...
首页> 外文期刊>Boundary-layer Meteorology >Use of a High-Resolution Sodar to Study Surface-layer Turbulence at Night
【24h】

Use of a High-Resolution Sodar to Study Surface-layer Turbulence at Night

机译:使用高分辨率声雷达在夜间研究表面层湍流

获取原文
获取原文并翻译 | 示例
           

摘要

Measurements in the atmospheric surface layer are generally made with point sensors located in the first few tens of metres. In most cases, however, these measurements are not representative of the whole surface layer. Standard Doppler sodars allow a continuous display of the turbulent thermal structure and wind profiles in the boundary layer up to 1000 m, with a few points, if any, in the surface layer. To overcome these limitations a new sodar configuration is proposed that allows for a higher resolution in the surface layer. Because of its capabilities (echo recording starting at 2 m, echo intensity vertical resolution of approximately 2 m, temporal resolution of 1 s) this sodar is called the surface-layer mini-sodar (SLM-sodar). Features and capabilities of the SLM-sodar are described and compared with the sodar. The comparison of the thermal vertical structure given by the SLM-sodar and the sodar provides evidence that, in most cases, the surface layer presents a level of complexity comparable to that of the entire boundary layer. Considering its high vertical resolution, the SLM-sodar is a promising system for the study of the nocturnal surface layer. The nocturnal SLM-sodar measurements have shown that, depending on wind speed, the structure of the surface layer may change substantially within a short time period. At night, when the wind speed is greater than 3 m s(-1), mechanical mixing destroys the wavy structure present in the nocturnal layer. Sonic anemometer measurements have shown that, in such cases, also the sensible heat flux varies with height, reaching a peak in correspondence with the wind speed peak. Under these conditions the assumption of horizontal homogeneity of the surface layer and the choice of the averaging time need to be carefully treated.CT 15th International Symposium for the Advancement of Boundary-Layer Remote Sensing (ISARS)CY JUN 28-30, 2010CL Univ Versailles St-Quentin-en-Yvelines, Inst Pierre Simon Laplace (IPSL), Paris, FRANCEHO Univ Versailles St-Quentin-en-Yvelines, Inst Pierre Simon Laplace (IPSL)SP Ecole Polytechnique; CASQY; Ctr Natl Etudes Spatiales (CNES); CNRS-INSU; EU Program COST; LATMOS; Lab Meteorol Dynamique (LMD); Leosphere; Meteo France; Reg Ile-de-France
机译:通常使用位于前几十米的点传感器进行大气表层的测量。但是,在大多数情况下,这些测量值不能代表整个表面层。标准多普勒声雷达可连续显示边界层中高达1000 m的湍流热结构和风廓线,而在表层中还有一些点(如果有的话)。为了克服这些限制,提出了一种新的声雷达配置,该声雷达配置允许在表面层中具有更高的分辨率。由于其功能(回声记录从2 m开始,回声强度垂直分辨率约为2 m,时间分辨率为1 s),此声dar被称为表面层微型声dar(SLM-声dar)。描述并比较了SLM声雷达的功能和特性。 SLM声雷达和声雷达给出的热垂直结构的比较提供了证据,表明在大多数情况下,表面层的复杂程度可与整个边界层相比。考虑到其高垂直分辨率,SLM-sodar是用于研究夜表层的有前途的系统。夜间SLM声雷达测量表明,取决于风速,表面层的结构可能会在短时间内发生显着变化。在晚上,当风速大于3 m s(-1)时,机械混合会破坏夜间层中存在的波浪形结构。音速风速仪的测量表明,在这种情况下,显热通量也会随高度而变化,达到与风速峰值相对应的峰值。在这种情况下,应仔细考虑表层水平均匀性的假设和平均时间的选择。CT第15届国际边界层遥感技术研讨会(ISARS)CY JUN 28-30,2010年,CL凡尔赛大学巴黎皮埃尔·西蒙·拉普拉斯学院(IPSL)的圣昆汀·恩·伊夫林(法国巴黎)皮埃尔·西蒙·拉普拉斯学院的圣昆汀·昂夫林(IPSL)的SP Ecole Polytechnique; CASQY; Ctr Natl Etudes Spatiales(CNES); CNRS-INSU;欧盟计划成本;拉莫斯Lab Meteorol Dynamique(LMD);狮子座法国Meteo;法兰西岛大区

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号