Dependence of EMIC wave parameters during quiet, geomagnetic storm, and geomagnetic storm phase times

被引:38
|
作者
Halford, A. J. [1 ,2 ]
Fraser, B. J. [3 ]
Morley, S. K. [4 ]
Elkington, S. R. [5 ]
Chan, A. A. [6 ]
机构
[1] Dartmouth Coll, Dept Phys & Astron, Hanover, NH 03755 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Univ Newcastle, Ctr Space Phys, Callaghan, NSW, Australia
[4] Los Alamos Natl Lab, Space Sci & Applicat ISR 1, Los Alamos, NM USA
[5] Univ Colorado, LASP, Boulder, CO 80309 USA
[6] Rice Univ, Dept Phys & Astron, Houston, TX USA
基金
澳大利亚研究理事会;
关键词
electromagnetic ion cyclotron waves; geomagnetic storms; wave parameters; CRRES satellite; ULF waves; geomagnetic index; ION-CYCLOTRON WAVES; VAN ALLEN PROBES; MAGNETIC PULSATIONS; RELATIVISTIC ELECTRONS; GEOSYNCHRONOUS ORBIT; STATISTICAL-ANALYSIS; SYNCHRONOUS ORBIT; RADIATION-BELT; MAGNETOSPHERE; CRRES;
D O I
10.1002/2016JA022694
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
As electromagnetic ion cyclotron (EMIC) waves may play an important role in radiation belt dynamics, there has been a push to better include them into global simulations. How to best include EMIC wave effects is still an open question. Recently many studies have attempted to parameterize EMIC waves and their characteristics by geomagnetic indices. However, this does not fully take into account important physics related to the phase of a geomagnetic storm. In this paper we first consider how EMIC wave occurrence varies with the phase of a geomagnetic storm and the SYM-H, AE, and Kp indices. We show that the storm phase plays an important role in the occurrence probability of EMIC waves. The occurrence rates for a given value of a geomagnetic index change based on the geomagnetic condition. In this study we also describe the typical plasma and wave parameters observed in L and magnetic local time for quiet, storm, and storm phase. These results are given in a tabular format in the supporting information so that more accurate statistics of EMIC wave parameters can be incorporated into modeling efforts.
引用
收藏
页码:6277 / 6291
页数:15
相关论文
共 50 条
  • [31] Geomagnetic storm hits Saturn
    不详
    PHYSICS WORLD, 2004, 17 (12) : 3 - 3
  • [32] What is an "Intense geomagnetic storm"?
    Kamide, Y
    SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS, 2006, 4 (06):
  • [33] GIANT SUNSPOT AND GEOMAGNETIC STORM
    不详
    NATURE, 1949, 163 (4136) : 203 - 203
  • [34] Comparing magnetopause predictions from two MHD models during a geomagnetic storm and a quiet period
    Dredger, Pauline M.
    Lopez, Ramon E.
    Collado-Vega, Yaireska M.
    FRONTIERS IN ASTRONOMY AND SPACE SCIENCES, 2023, 10
  • [35] A SOURCE FOR THE GEOMAGNETIC STORM MAIN PHASE RING CURRENT
    LYONS, LR
    WILLIAMS, DJ
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1980, 85 (NA2): : 523 - 530
  • [36] Geomagnetic disturbance intensity dependence on the universal timing of the storm peak
    Katus, R. M.
    Liemohn, M. W.
    Keesee, A. M.
    Immel, T. J.
    Ilie, R.
    Welling, D. T.
    Ganushkina, N. Yu.
    Perlongo, N. J.
    Ridley, A. J.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2016, 121 (08) : 7561 - 7571
  • [37] Dependence of geomagnetic activity during magnetic storms on the solar wind parameters for different types of streams: 2. Main phase of storm
    N. S. Nikolaeva
    Yu. I. Yermolaev
    I. G. Lodkina
    Geomagnetism and Aeronomy, 2012, 52 : 28 - 36
  • [38] Dependence of Geomagnetic Activity during Magnetic Storms on the Solar Wind Parameters for Different Types of Streams: 2. Main Phase of Storm
    Nikolaeva, N. S.
    Yermolaev, Yu. I.
    Lodkina, I. G.
    GEOMAGNETISM AND AERONOMY, 2012, 52 (01) : 28 - 36
  • [39] AN OBSERVATION OF STRONG THERMOSPHERIC WINDS DURING A GEOMAGNETIC STORM
    SMITH, LB
    JOURNAL OF GEOPHYSICAL RESEARCH, 1968, 73 (15): : 4959 - &
  • [40] INFLATION OF GEOMAGNETIC-FIELD DURING A MAGNETIC STORM
    FERRARO, VCA
    GEOPHYSICAL JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY, 1971, 25 (05): : 419 - &