设为首页
加入收藏
Full Spectrum Inversion of Mountain-based GPS Occultation Data
-
摘要: 山基掩星观测是一种探测特定区域气象数据的新技术。该文从山基掩星探测技术的概念出发，阐述了山基掩星探测技术的特点和优势，介绍了山基掩星观测数据几何光学反演方法; 在详细介绍全谱反演技术的基础上，提出了采用全谱反演技术来处理山基掩星观测数据的新方法。采用该方法对2005年8月在河北兴隆雾灵山获取的山基掩星观测试验探测数据进行了处理，成功获得了大气折射率剖面, 将全谱反演结果与几何光学反演结果和同时获取的时空匹配的探空数据进行了比对分析。结果表明：全谱反演结果与几何光学反演结果平均相对偏差小于2%，全谱反演结果偏小，标准偏差低于3%；全谱反演结果与常规探空结果的平均相对偏差为8.15%，全谱反演结果偏小，标准偏差为1.4%。Abstract: Mountain-based GPS radio occultation sounding is an economic novel technique for monitoring temporal and spatial variations of regional lower atmospheric environments. The GPS receiver, which is on a mountain top with a downward looking perspective toward the earth's limb, can track any GPS satellite as it sets or rises behind the earth's limb, therefore it collects data at both negative and positive elevations to the receiver's local horizon. By combining both the negative and the positive elevations data, a high-resolution profile of refractivity below the height of the receiver and in some case extending to 1—2 km above the receiver can be obtained.An experiment of the mountain-based GPS radio occultation is conducted on the top of Mt Wuling during 1—29 August 2005. During the experiment, the radiosonde observation is taken at Xinglong County, which is about 30 km away to the southeast of the Mt Wuling. Mountain-based occultation data and radiosonde data are successfully obtained. The traditional Geometric OPtics (GOP) inversion method are described in details, and refractivity profiles below the GPS receiver are obtained from occultation data by this method. A novel Full Spectrum Inversion (FSI) is also applied for mountain-based occultation data, which can deal with the multi-path effects frequently occurring in the lower atmosphere, while the traditional method usually becomes inefficient here. FSI provides a simple and efficient tool for deriving the instantaneous frequencies of a signal composed of several narrow banded sub-signals. When certain criteria are fulfilled, FSI is capable of resolving the frequency variation of each signal component. Since FSI is based on the Fourier transform of the entire signal, the problem that different signals get to the GPS receiver at the same time in multi-path regions is thus solved. Refractivity profiles below the receiver are also obtained by FSI. The comparisons of the refractivity obtained from the same GPS radio occultation events indicate that with FSI method, the precision has been improved by 2%, and the standard deviation is less than 3%. The refractivity differences between FSI and radiosonde are also achieved in a time window of 1.5 h and azimuth angle window of 40°, the comparison results show that the mean refractivity relative deviation is-8.15% with a standard deviation of 1.4%. The results suggest that the FSI is an efficient inversion scheme for mountain-based GPS radio occultation data. In the future, further research will be carried out on how to improve the inversion precision, and use this method in space GPS radio occultation data.
-
图 2 几何光学反演法与全谱反演技术流程图
Fig. 2 Flow chart of Geometric OPtics (GOP) and Full Spectrum Inversion (FSI) methods
图 3 全谱反演结果与几何光学反演结果比对情况
Fig. 3 Comparison of the refractivity obtained from FSI and GOP
图 4 比对结果相对误差 (相对几何光学反演结果)
Fig. 4 Relative deviation (comparison to the results obtained from GOP)
-
[1] Meehan T K, Kursinski E R, Hajj G A, et al. Analysis of GPS signals occulted by the atmosphere as tracked from mauna Kea using the TurboRogue GPS receiver. Trans Am Geophys Union (EOS), 1991, 72:372. [2] Cinzia Z, Hajj G, Robert E K. A novel approach to atmospheric profiling with a mountainbased or airborn GPS receiver. J Geophys Res, 1999, 104(D20):24435-24447. doi: 10.1029/1999JD900766 [3] Mousa A T. Inversion Algorithm for GPS down Looking Occultation Data: Simulation Analysis.Japan Earth and Planetary Science Joint Meeting, Tokyo, 2002:27-31. [4] Aoyama Y, Shoji Y, Mousa A, et al. Down Looking GPS Occultation Measurement on the Top of Mt Fuji. Proceeding of International Workshop on GPS Meteorology. Tsukuba, Japan, 2003. [5] 张训械, 曾桢, 胡雄, 等.山基无线电掩星模拟.电波科学学报, 2004, 19(5):530-536. http://www.cnki.com.cn/Article/CJFDTOTAL-DBKX200405004.htm [6] 胡雄, 张训械, 吴小成, 等.山基GPS掩星观测实验及其反演原理.地球物理学报, 2006, 49(1):22-27. http://www.cnki.com.cn/Article/CJFDTOTAL-DQWX200601004.htm [7] 宫晓艳, 胡雄, 吴小成, 等.雾灵山GPS掩星观测试验分析.应用气象学报, 2008, 19(2):180-187. doi: 10.11898/1001-7313.20080233 [8] 吴小成, 胡雄, 宫晓艳, 等.山基GPS掩星折射率与探空折射率比较.地球物理学进展, 2008, 23(4):1149-1155. http://www.cnki.com.cn/Article/CJFDTOTAL-DQWJ200804021.htm [9] 范磊, 符养, 杜晓勇, 等.雾灵山山基掩星观测反演误差分析.武汉大学学报:信息科学版, 2008, 33(1):89-92. http://cpfd.cnki.com.cn/Article/CPFDTOTAL-ZGQX200811011005.htm [10] 孙学金, 赵世军, 余鹏. GPS掩星切点水平漂移规律的数值研究.应用气象学报, 2004, 15(2):174-180. http://qikan.camscma.cn/jams/ch/reader/view_abstract.aspx?file_no=20040222&flag=1 [11] 杜明斌, 杨引明, 丁金才. COSMIC反演精度和有关特性的检验.应用气象学报, 2009, 20(5):586-593. doi: 10.11898/1001-7313.20090510 [12] Jensen A S, Lohmann M S, Benzon H H, et al. Full spectrum inversion of radio occultation signals. Radio Sci, 2003, 38(3), doi: 10.1029/2002RS002763. [13] 胡雄, 曾桢, 张训械, 等.大气GPS掩星观测反演方法.地球物理学报, 2005, 48(4):768-774. http://www.cnki.com.cn/Article/CJFDTOTAL-DQWX200504005.htm [14] 肖卫华, 符养, 高太长, 等.利用折射指数推算大气纬圈平均风场方法.应用气象学报, 2011, 22(3):346-355. doi: 10.11898/1001-7313.20110311 [15] Born M, Wolf E. Principle of Optics. New York: Cambridge Univ Press, 1999. [16] 王名才.大气科学常用公式.北京:气象出版社, 1994. -
下载:
图(5)
计量
- 摘要浏览量: 4463
- HTML全文浏览量: 1052
- PDF下载量: 1602
- 被引次数: 0
