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

中低纬度Pc3-4地磁脉动特性研究——子午工程数据分析初步结果

张青梅 王赤 李晖 李传起

张青梅, 王赤, 李晖, 李传起. 中低纬度Pc3-4地磁脉动特性研究——子午工程数据分析初步结果[J]. 空间科学学报, 2013, 33(6): 608-616. doi: 10.11728/cjss2013.06.608
引用本文: 张青梅, 王赤, 李晖, 李传起. 中低纬度Pc3-4地磁脉动特性研究——子午工程数据分析初步结果[J]. 空间科学学报, 2013, 33(6): 608-616. doi: 10.11728/cjss2013.06.608
Zhang Qingmei, Wang Chi, Li Hui, Li Chuanqi. Characters of the Pc3-4 Magnetic Pulsations at Middle and Low Latitudes: Preliminary Geomagnetic Results From Chinese Meridian Project[J]. Journal of Space Science, 2013, 33(6): 608-616. doi: 10.11728/cjss2013.06.608
Citation: Zhang Qingmei, Wang Chi, Li Hui, Li Chuanqi. Characters of the Pc3-4 Magnetic Pulsations at Middle and Low Latitudes: Preliminary Geomagnetic Results From Chinese Meridian Project[J]. Journal of Space Science, 2013, 33(6): 608-616. doi: 10.11728/cjss2013.06.608

中低纬度Pc3-4地磁脉动特性研究——子午工程数据分析初步结果

doi: 10.11728/cjss2013.06.608
基金项目: 国家重点基础研究发展计划项目(2012CB825602);国家自然科学基金项目(41231067, 41204118)和国家重点实验室专项基金项目共同资助
详细信息
    作者简介:

    张青梅,E-mail:qmzhang@spaceweather.ac.cn

    通讯作者:

    王赤,E-mail:cw@spaceweather.ac.cn

  • 中图分类号: P353

Characters of the Pc3-4 Magnetic Pulsations at Middle and Low Latitudes: Preliminary Geomagnetic Results From Chinese Meridian Project

  • 摘要: 利用新建成的子午工程地磁台站数据,对比分析了地磁平静期间(2011年3月20-27日)和磁暴期间(2011年9月25日至10月1日)Pc3-4地磁脉动的时空分布特征及其对行星际条件的响应.数据分析结果表明,中低纬度(1.3<L<2.3,L为磁壳参数)的Pc3-4地磁脉动在这两个时期内的分布存在明显的晨昏不对称性,在昼侧前出现明显的Pc3-4地磁脉动并与行星际上游波动密切相关,其振幅增强可能与太阳风动压脉冲相关,高速太阳风更易导致Pc3-4地磁脉动;而对于近赤道低纬(L<1.3)区域,无论是在地磁平静期还是磁暴期均未能观测到Pc3-4地磁脉动,Pc3-4地磁脉动存在明显的纬度效应.

     

