Analysis of solar plasma parameters during intense geomagnetic storm (SYM/H<-100) in 2023

被引:0
作者
Kumar, Pawan [1 ]
Pal, Mahender [1 ]
Singh, Sham [2 ]
机构
[1] IKG Punjab Tech Univ, Dept Phys, Jalandhar, India
[2] Chandigarh Engn Coll CGC Landran, Mohali, India
来源
RADIATION EFFECTS AND DEFECTS IN SOLIDS | 2024年 / 179卷 / 7-8期
基金
美国国家航空航天局;
关键词
Geomagnetic indices; solar wind; geomagnetic storms and solar plasma; WIND; EARTH;
D O I
10.1080/10420150.2024.2378423
中图分类号
TL [原子能技术]; O571 [原子核物理学];
学科分类号
0827 ; 082701 ;
摘要
We utilize numerous solar plasma and field parameters with geomagnetic indices for the geomagnetic storm in 25 solar cycles. Using Planetary index (Kp) having 3 h data, Dst index hourly data, Symmetric horizontal field (SYM/H) minute resolution data and solar plasma measurements from multiple satellites, examine the chain of significant events that occurred in the year 2023. Statical analysis of geomagnetic provisional activity Sym/H has better results than Kp index during various main phases of geomagnetic activity. The statistical correlation technique is used to examine the relationship between Interplanetary parameters and geomagnetic indices during major geomagnetic storms. This research improves our comprehension of solar-terrestrial interactions and provides valuable insights for enhancing space weather forecasting models.
引用
收藏
页码:985 / 993
页数:9
相关论文
共 24 条
  • [1] AKASOFU SI, 1981, SPACE SCI REV, V28, P121, DOI 10.1007/BF00218810
  • [2] EMPIRICAL RELATIONSHIP BETWEEN INTERPLANETARY CONDITIONS AND DST
    BURTON, RK
    MCPHERRON, RL
    RUSSELL, CT
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1975, 80 (31): : 4204 - 4214
  • [3] Sun-Earth connection event of super geomagnetic storm on 2001 March 31: the importance of solar wind density
    Cheng, Li-Bin
    Le, Gui-Ming
    Zhao, Ming-Xian
    [J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2020, 20 (03)
  • [4] Clauen K.U., 2014, J. Geophys. Res.: Space Phys, V119, P9786
  • [5] Interplanetary conditions causing intense geomagnetic storms (Dst ≤-100 nT) during solar cycle 23 (1996-2006)
    Echer, E.
    Gonzalez, W. D.
    Tsurutani, B. T.
    Gonzalez, A. L. C.
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2008, 113 (A5)
  • [6] Foster J.C., 2014, Space Sci. Rev, V184, P35
  • [7] DUAL-PEAK SOLAR-CYCLE DISTRIBUTION OF INTENSE GEOMAGNETIC STORMS
    GONZALEZ, WD
    GONZALEZ, ALC
    TSURUTANI, BT
    [J]. PLANETARY AND SPACE SCIENCE, 1990, 38 (02) : 181 - 187
  • [8] Similarities and differences in low- to middle-latitude geomagnetic indices
    Katus, R. M.
    Liemohn, M. W.
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2013, 118 (08) : 5149 - 5156
  • [9] Kivelson M.G., 1995, J. Geophys. Res.: Space Phys, V100, P9103
  • [10] Kivelson M.G., 1995, Introduction to Space Physics