首页> 外文学位 >CONVECTIVE SCALE INTERACTION: ARC CLOUD LINES AND THE DEVELOPMENT AND EVOLUTION OF DEEP CONVECTION (SATELLITE METEOROLOGY, THUNDERSTORMS).
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CONVECTIVE SCALE INTERACTION: ARC CLOUD LINES AND THE DEVELOPMENT AND EVOLUTION OF DEEP CONVECTION (SATELLITE METEOROLOGY, THUNDERSTORMS).

机译:对流尺度相互作用:弧云线与深对流的发展和演变(卫星气象学,雷暴)。

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摘要

Information from satellite data and research aircraft data are used to provide new understanding concerning the mesoscale development and evolution of deep convection in an atmosphere typified by weak synoptic-scale forcing. The major topic covered is the importance of convective scale interaction in the development and evolution of deep convection. This interaction is shown to manifest itself as the merger and intersection of thunderstorm outflow boundaries (arc cloud lines) with other convective lines, areas or boundaries.; Using geostationary satellite visible and infrared data convective scale interaction is shown to be responsible for over 85% of the intense convection (colder than -42(DEGREES)C) over the southeast United States by late afternoon (6 pm local), and an overwhelming majority of that area's afternoon rainfall.; Using satellite image and sounding data, as well as research aircraft information, it is shown how variations in a local environment's ability to support strong convection may be determined. Using this information, coupled with information about the arc cloud line's life cycle, four distinct properties of convective scale interaction are analyzed. (1) Thunderstorm outflow boundaries may maintain their identity as arc cloud lines for several hours after they have moved away from their parent source. (2) The arc cloud line outflow boundary can, and often does, cause deep convection to develop along it at distances well over 150 km from its point of generation. (3) Deep convective development along an outflow boundary is a selective process--it only occurs where the arc cloud line merges with a cumulus region or intersects another boundary. When the arc cloud line moves into clear skies no deep convection develops. (4) As the cumulus regime evolves on a given day, and much of the cumulus field dies away, the majority of new thunderstorms are confined to arc cloud line intersection points.
机译:来自卫星数据和研究飞机数据的信息用于提供有关以对流尺度强迫为代表的大气中深对流的中尺度发展和演变的新认识。涉及的主要主题是对流尺度相互作用在深度对流发展和演化中的重要性。这种相互作用表现为雷暴流出边界(弧云线)与其他对流线,区域或边界的合并和交汇。使用对地静止卫星可见和红外数据对流尺度的相互作用表明,到午后(当地时间下午6点),美国东南部的强对流(超过-42(DEGREES)C)的比例超过了85%,并且压倒性多数该地区大部分下午的降雨。使用卫星图像和探测数据以及研究飞机的信息,可以显示如何确定本地环境支持强对流的能力的变化。使用此信息,再加上有关弧云线生命周期的信息,对流尺度相互作用的四个不同属性进行了分析。 (1)雷暴流出边界在离开其父源后可能会保持其作为弧云线的身份长达几个小时。 (2)弧云线出流边界可以并且经常确实引起深对流,在距其生成点超过150 km的距离处沿其发展。 (3)沿流出边界的深对流发展是一个选择性过程-仅在弧云线与积云区域合并或与另一个边界相交的情况下发生。当弧云线移到晴朗的天空时,不会形成深对流。 (4)随着积云制度在某一天的发展,并且许多积云场都消失了,大多数新的雷暴都被限制在弧云线相交点。

著录项

  • 作者单位

    Colorado State University.;

  • 授予单位 Colorado State University.;
  • 学科 Physics Atmospheric Science.
  • 学位 Ph.D.
  • 年度 1986
  • 页码 218 p.
  • 总页数 218
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 大气科学(气象学);
  • 关键词

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