Does geomagnetic storm magnitude depend on solar flare importance?

被引:6
|
作者
Yermolaev, Yu. I. [1 ]
Yermolaev, M. Yu. [1 ]
机构
[1] Russian Acad Sci, Space Res Inst, Moscow 117997, Russia
基金
俄罗斯基础研究基金会;
关键词
CORONAL MASS EJECTIONS; EVENTS; CMES;
D O I
10.1134/S0010952509060021
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
In order to predict space weather effects, solar flares are often used as precursors of magnetic storms on the Earth. In particular, possible relation between the solar flare importance and magnetic storm intensity is discussed in some papers. However, published results contradict each other. We compare the published results on the flare-storm dependence and discuss possible causes of this disagreement: (1) different intervals of observation, (2) differing statistics, and (3) different methods of identification of events and their comparison. Our analysis has shown that the fact of occurrence and the magnitude of a geomagnetic storm cannot be determined, generally, using only the solar flare importance. However, analyzing additional information on the coronal mass ejection (CME), associated with the geomagnetic storm, one can offer an algorithm for the storm magnitude prediction on the basis of flare importance.
引用
收藏
页码:460 / 465
页数:6
相关论文
共 50 条
  • [31] Long-period geomagnetic pulsations as solar flare precursors
    N. A. Barkhatov
    V. N. Obridko
    S. E. Revunov
    S. D. Snegirev
    D. V. Shadrukov
    O. A. Sheiner
    Geomagnetism and Aeronomy, 2016, 56 : 249 - 255
  • [32] DIFFUSIVE ENTRY OF SOLAR-FLARE PARTICLES INTO GEOMAGNETIC TAIL
    MICHEL, FC
    DESSLER, AJ
    JOURNAL OF GEOPHYSICAL RESEARCH, 1970, 75 (31): : 6061 - +
  • [33] Long-period geomagnetic pulsations as solar flare precursors
    Barkhatov, N. A.
    Obridko, V. N.
    Revunov, S. E.
    Snegirev, S. D.
    Shadrukov, D. V.
    Sheiner, O. A.
    GEOMAGNETISM AND AERONOMY, 2016, 56 (02) : 249 - 255
  • [34] ON THE IONOSPHERIC CURRENT SYSTEM OF THE GEOMAGNETIC SOLAR FLARE EFFECT (SFE)
    VOLLAND, H
    TAUBENHEIM, J
    JOURNAL OF ATMOSPHERIC AND TERRESTRIAL PHYSICS, 1958, 12 (04): : 258 - 265
  • [35] Does the magnitude of the TWA depend on the amplitude of the corresponding T wave?
    Madias, John E.
    JOURNAL OF CARDIOVASCULAR ELECTROPHYSIOLOGY, 2008, 19 (04) : E32 - E32
  • [36] APPARENT AREA AS A BASIS FOR SOLAR FLARE IMPORTANCE
    SAWYER, CB
    ASTROPHYSICAL JOURNAL, 1967, 147 (01): : 193 - &
  • [38] Impact of the October 28, 2021 Solar Flare and the November 4, 2021 Geomagnetic Storm on the Low, Middle, and High-Latitude Ionosphere
    Uga, Chali Idosa
    Uluma, Edward
    Adhikari, Binod
    Giri, Ashutosh
    Belay, Negasa
    DISCOVER SPACE, 2024, 128 (01)
  • [39] Reconstruction of Solar Wind Features That Caused a Super Geomagnetic Storm
    Lui, A. T. Y.
    Gonzalez, W. D.
    PROCEEDINGS OF THE THIRTEENTH INTERNATIONAL SOLAR WIND CONFERENCE (SOLAR WIND 13), 2013, 1539 : 406 - 409
  • [40] RELATIONSHIP BETWEEN GEOMAGNETIC STORM DEVELOPMENT AND THE SOLAR WIND PARAMETER β
    Kurazhkovskaya, N. A.
    Klain, B., I
    Zotov, O. D.
    SOLAR-TERRESTRIAL PHYSICS, 2021, 7 (04): : 24 - 32