Relationship between the geomagnetic Dst(min) and the interplanetary Bz(min) during cycle 23

被引:13
|
作者
Kane, R. P. [1 ]
机构
[1] Inst Nacl Pesquisas Espaciais, BR-12245970 Sao Jose Dos Campos, SP, Brazil
关键词
Geomagnetic storms; Dst; Interplanetary magnetic fields; Sun-Earth relationship; SOLAR-WIND; RING CURRENT; MAGNETIC STORM; MAGNETOSPHERE; INTENSE; SPACE; SIGNATURES; PARTICLES; PRESSURE; EARTH;
D O I
10.1016/j.pss.2009.11.005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In cycle 23 for geomagnetic storms of -Dst(min) > 50 nT, the plot of -Dst(min) versus -Bz(min) for the low -Bz(min) range 0-10 nT showed erratic variation in Dst(min), (correlation 0.19). Even for -Bz(min) range 10-20 nT, -Dst(min) values had considerable scatter (correlation 0.57). For -Bz(min). > 20 nT, the relationship was good (correlation 0.82). For the whole range -Bz(min) 0-50 nT, the correlation was high (0.88). Thus, if -Bz(min) is very large (similar to 20 nT), large -Dst(min) occurs but in a wide range of 100-500 nT. (C) 2009 Elsevier Ltd. All rights reserved.
引用
收藏
页码:392 / 400
页数:9
相关论文
共 50 条
  • [21] A study on the main periodicities in interplanetary magnetic field Bz component and geomagnetic AE index during HILDCAA events using wavelet analysis
    Souza, A. M.
    Echer, E.
    Bolzan, M. J. A.
    Hajra, R.
    JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2016, 149 : 81 - 86
  • [22] Cosmic rays during great geomagnetic storms in cycle 23 of solar activity
    Kravtsova, M. V.
    Sdobnov, V. E.
    GEOMAGNETISM AND AERONOMY, 2016, 56 (02) : 143 - 150
  • [23] Cosmic rays during great geomagnetic storms in cycle 23 of solar activity
    M. V. Kravtsova
    V. E. Sdobnov
    Geomagnetism and Aeronomy, 2016, 56 : 143 - 150
  • [24] Response of the geomagnetic activity to solar wind turbulence during solar cycle 23
    D'Amicis, R.
    Bruno, R.
    Bavassano, B.
    JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2011, 73 (5-6) : 653 - 657
  • [25] Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms
    Shi XiaoFei
    Zong QiuGang
    Wang YongFu
    SCIENCE CHINA-TECHNOLOGICAL SCIENCES, 2012, 55 (10) : 2769 - 2777
  • [26] Solar and Heliospheric Causes of Geomagnetic Perturbations during the Growth Phase of Solar Cycle 23
    V. Bothmer
    I. S. Veselovsky
    A. V. Dmitriev
    A. N. Zhukov
    P. Cargill
    E. P. Romashets
    O. S. Yakovchouk
    Solar System Research, 2002, 36 : 499 - 506
  • [27] Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison
    Mitsakou, E.
    Babasidis, G.
    Moussas, X.
    ADVANCES IN SPACE RESEARCH, 2009, 43 (04) : 495 - 498
  • [28] Solar Sources of Interplanetary Coronal Mass Ejections During the Solar Cycle 23/24 Minimum
    E. K. J. Kilpua
    M. Mierla
    A. N. Zhukov
    L. Rodriguez
    A. Vourlidas
    B. Wood
    Solar Physics, 2014, 289 : 3773 - 3797
  • [29] Solar Sources of Interplanetary Coronal Mass Ejections During the Solar Cycle 23/24 Minimum
    Kilpua, E. K. J.
    Mierla, M.
    Zhukov, A. N.
    Rodriguez, L.
    Vourlidas, A.
    Wood, B.
    SOLAR PHYSICS, 2014, 289 (10) : 3773 - 3797
  • [30] The intensity of geomagnetic storms associated with the interplanetary magnetic field and solar wind parameters during Solar Cycle 24
    Santoso, Anwar
    Sismanto, Sismanto
    Priyatikanto, Rhorom
    Hartantyo, Eddy
    Martiningrum, Dyah R.
    EARTH AND PLANETARY PHYSICS, 2025, 9 (02) : 375 - 386