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Analysis of the Influence of the Superrefraction Effect on the Earth's Neutral Atmospheric Parameters Retrieval

机译:超折射效应对地球中性大气参数反演的影响分析

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The superrefraction, which can be frequently found in the moist lower troposphere, degrades the accuracy of the retrieved atmospheric parameters from GPS/LEO occultation data. The GPS/LEO occupation data containing superrefraction effect can be simulated by using multiple phase screens technique, with the refractivity model or high resolution ecmPrf profile (echPrf data). Simulation results show that superrefraction effect can lead to refractivity error in the moist lower troposphere, which in some case can be as large as about -9.6%. About 24530 echPrf profiles from DOY(day of year) 151 to DOY 161 in 2007, are divided into A, B, C, D 4 categories. According to the minimum of refractivity gradient of the echPrf data, the minimum of the refractivity gradient of the echPrf data is decreasing from category A to category D. The category C and category D contain the occultation profiles with the superrefraction effect. The refractivity profiles in 4 categories are compared with those of the corresponding COSMIC(Constellation Observing System for Meteorology, Ionosphere and Climate) data. Statistical comparison results show: about 5.6% of the echPrf profiles with superrefraction effect can be found. The mean and standard deviation of the fractional difference of refractivity between COSMIC observation and echPrf data near the ground are about -0.51% and 2.71% for set A, -1.64% and 4.27% for set B, -3.59% and 5.49% for set C, -8.50% and 7.21% for set D. The locations of the superrefraction phenomenon in the tropics are mainly near the following regions: North America (Mexico), South America (the western coast of Peru), North Africa (the Sahara desert), and South Africa on the Atlantic side.
机译:通常在潮湿的对流层低层中发现的超折射降低了从GPS / LEO掩星数据中检索到的大气参数的准确性。包含超折射效应的GPS / LEO占领数据可以使用折射率模型或高分辨率ecmPrf剖面(echPrf数据),通过使用多相屏蔽技术进行模拟。仿真结果表明,超折射效应会导致在较低的对流层低层产生折射率误差,在某些情况下,折射率误差可能高达-9.6%。从DOY(每年的日期)151到2007年的DOY 161大约有24530个echPrf配置文件,分为A,B,C,D 4类。根据echPrf数据的最小折射率梯度,echPrf数据的最小折射率梯度从类别A减小到类别D。类别C和类别D包含具有超折射作用的掩星剖面。将4个类别的折射率分布与相应的COSMIC(气象,电离层和气候星座观测系统)数据的折射率分布进行比较。统计比较结果表明:可以发现约5.6%的echPrf轮廓具有超折射效果。 COSMIC观测值与地面附近的echPrf数据之间的折光率分数差异的平均值和标准偏差对于A组约为-0.51%和2.71%,对于B组约为-1.64%和4.27%,对于B组为-3.59%和5.49% C,对于D组,为-8.50%和7.21%。热带地区的超折射现象的位置主要位于以下地区:北美洲(墨西哥),南美洲(秘鲁的西海岸),北非(撒哈拉沙漠) ),以及在大西洋沿岸的南非。

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