Gong Xiaoyan, Hu Xiong, Wu Xiaocheng, et al. Mountain-based GPS occultation observation experiment at Mt Wuling. J Appl Meteor Sci, 2008, 19(2): 180-187.
Citation: Gong Xiaoyan, Hu Xiong, Wu Xiaocheng, et al. Mountain-based GPS occultation observation experiment at Mt Wuling. J Appl Meteor Sci, 2008, 19(2): 180-187.

Mountain-based GPS Occultation Observation Experiment at Mt Wuling

  • Received Date: 2007-04-06
  • Rev Recd Date: 2007-09-24
  • Publish Date: 2008-04-30
  • Mountain-based GPS occultation technique is referred to as receiving the radio signals of GPS satellites with very low elevations and negative elevations using a GPS receiver at the top of high mountain and retrieving the lower atmospheric refractivity profiles. A mountain-based GPS occultation observation experiment is performed at Mt Wuling (40.60°N, 117.48°E, 2118 m) in Hebei Province during August 1—29, 2005. The campaign is organized by China Meteorological Administration, a few other organizations participate in the experiment. Totally 576-hour raw observation data are collected by JAVAD two-frequency GPS receiver provided by Center for Space Science and Applied Research, Chinese Academy of Sciences, and 1136 occultation events are recorded. Out of the total occultation events, 621 are rising occultation events and 515 are setting occultation ones. There are about 2 occultation events observed in one hour on average. Detailed statistics and analyses are made to show features of all the observed occultation events, such as the distribution of the occurring time, the duration, minimum elevations and azimuth. The results are as follows. The distribution of the occurring time of the observed mountain-based occultation events is nearly random uniform, and it seems that there are more observed occultation events for two periods of time, one is from 20:00 (local time) to 22:00, and the other is from 04:00 to 06:00. The duration of most occultation events is from 15 minutes to 20 minutes, and about 18 minutes on average. The range of azimuth of observed occultation events is between 110° and 290°, the peak of the distribution of azimuth is between 180° and 195°. These features are related to some important factors, such as the distribution of GPS satellites' orbits, the location of GPS receiver and the direction which the antenna points to. The minimum elevations of most occultation events are between -3° and -2.5°, the lowest negative elevations of all the events is -4.994° from south direction, which is possibly resulted from the landform around the observation station. The minimum elevations of setting occultation events are lower than that of rising occultation events obviously. It shows that the ability to track rising occultation events of commercial GPS receiver is weak. If the same GPS satellite is occulted, it is occulted mostly from the same azimuth, and their occurring time is close (their differences are usually less than two hour). This is determined by distribution of GPS satellites' orbits, cycle and features of movement. A new effective method is provided by mountain-based occultation observations for monitoring lower atmospheric environment. This emerging technique has potential applications. Above are the first statistic and analytic results from observed data by which reference can be provided for mountain-based occultation observation's operation application.
  • Fig. 1  Scheme of mountain-based radio occultation observations

    Fig. 2  Histogram of the predicted mountain-based occultation events occurring azimuth angles

    Fig. 3  Plot of the observed mountain-based occultation events occuring time and observing days (a) histogram of the observed mountain-based occultation events' occurring time, (b) the curve of observing days for each hour

    Fig. 4  Histogram of the observed mountain-based occultation events' duration

    Fig. 5  Histogram of the observed mountain-based occultation events minimum elevation (a) hisgogram of the obseved mountain-based occultation events minimum elevation, (b) histogram of the rising and setting occultation events minimun elevation

    Fig. 6  Scatter dot plot of minimum elevations versus azimuth angles

    Fig. 7  Histogram of the observed mountain-based occultation events occurring azimuth angles

    Fig. 8  Scatter dot plot of occurring times (a) and GPS occultation number versus azimuth angles (b)

    Table  1  The number of observed mountain-based occultation events during August 1—29, 2005

  • [1]
    Hajj G A, Romans L J. Ionospheric electron density profiles obtained with the global positioning system:Results from the GPS/MET Experiment. Radio Sciences, 1998, 33(1):175-190. doi:  10.1029/97RS03183
    [2]
    Rius A, Ruffini G, Romeo A. Analysis of ionospheric electron density distribution from GPS/MET occultations. IEEE Trans, Geoscience and Remote Sensing, 1998, 36(2):383-394. doi:  10.1109/36.662724
    [3]
    Ware R, Exner M, Feng D, et al. GPS sounding of the atmosphere from low earth orbit:Preliminary results. Bull Am Meteorol Soc, 1996, 77:19-40. doi:  10.1175/1520-0477(1996)077<0019:GSOTAF>2.0.CO;2
    [4]
    Rocken C, Kuo Y H, Schreiner W, et al. COSMIC system description. TAO, 2000, 11(1):21-52. https://www.researchgate.net/publication/234422312_COSMIC_system_description
    [5]
    Kursinski E R, Hajj G A, Schofield J T, et al. Observing earth's atmosphere with radio occultation measurements using the Global Positioning System. J Geophys Res, 1997, 102(D19):23429-23465. doi:  10.1029/97JD01569
    [6]
    Rocken C, Anthes R, Exner M, et al. Analysis and validation of GPS/MET data in the neutral atmosphere. J Geophys Res, 1997, 102(D25):29849-29866. doi:  10.1029/97JD02400
    [7]
    Zuffada C, Hajj G, Kursinski E R. A novel approach to atmospheric profiling with a montain-based or airborne GPS receiver. J Geophys Res, 1999, 104(D20):24435-24447. doi:  10.1029/1999JD900766
    [8]
    Aoyama Y, Shoji Y. Mountain top and Airborne GPS Observations, and Effects of Turbulence on RO Signals. Colloquium on Atmospheric Remote Sensing Using the Global Positioning System, Boulder, Colorado, June 20—July 2, 2004.
    [9]
    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
    [10]
    曾桢.地球大气GPS无线电掩星观测技术研究.武汉:中国科学院研究生院, 2003.
    [11]
    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
    [12]
    何平, 徐宝祥, 周秀骥, 等.地基GPS反演大气水汽含量的初步试验.应用气象学报, 2002, 13(2):179-183. http://qikan.camscma.cn/jams/ch/reader/view_abstract.aspx?file_no=20020222&flag=1
    [13]
    谢璞, 张朝林, 王迎春, 等.北京地区单双频地基GPS大气水汽遥测试验与研究.应用气象学报, 2006, 17(增刊):28-33. http://www.cnki.com.cn/Article/CJFDTOTAL-YYQX2006S1003.htm
    [14]
    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
    [15]
    严豪健, 郭鹏, 张贵霞, 等.上海天文台GPS掩星技术研究现状.中国科学院上海天文台年刊, 2003, 24:39-47. http://www.cnki.com.cn/Article/CJFDTOTAL-KXTW200300005.htm
  • 加载中
  • -->

Catalog

    Figures(8)  / Tables(1)

    Article views (4081) PDF downloads(1265) Cited by()
    • Received : 2007-04-06
    • Accepted : 2007-09-24
    • Published : 2008-04-30

    /

    DownLoad:  Full-Size Img  PowerPoint