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Cirrus crystal fall velocity estimates using the Match method with ground-based lidars: first investigation through a case study

机译:利用Match方法与地基激光雷达对卷云晶体坠落速度进行估算:首先通过案例研究

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Cirrus ice particle sedimentation velocity (v_s) is one of the critical variables for the parameterization of cirrus properties in a global climate model (GCM). In this study a methodology to estimate cirrus properties, such as crystal mean fall speed, through successive lidar measurements is evaluated. This "Match" technique has been applied on cirrus cloud observations and then tested with measurements from two ground-based lidars located in the Mediterranean area. These systems, with similar instrumental characteristics, are installed at the Observatory of Haute Provence (OHP, 43.9° N, 5.7° E) in France and at Rome Tor Vergata (RTV, 41.8° N, 12.6° E) in Italy. At a distance of approximately 600 km, the two lidar stations have provided systematic measurements for several years and are along a typical direction of an air path. A test case of an upper tropospheric cirrus, observed over both sites during the night between 13 and 14 March 2008, has been selected and the feasibility of the Match-cirrus approach investigated through this case. The analysis through lidar principal parameters (vertical location, geometrical thickness and optical depth) reveals a case of a thin sub-visible cirrus (SVC) located around the tropopause. A first range of values for v_s (1.4-1.9 cm s~(-1), consistent with simple-shaped small crystals) has been retrieved with a simplified approach (adiabatic transport and "frozen" microphysical conditions inside the cirrus). The backward trajectory analysis suggests a type of cirrus formed by large-scale transport processes (adiabatic cooling of moist air masses coming from the subtropical area around Mexico gulf), which is characterized by a long atmospheric lifetime and horizontal extension of several hundred km. The analysis of this case study reveals that many uncertainties reduce the confidence of the retrieved estimates of the crystal fall velocity. However, this paper allows for assessing the technique feasibility by identifying the main critical issues for future similar investigations. This study shows that such approach is feasible; however, the methodology should be improved and some directions have been suggested for future campaigns.
机译:卷云冰粒沉降速度(v_s)是全球气候模型(GCM)中卷云属性参数化的关键变量之一。在这项研究中,评估了通过连续激光雷达测量估算卷云特性(例如晶体平均下降速度)的方法。这种“匹配”技术已应用于卷云观测,然后通过位于地中海地区的两个地面激光雷达的测量结果进行了测试。这些具有类似仪器特性的系统安装在法国的上普罗旺斯天文台(OHP,北纬43.9°,东经5.7°)和意大利的罗马维尔塔塔(RTV,北纬41.8°,北纬12.6°)。在大约600 km的距离上,这两个激光雷达站已经进行了数年的系统测量,并且沿风路的典型方向。选择了在2008年3月13日至14日夜间在两个站点上观测到的对流层高卷云的测试案例,并通过该案例研究了Match-cirrus方法的可行性。通过激光雷达的主要参数(垂直位置,几何厚度和光学深度)进行的分析揭示了位于对流层顶周围的薄亚可见卷云(SVC)的情况。 v_s的第一个值范围(1.4-1.9 cm s〜(-1),与简单形状的小晶体一致)已通过简化方法(绝热传输和卷云内部的“冻结”微物理条件)获得了。向后的轨迹分析表明,是由大规模的运输过程(来自墨西哥湾附近的亚热带地区的湿空气的绝热冷却)形成的卷云,其特点是大气寿命长,水平延伸几百公里。对本案例研究的分析表明,许多不确定性降低了所获得的晶体下落速度估算值的可信度。但是,本文允许通过确定未来类似研究的主要关键问题来评估技术的可行性。这项研究表明这种方法是可行的。但是,应该改进方法,并为未来的运动提出了一些指导。

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