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Atmospheric Characterization on the Kennedy Space Center Shuttle Landing Facility

机译:肯尼迪航天中心航天飞机着陆设施的大气特征

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Large temperature gradients are a known source of strong atmospheric turbulence conditions. Often times these areas of strong turbulence conditions are also accompanied by conditions that make it difficult to conduct long term optical atmospheric tests. The Shuttle Landing Facility (SLF) at the Kennedy Space Center (KSC) provides a prime testing environment that is capable of generating strong atmospheric turbulence yet is also easily accessible for well instrumented testing. The Shuttle Landing Facility features a 5000 m long and 91 m wide concrete runway that provides ample space for measurements of atmospheric turbulence as well as the opportunity for large temperature gradients to form as the sun heats the surface. We present the results of a large aperture LED scintillometer, a triple aperture laser scintillometer, and a thermal probe system that were used to calculate a path averaged and a point calculation of C_n~2. In addition, we present the results of the Plenoptic Sensor that was used to calculate a path averaged C_n~2 value. These measurements were conducted over a multi-day continuous test with supporting atmospheric and weather data provided by the University of Central Florida.
机译:大的温度梯度是强烈的大气湍流条件的已知来源。通常,在这些湍流条件强的地区,还伴有难以进行长期光学大气测试的条件。肯尼迪航天中心(KSC)的航天飞机着陆设施(SLF)提供了一个主要的测试环境,该环境能够产生强烈的大气湍流,并且也易于进行仪器良好的测试。航天飞机着陆设施具有一条5000 m长,91 m宽的混凝土跑道,为测量大气湍流提供了充足的空间,并为太阳加热地面时形成较大的温度梯度提供了机会。我们介绍了大孔径LED闪烁仪,三孔径激光闪烁仪和热探针系统的结果,这些结果用于计算平均路径和C_n〜2的点计算。此外,我们介绍了全光传感器的结果,该结果用于计算路径平均C_n〜2值。这些测量是在连续多天的连续测试中进行的,并由佛罗里达州中部大学提供了支持的大气和天气数据。

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