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Parry arc: a polarization lidar, ray-tracing, and aircraft case study

机译:帕里弧:极化激光雷达,射线追踪和飞机案例研究

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摘要

Using simple ray-tracing simulations, the cause of the rare Parry arc has been linked historically to horizontally oriented columns that display the peculiar ability to fall with a pair of prism faces closely parallel to the ground. Although we understand the aerodynamic forces that orient the long-column axis in the horizontal plane, which gives rise to the relatively common tangent arcs of the 22° halo, the mechanism leading to the Parry crystal orientation has never been resolved adequately. On 16 November 1998, at the University of Utah Facility for Atmospheric Remote Sensing, we studied a cirrus cloud producing a classic upper Parry are using polarization lidar and an aircraft with a new highresolution ice crystal imaging probe. Scanning lidar data, which reveal extremely high linear depolarization ratios δ a few degrees off the zenith direction, are simulated with ray-tracing theory to determine the ice crystal properties that reproduce this previously unknown behavior. It is found that a limited range of thick-plate crystal axis (length-to-diameter) ratios from ~0.75 to 0.93 generates a maximum δ≈2.0-5.0 for vertically polarized 0.532-μm light when the lidar is tilted 1°-2° off the zenith. Halo simulations based on these crystal properties also generate a Parry arc. However, although such particles are abundant in the in situ data in the height interval indicated by the lidar, one still has to invoke an aerodynamic stabilization force to produce properly oriented particles. Although we speculate on a possible mechanism, further research is needed into this new explanation for the Parry arc.
机译:使用简单的光线跟踪模拟,罕见的Parry弧的原因在历史上一直与水平定向的列相关联,这些列显示了在一对平行于地面的棱柱面上掉落的独特能力。尽管我们了解了将长柱轴定向在水平面上的空气动力,这会引起22°光晕的相对切线弧,但导致帕里晶体取向的机理尚未得到充分解决。 1998年11月16日,我们在犹他大学大气遥感设施中研究了卷云,该卷云使用偏振激光雷达和带有新型高分辨率冰晶成像探头的飞机制造了经典的帕里上层。扫描激光雷达数据显示出与天顶方向相距几度的极高线性去极化比δ,并使用射线跟踪理论进行模拟,以确定可重现此先前未知行为的冰晶特性。研究发现,当激光雷达倾斜1°-2时,对于垂直偏振的0.532-μm光,厚板晶轴(长径比)的范围从0.75到0.93会产生最大δ≈2.0-5.0 °脱离天顶。基于这些晶体特性的光晕模拟也会生成帕里弧。但是,尽管在激光雷达指示的高度间隔中,此类粒子在原位数据中很丰富,但仍必须调用气动稳定力才能产生正确定向的粒子。尽管我们推测了一种可能的机制,但仍需要进一步研究帕里弧的这一新解释。

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