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风云三号C星GNOS北斗掩星电离层探测初步结果

杨光林 孙越强 白伟华 张效信 杨忠东 张鹏 谭广远

杨光林, 孙越强, 白伟华, 张效信, 杨忠东, 张鹏, 谭广远. 风云三号C星GNOS北斗掩星电离层探测初步结果[J]. 空间科学学报, 2019, 39(1): 36-45. doi: 10.11728/cjss2019.01.036
引用本文: 杨光林, 孙越强, 白伟华, 张效信, 杨忠东, 张鹏, 谭广远. 风云三号C星GNOS北斗掩星电离层探测初步结果[J]. 空间科学学报, 2019, 39(1): 36-45. doi: 10.11728/cjss2019.01.036
YANG Guanglin, SUN Yueqiang, BAI Weihua, ZHANG Xiaoxin, YANG Zhongdong, ZHANG Peng, TAN Guangyuan. Beidou Navigation Satellite System Sounding of the Ionosphere from FY-3C GNOS:Preliminary Results[J]. Journal of Space Science, 2019, 39(1): 36-45. doi: 10.11728/cjss2019.01.036
Citation: YANG Guanglin, SUN Yueqiang, BAI Weihua, ZHANG Xiaoxin, YANG Zhongdong, ZHANG Peng, TAN Guangyuan. Beidou Navigation Satellite System Sounding of the Ionosphere from FY-3C GNOS:Preliminary Results[J]. Journal of Space Science, 2019, 39(1): 36-45. doi: 10.11728/cjss2019.01.036

风云三号C星GNOS北斗掩星电离层探测初步结果

doi: 10.11728/cjss2019.01.036
基金项目: 

国家自然科学基金项目(41405039, 41405040, 41505030, 41606206, 41775034),中国科学院空间先导专项(XDA15007501),中国科学院科研装备研制项目(YZ201129),国家重点研发计划重点专项项目(2017YB0502800, 2017YFB0502802),公益性行业(气象)科研专项基金(GYHY201006048, GYHY201306063)共同资助

详细信息
    作者简介:

    杨光林,yglyang@cma.gov.cn

    通讯作者:

    白伟华,bjbwh@163.com

  • 中图分类号: P352

Beidou Navigation Satellite System Sounding of the Ionosphere from FY-3C GNOS:Preliminary Results

  • 摘要: 利用风云三号卫星C星GNOS掩星探测仪电离层数据,分析了2013年10月FY-3C GNOS探测的北斗掩星电离层廓线分布,将2013年10月1日至2015年10月10日期间FY-3C GNOS观测的F2层峰值电子密度(NmF2)与地面电离层测高仪观测结果进行对比,验证了FY-3C GNOS北斗电离层掩星的探测精度.结果表明,FY3-C GNOS北斗电离层掩星与电离层测高仪探测的NmF2数据相关系数为0.96,平均偏差为10.21%,标准差为19.61%.在不同情况下其数据精度有如下特征:白天精度高于夜晚;夏季精度高于分季,分季精度高于冬季;中纬地区精度高于低纬地区,低纬地区精度高于高纬地区; BDS倾斜同步轨道(IGSO)卫星精度高于同步轨道(GEO)卫星和中轨道(MEO)卫星.FY-3C GNOS北斗电离层掩星与国际上其他掩星电离层数据精度的一致性对GNSS掩星探测资料的综合利用具有重大意义.

     

