留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名
邮箱
手机号码
标题
留言内容
验证码

一种改进的Kp指数现报模式

王庚 罗冰显 刘四清 龚建村

王庚, 罗冰显, 刘四清, 龚建村. 一种改进的Kp指数现报模式[J]. 空间科学学报, 2016, 36(2): 153-166. doi: 10.11728/cjss2016.02.153
引用本文: 王庚, 罗冰显, 刘四清, 龚建村. 一种改进的Kp指数现报模式[J]. 空间科学学报, 2016, 36(2): 153-166. doi: 10.11728/cjss2016.02.153
WANG Geng, LUO Bingxian, LIU Siqing, GONG Jiancun. An Improved Algorithm for Nowcast of Kp Index[J]. Chinese Journal of Space Science, 2016, 36(2): 153-166. doi: 10.11728/cjss2016.02.153
Citation: WANG Geng, LUO Bingxian, LIU Siqing, GONG Jiancun. An Improved Algorithm for Nowcast of Kp Index[J]. Chinese Journal of Space Science, 2016, 36(2): 153-166. doi: 10.11728/cjss2016.02.153

一种改进的Kp指数现报模式

doi: 10.11728/cjss2016.02.153 cstr: 32142.14.cjss2016.02.153
基金项目: 国家自然科学基金项目(41474164)和国家重点基础研究计划项目(2012CB825606,2011CB811406)共同资助
详细信息
    通讯作者:
    • 王庚,E-mail:wanggengayst@163.com
  • 中图分类号: P353

An Improved Algorithm for Nowcast of Kp Index

  • 摘要: 在评估国际常用Kp指数现报模式Takahashi及其应用于中国地 磁台站效果的基础上, 提出了一种改进的地磁Kp指数现报模式, 其可以 有效识别地磁规则日变化的逐日变化特性, 反映地磁扰动的季节效应和地方时 效应, 从而提升了Kp指数现报的准确性. 采用Takahashi模式开发时所 使用的台站数据进行对比, 新模式将单站地磁Kp指数现报效率由0.77 提升至0.84, 多站联合Kp指数现报效率由0.88提升至0.92; 采用 2000-2006年北京十三陵台站(BMT, 磁纬29°N)数据进 行评估, Kp指数现报效率由0.70提升至0.80. 对Kp指数现 报结果的误差分析发现, 现报误差存在明显的地方时差异和一定的季节差异, 误差随扰动强度变化并在中强磁扰时最大. 利用SuperMAG的指数分析表明, Kp台站的经度不均匀分布会对现报效果造成一定影响.

     