  • [1] Saito T. Magnetic pulsations[J]. Space Sci. Rev., 1969, 10:319
    [2] Orr D, Webb D C. Statistical studies of geomagnetic pulsations with periods between 10 and 70s and their relationship to the plasmapause region[J]. Planet. Space Sci., 1975, 23:1169
    [3] Ansari I A, Fraser B J. A multistation study of low latitude Pc3 geomagnetic pulsations[J]. Planet. Space Sci., 1986, 34:519
    [4] Cao M, Mcpherron R L, Russell C T. Statistical study of ULF wave occurrence in the dayside magnetosphere[J]. J. Geophys. Res., 1994, 99:8731
    [5] Obana Y, Yoshikawa A, Olsan J V, et al. North-south asymmetry of the amplitude of high-latitude Pc3-5 pulsations: Observations at conjugate stations[J]. J. Geophys. Res., 2005, 110:10214
    [6] Yumoto K. Generation and propagation mechanisms of low-latitude magnetic pulsations: A review[J]. J. Geophys. Res., 1986, 60:79-105
    [7] Kurchashov Y P, Nikomarov Y S, Pilipenko V A, et al. Field line resonance effects in local meridional structure of mid-latitude geomagnetic pulsations[J]. Ann. Geophys., 1987, 5A:147-154
    [8] Miletits C Z, Verö J, Stuart W. Dynamic spectra of pulsation events at L~1.9 and L~3.3[J]. J. Atmos. Terr. Phys., 1988, 50:649-656
    [9] Satio T. A new index of geomagnetic pulsation and its relation to solar M-regions[J]. Rept. Ionos. Space Res., 1964, 18:260-274
    [10] Bolshakova O V, Troitskaya V A. Relation between the direction of the interplanetary magnetic field and steady oscillation conditions[J]. Dokl. Akad. Nauk. SSSR, 1968, 180:343
    [11] Troitskaya V A, Plyasova-Bakunina T A, Guglielmi A V. Relationship between Pc2-4 pulsations and the interplanetary field[J]. Dokl. Akad. Nauk. SSSR, 1971, 197:1313
    [12] Troitskaya V A, Bolshakova O V. Diagnostics of the magnetosphere using multipoint measurements of ULF-waves[J]. Adv. Space Res., 1988, 8:413-425
    [13] Greenstadt E W, Olson J V. Pc3,4 activity and interplanetary field orientation[J]. J. Geophys. Res., 1976, 81:5911-5920
    [14] Russell C T, Luhmann J G, Odera T J, et al. The rate of occurrence of dayside Pc3,4 pulsations: the L-value dependence of the IMF cone angle effect[J]. Geophys. Res. Lett., 1983, 10:663-666
    [15] Takahashi K, McPherron R L, Terasawa T. Dependence of the spectrum of Pc3-4 pulsations on the interplanetary magnetic field[J]. J. Geophys. Res., 1984, 89:2770-2780
    [16] Miyake W, Mukai T, Yumoto K, Saito T, Hirao K. A correlation study between the solar wind speed observed by Suisei and the amplitude of Pc3 geomagnetic pulsations[J]. J. Geomag. Geoelectr., 1987, 39:159-164
    [17] Yedidia B A, Vellante M, Villante U, et al. A study of the relationship between micropulsations and solar wind properties[J]. J. Geophys. Res., 1991, 96:3465-3470
    [18] Wolfe A. Dependence of mid-latitude hydromagnetic energy spectra on solar wind speed and interplanetary magnetic field direction[J]. J. Geophys. Res., 1980, 85:5977-5982
    [19] Wolfe A, Meloni A. ULF geomagnetic power near L=4, 6. Relationship to upstream solar wind quantities[J]. J. Geophys. Res., 1981, 86:7507-7512
    [20] Verö J. Determination of the solar wind velocity from pulsa\-tion indices[J]. J. Atmos. Terr. Phys., 1975, 37:561-564
    [21] Chi P, Russell C, Bloom R, Singer H. Solar wind control of ultra low-frequency wave activity at L=3[J]. J. Geophys. Res., 1998, 103:29467-29477
    [22] Chugunova O M, Pilipenko V A, Engebretson M, Rodger A. Statistical relations between the probability of occurrence of Pc3-4 pulsations at high latitudes in the Antarctic regions and the solar wind and IMF parameters[J]. Geomag. Aeron., 2007, 47:205-215
    [23] Le G, Chi P J, Goedecke W, et al. Magnetosphere on May 11, 1999, the day the solar wind almost disappeared: II. Magnetic pulsations in space and on the ground[J]. Geophys. Res. Lett., 2000, 27:2165-2168
    [24] Le G, Russell C T, Petrinec S M. Magnetosphere on May 11, 1999, the day the solar wind almost disappeared: I. Current systems[J]. Geophys. Res. Lett., 2000, 27:1827-1830
    [25] Zanandrea A, DaCosta J M, Dutra S L G, et al. Pc3-4 geomagnetic pulsations at very low latitude in Brazil[J]. Planet. Space Sci., 2004, 52:1209-1215
    [26] Villante U, Vellante M, Francia P, et al. ULF fluctuations of the geomagnetic field and ionospheric sounding measurements at low latitudes during the first CAWSES campaign[J]. Ann. Geophys., 2006, 24:1455-1468
    [27] De Lauretis M, Francia P, Regi M, et al. Pc3 pulsations in the polar cap and at low latitude[J]. J. Geophys. Res., 2010, 115, A11223, doi: 10.1029/2010JA015967
    [28] Heilig B, Lotz S, Verö J, et al. Empirically modelled Pc3 activity based on solar wind parameters[J]. Ann. Geophys., 2010, 28:1703-1722
    [29] Villante U, DePaulis C, Francia P. The transmission of upstream waves to the magnetosphere: An analysis at widely separated ground stations[J]. J. Geophys. Res., 2011, 116, A06219, doi: 10.1029/2010JA016263
    [30] Zong Q G, Zhou X Z, Wang Y F, et al. Energetic electron response to ULF waves induced by interplanetary shocks in the outer radiation belt[J]. J. Geophys. Res., 2009, 114(A10):A10204, doi: 10.1029/2009JA014393
    [31] Zhang X Y, Zong Q G, Wang Y F, et al. ULF waves excited by negative/positive solar wind dynamic pressure impulses at geosynchronous orbit[J]. J. Geophys. Res., 2010, 115(A10):A10221, doi: 10.1029/2009JA015016
    [32] Wang C. New chains of space weather monitoring stations in China[J]. Space Weather, 2010, 8, S08001, doi: 10.1029/2010SW000603
    [33] Greenstadt E W, Olson J V, Loewen P D, et al. Correlation of Pc3, 4, and 5 activity with solar wind speed[J]. J. Geophys. Res., 1979, 84:6694-6696
    [34] Greenstadt E W, Olson J V. Geomagnetic pulsation signals and hourly distribution of IMF orientation[J]. J. Geophys. Res., 1979, 84:1493-1498
    [35] Greenstadt E W. Field-determined oscillations in the magnetosheath as possible source of medium-period, daytime micropulsations[C]//Proceedings of the Conference on Solar Terrestrial Relations. Calgary Alta: University of Calgary, 1973. 515
  • 加载中
计量
  • 文章访问数:  900
  • HTML全文浏览量:  1
  • PDF下载量:  1801
  • 被引次数: 0
出版历程
  • 收稿日期:  2013-01-10
  • 修回日期:  2013-03-18
  • 刊出日期:  2013-11-15

目录

    /

    返回文章
    返回