  • [1] LIU J Y, TSAI Y B, MA K F, et al. Ionospheric GPS Total Electron Content (TEC) disturbances triggered by the 26 December 2004 Indian Ocean tsunami[J]. J. Geophys. Res.:Space Phys., 2006, 111(A5):698-704
    [2] LIU J Y, CHEN C H, LIN C H, et al. Ionospheric disturbances triggered by the 11 March 2011 M9.0 Tohoku earthquake[J]. J. Geophys. Res. Space Phys., 2011, 116(A6):97-108
    [3] WAN W X, LIU L, YUAN H, et al. The GPS measured SITEC caused by the very intense solar flare on July 14, 2000[J]. Adv. Space Res., 2005, 36(12):2465-2469
    [4] DING F, WAN W, LIU L, et al. A statistical study of large-scale traveling ionospheric disturbances observed by GPS TEC during major magnetic storms over the years 2003-2005[J]. J. Geophys. Res.:Space Phys., 2008, 113 (A3):A00A01. DOI: 10.1029/2008JA013037
    [5] PAVELYEV A G, LIOU Y A, WICKERT J, et al. Effects of the ionosphere and solar activity on radio occultation signals:Application to CHAllenging Minisatellite Payload satellite observations[J]. J. Geophys. Res.:Space Phys., 2007, 112(A6):49-60
    [6] LIU L, ZHAO B Q, WAN W X, et al. Seasonal variations of the ionospheric electron densities retrieved from Constellation Observing System for Meteorology, Ionosphere, and Climate mission radio occultation measurements[J]. J. Geophys. Res.:Space Phys., 2009, 114(A2). DOI: 10.1029/2008ja013819
    [7] YUE X, SCHREINER W S, LEI J, et al. Climatology of ionospheric upper transition height derived from COSMIC satellites during the solar minimum of 2008[J]. J. Atmos. Solar-Terr. Phys., 2010, 72(17):1270-1274
    [8] YUE X, SCHREINER W S, KUO Y, et al. Global 3D ionospheric electron density reanalysis based on multisource data assimilation[J]. J. Geophys. Res.:Space Phys., 2012, 117(A9):667-672
    [9] YUE X A, SCHREINER W S, KUO Y H. A feasibility study of the radio occultation electron density retrieval aided by a global ionospheric data assimilation model[J]. J. Geophys. Res.:Space Phys., 2012, 117(A8):648-659
    [10] 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]. J. Geophys. Res. Atmos., 1997, 102(D19):23429-23465
    [11] ROCKEN C, ANTHES R, EXNER M, et al. Analysis and validation of GPS/MET data in the neutral atmosphere[J]. J. Geophys. Res. Atmos., 1997, 102(D25):29849-29866
    [12] WARE R, ROCKEN C, SOLHEIM F, et al. GPS sounding of the atmosphere from low earth orbit:preliminary results[J]. Bull. Ame. Meteor. Soc., 1996, 77(1):19-40
    [13] WICKERT J, SCHMIDT T, BEYERLE G, et al. The radio occultation experiment aboard CHAMP:Operational data analysis and validation of vertical atmospheric profiles[J]. J. Meteor. Soc. Japan. Ser. Ⅱ, 2004, 82(1B):381-395
    [14] WICKERT J, BEYERLE G, KÖNIG R, et al. GPS radio occultation with CHAMP and GRACE:A first look at a new and promising satellite configuration for global atmospheric sounding[J]. Ann. Geophys., 2005, 23(3):653-658
    [15] ANTHES R A, ROCKEN C, KUO Y H. Applications of COSMIC to Meteorology and Climate[J]. Terr. Atmos. Ocean. Sci., 2000, 11(1):115-156
    [16] ANTHES R A, BERNHARDT P A, CHEN Y, et al. The COSMIC/FORMOSAT-3 Mission:Early Results[J]. Bull. Am. Meteor. Soc., 2008, 89(3):313-333
    [17] BAI W H, SUN Y Q, DU Q F, et al. An introduction to the FY3 GNOS instrument and mountain-top tests[J]. Atmos. Meas. Techn., 2014, 7(6):1817-1823
    [18] HAJJ G A, ROMANS L J. Ionospheric electron density profiles obtained with the Global Positioning System:Results from the GPS/MET experiment[J]. Radio Sci., 1998, 33(1):175-190
    [19] LEI J, SYNDERGAARD S, BURNS A G, et al. Comparison of COSMIC ionospheric measurements with ground-based observations and model predictions:Preliminary results[J]. J. Geophys. Res., 2007, 112(A7):601-623
    [20] KELLEY M C, WONG V K, APONTE N, et al. Comparison of COSMIC occultation-based electron density profiles and TIP observations with Arecibo incoherent scatter radar data[J]. Radio Sci., 2009, 44(4):1-13
    [21] LIU J Y, LEE C C, YANG J Y, et al. Electron density profiles in the equatorial ionosphere observed by the FORMOSAT-3/COSMIC and a digisonde at Jicamarca[J]. GPS Solut., 2010, 14(1):75-81
    [22] KRANKOWSKI A, ZAKHARENKOVA I, KRYPIAK-GREGORCZYK A, et al. Ionospheric electron density observed by FORMOSAT-3/COSMIC over the European region and validated by ionosonde data[J]. J. Geod., 2011, 85(12):949-964
    [23] CHUO Y J, LEE C C, CHEN W S, et al. Comparison between bottomside ionospheric profile parameters retrieved from FORMOSAT3 measurements and ground-based observations collected at Jicamarca[J]. J. Atmos. Solar-Terr. Phys., 2011, 73(13):1665-1673
    [24] ELY C V, BATISTA I S, ABDU M A. Radio occultation electron density profiles from the FORMOSAT-3/COSMIC satellites over the Brazilian region:a comparison with Digisonde data[J]. Adv. Space Res., 2012, 49(11):1553-1562
    [25] SAHAI Y, JESUS R D, FAGUNDES P R, et al. Effects observed in the equatorial and low latitude ionospheric F-region in the Brazilian sector during low solar activity geomagnetic storms and comparison with the COSMIC measurements[J]. Adv. Space Res., 2012, 50(10):1344-1351
    [26] SUN Lingfeng, ZHAO Biqiang, YUE Xin'an, et al. Comparison between ionospheric character parameters retrieved from FORMOSAT3 measurement and ionosonde observation over China[J]. Chin. J. Geophys., 2014, 57 (11):3625-3632(孙凌峰, 赵必强, 乐新安, 等. 中国区域电离层垂测仪探测参量与COSMIC掩星反演结果比较研究[J]. 地球物理学报, 57(11):3625-3632)
    [27] HU L H, NING B Q, LIU L B, et al. Comparison between ionospheric peak parameters retrieved from COSMIC measurement and ionosonde observation over Sanya[J]. Adv. Space Res., 2014, 54(6):929-938
    [28] REINISCH B W, GALKIN I A. Global Ionospheric Radio Observatory (GIRO)[J]. Earth Planets Space, 2011, 63(4):377-381
    [29] JAKOWSKI N, WEHRENPFENNIG A, HEISE S, et al. GPS radio occultation measurements of the ionosphere from CHAMP:Early results[J]. Geophys. Res. Lett., 2002, 29(10). DOI: 10.1029/2001gl014364
    [30] LIMBERGER M, HERNÁNDEZ-PAJARES M, ARAGÓN-ÁNGEL A, et al. Long-term comparison of the ionospheric F2 layer electron density peak derived from ionosonde data and Formosat-3/COSMIC occultations[J]. J. Space Weather Space Climate, 2015, 5:A21. DOI: 10.1051/swsc/2015023
    [31] YANG G L, SUN Y Q, BAI W H, et al. Validation results of NmF2 and hmF2 derived from ionospheric density profiles of GNOS on FY-3C Satellite[J]. Sci. China:Technol. Sci., 2017, 61(9):1372-1383
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出版历程
  • 收稿日期:  2017-12-11
  • 修回日期:  2018-05-28
  • 刊出日期:  2019-01-15

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