  • [1] BARTELS J. The Standardized Index, Ks, and the Planetary Index, Kp[M]. Paris: IUGG Publication Office, 1949
    [2] BARTELS J, HECK N H, JOHNSTON H F. The three-hour-range index measuring geomagnetic activity[J]. Terr. Mag. Atmos. Elec., 1939, 44(4):411-454
    [3] THOMSEN M F. Why Kp is such a good measure of magnetospheric convection[J]. Space Weather, 2004, 2, S11004
    [4] GUSSENHOVEN M S, HARDY D A, HEINEMANN N. Systematics of the equatorward diffuse auroral boundary[J]. J. Geophys. Res., 1983, 88(7):5692-5708
    [5] MCILWAIN C E. Plasma convection in the vicinity of the geosynchronous orbit[M]//Earth's Magnetospheric Processes. Netherlands: Springer, 1972:268-279
    [6] FRIEDEL R H W, KORTH H, HENDERSON M G, et al. Plasma sheet access to the inner magnetosphere[J]. J. Geophys. Res., 2001, 106(4):5845-5858
    [7] CAUFFMAN D P, GURNETT D A. Double-probe measurements of convection electric fields with the Injun-5 satellite[J]. J. Geophys. Res., 1971, 76(25):6014-6027
    [8] ROWLAND D E, WYGANT J R. Dependence of the large-scale, inner magnetospheric electric field on geomagnetic activity[J]. J. Geophys. Res., 1998, 103(A7):14959-14964
    [9] BINSACK J H. Plasmapause observations with the MIT experiment on IMP 2[J]. J. Geophys. Res., 1967, 72(21): 5231-5237
    [10] CARPENTER D L, PARK C G. On what ionospheric workers should know about the plasmapause-plasmasphere[J]. Rev. Geophys., 1973, 11(1):133-154
    [11] HEPPNER J P. High latitude electric fields and the modulations related to interplanetary magnetic field parameters[J]. Radio Sci., 1973, 8(11):933-948
    [12] ALCAYDE D, CAUDAL G, FONTANARI J. Convection electric fields and electrostatic potential over 61°<< 72° invariant latitude observed with the European Incoherent Scatter Facility: 1. Initial results[J]. J. Geophys. Res., 1986, 91(1):233-247
    [13] Wing S, Johnson J R, Jen J, et al. Kp forecast models[J]. J. Geophys. Res., 2005, 110, A04203
    [14] BOBERG F, WINTOFT P, LUNDSTEDT H. Real time Kp prediction from solar wind data using neural networks [J]. Phys. Chem. Earth., 2000, 25(4):275-280
    [15] BALA R, REIFF P H, LANDIVAR J E. Real-time prediction of magnetosphere activity using the Boyle index[J]. Space Weather, 2009, 7, S04003
    [16] Takahashi K, Toth B A, Olson J V. An automated procedure for near-real-time Kp estimates[J]. J. Geophys. Res., 2001, 106(A10):21017-21032
    [17] MENVIELLE M, PAPITASHVILI N, HÄKKINEN L, et al. Computer production of K indices: review and comparison of methods[J]. Geophys. J. Intern., 1995, 123(3): 866-886
    [18] CHAPMAN S, BARTELS J. Geomagnetism[M]. London: Oxford University Press, 1940
    [19] MAYAUD P N. Atlas of Indices K[M]. Paris: IUGG Publication Office, 1967
    [20] XU Wenyao. Day-to-day variability of the Sq dynamo currents and Sq index[J]. Chin. J. Geophys., 1992, 35(6): 676-684 (徐文耀. Sq发电机电流的逐日变化和Sq指数[J]. 地球物理学报, 1992, 35(6):676-683)
    [21] KIRCHHOFF V W J H, CARPENTER L A. The day-to-day variability in ionospheric electric fields and currents[J]. J. Geophys. Res., 1976, 81(16):2737-2742
    [22] WU Yingyan, XU Wenyao, CHEN Gengxiong. Analysis of the periodical characteristics of Sq index[J]. Chin. J. Geophys., 2012, 55(3):953-959 (吴迎燕, 徐文耀, 陈耿雄. Sq指数的周期变化分析[J]. 地球物理学报, 2012, 55(3):953-959)
    [23] OLSON W P. Introduction to the topology of magnetospheric current systems[J]. Geophys. Monogr. Ser., 1984, 28:49-62
    [24] TAKEDA M. Day-to-day variation of equivalent Sq current system during March 11-16, 1970[J]. J. Geomagn. Geoelec., 1984, 36(5):215-228
    [25] XU W Y. Effects of the magnetospheric currents on the Sq-field and a new magnetic index characterizing Sq dynamo current intensity[J]. J. Geomagn. Geoelec., 1992, 44(3):449-458
    [26] GJERLOEV J W. The SuperMAG data processing technique[J]. J. Geophys. Res., 2012, 117, A09213
    [27] YANG M L, LIU C M, YE D H. Preliminary study of computing K index with FMI method[J]. Seismol. Geom. Obs. Res., 2004, 25(2):55-61(杨马陵, 刘昌谋, 叶东华. FMI方法计算地磁K指数的初步研究[J]. 地震地磁观测与研究, 2004, 25(2):55-61)
    [28] BITTERLY M, MENVIELLE M, BITTERLY J, et al. A comparison between computer derived (FMI method) and hand-scaled K indices at Port Aux Francis and Port Alfred French observatories[C]//Proceeding of the International Workshop on Geomagnetic Instrument, Data Acquisition and Processing. Bruxelles: Académie Royale de Belgique, 1997:136-143
    [29] PIRJOLA R, RYNO J, SUCKSDORFF C. Computer production of K-indices by a simple method based on linear elimination[C]//Proceeding of the International Workshop on Geomagnetic Observatory Data Acquisition and Processing, 1990:136-146
    [30] SUCKSDORFF C, PIRJOLA R, HÄKKINEN L. Computer production of K-values based on linear elimination[J]. Geophys. Trans., 1991, 36:333-345
    [31] BAKER D N, KLIMAS A J, MCPHERRON R L, et al. The evolution from weak to strong geomagnetic activity: An interpretation in terms of deterministic chaos[J]. Geophys. Res. Lett., 1990, 17(1):41-44
    [32] SVALGAARD L. Recalibration of Bartels' geomagnetic activity indices Kp and ap to include universal time variations[J]. J. Geophys. Res., 1976, 81(28):5182-5188
    [33] NEWELL P T, GJERLOEV J W. Evaluation of SuperMAG auroral electrojet indices as indicators of substorms and auroral power[J]. J. Geophys. Res., 2011, 116, A12211
    [34] NEWELL P T, GJERLOEV J W. SuperMAG-based partial ring current indices[J]. J. Geophys. Res., 2012, 117, A05215
  • 加载中
计量
  • 文章访问数:  2664
  • HTML全文浏览量:  359
  • PDF下载量:  1335
  • 被引次数: 

    0(来源:Crossref)

    0(来源:其他)

出版历程
  • 收稿日期:  2015-02-10
  • 修回日期:  2015-09-01
  • 刊出日期:  2016-03-15

目录

    /

    返回文章
    返回