August and September of 2004 and 2005 on an island in the middle of Great Bear Lake, Northwest Territories. For this period of the year, the late summer, when increasing variability in surface pressure starts occurring, the effect of different synoptic-scale regimes on the lake-atmosphere interface is investigated to understand the regional specificities, with comparisons to nearby stations and a high spatial and temporal resolution reanalysis model (North American Regional Reanalysis). The planetary boundary layer over the lake systematically shows typical surface and mixed layer structures but with varying depths depending on the mean lower tropospheric temperature. Inversions in the surface layer, linked with warm regimes, support deep mixed layers. Within the surface layer, during warm regimes, a superadiabatic lapse rate can support (or not) a higher-stability sublayer on top of it, in which case the mixed layer happens to be much deeper. The first mechanism for lake evaporation includes the occasional passage of synoptic-scale storm systems with both warm and cold frontal features creating strong, short-lived latent heat interactions between the lake and the atmosphere, but relatively low total amounts of evaporation. The main mechanism for extensive evaporation is a cold anticyclone allowing for significant daytime insolation. A lake-breeze circulation can then develop and provide strong-enough mesoscale winds for diurnal upward latent heat exchanges, with wind channelling into Keith Arm of the lake for strong lake-breeze onshore winds.
机译:2004年8月,2004年9月和2005年9月,在西北地区大熊湖中部的一个小岛上,通过特殊的数据收集工作收集了地表观测,湖泊蒸发数据和高空探测数据。在这一年的夏季末期,当开始出现地表压力变化的时候,研究了不同天气尺度制度对湖泊-大气界面的影响,以了解区域的特殊性,并与附近的气象站进行了比较,结果表明,时空分辨率再分析模型(北美区域再分析)。湖上的行星边界层系统地显示出典型的表层和混合层结构,但深度的变化取决于对流层平均较低温度。与温暖状态有关的表层反演支持深层混合层。在表层内部,在温暖的天气条件下,超级绝热流失速率可以支持(或不支持)其顶部更高的稳定性子层,在这种情况下,混合层恰好更深。湖泊蒸发的第一个机制包括天气尺度的暴风雨系统偶尔通过,同时具有锋面和冷锋特征,在湖泊和大气之间产生强的,短暂的潜热相互作用,但蒸发总量相对较低。大量蒸发的主要机理是冷的反气旋,可在白天大量暴晒。然后,湖风循环会发展并提供足够强的中尺度风,以进行日向上的潜热交换,风会进入湖的Keith Arm,从而产生强劲的湖风陆上风。

著录项

  • 作者

    Milewski, Thomas.;

  • 作者单位

    McGill University (Canada).;

  • 授予单位 McGill University (Canada).;
  • 学科 Physics Astronomy and Astrophysics.; Atmospheric Sciences.
  • 学位 M.Sc.
  • 年度 2006
  • 页码 93 p.
  • 总页数 93
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;
  • 关键词

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