Publications of Ming-Xian Zhao

A list of publications authored or co-authored by Ming-Xian Zhao, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.

Orcid ID: 0000-0002-1031-018X

List of publications ordered by citations
Number of papers: 31 (refereed: 30)
No. of citations: 419
First author papers: 9 (refereed: 9)

2025

  1. Revisiting the solar wind structures contributing crucially to the main phase of the major geomagnetic storms in May 1997 [0]
    Li, Qi, Zhao, Ming-Xian & Le, Gui-Ming, Terrestrial, Atmospheric and Oceanic Sciences, 36, 31
  2. Dependence of SYMH Change Rate on Dynamic Pressure during the Main Phases of Storms: A Comparative Analysis of the 2024 May and 2003 November Superstorms [3]
    Zhao, Ming-Xian & Le, Gui-Ming, ApJ, 978, 157

2024

  1. An index description of the general characteristics of thermospheric density based on the Two-Line-Element datasets and the Spectral Whitening Method [0]
    Woo, yihan, Mao, Tian, Wang, Jing-Song, Tang, Wei, Song, Qiao & Zhao, Ming-Xian, 171517992.22139574
  2. An Index Description of the General Characteristics of Thermospheric Density Based on the Two-Line-Element Data Sets and the Spectral Whitening Method [2]
    Wu, Yihan, Mao, Tian, Wang, Jing-Song, Tang, Wei, Song, Qiao & Zhao, Ming-Xian, Journal of Geophysical Research (Space Physics), 129, e2024JA032733
  3. Establishment and Application of an Interplanetary Disturbance Index Based on the Solar Wind–Magnetosphere Energy Coupling Function and the Spectral Whitening Method [0]
    Zhao, Xiaowei, Wang, Jingsong, Zhao, Mingxian, Liu, Ying D., Hu, Huidong, Liu, Mingzhe, Mao, Tian & Zong, Qiugang, ApJ, 970, 133

2023

  1. Properties of the Main Phases of the Super Geomagnetic Storms (ΔSYM-H ≤ -250 nT) with Different Heliolongitudes [2]
    Zhao, Ming-Xian, Le, Gui-Ming & Liu, Yong-Hua, Research in Astronomy and Astrophysics, 23, 015007

2022

  1. Properties of the Geomagnetic Storm Main Phase and the Corresponding Solar Wind Parameters on 21–22 October 1999 [9]
    Li, Qi, Zhao, Ming-Xian & Le, Gui-Ming, Universe, 8, 346
  2. What Can We Learn from the Geoeffectiveness of the Magnetic Cloud on 2012 July 15-17? [8]
    Liu, Gui-Ang, Zhao, Ming-Xian, Le, Gui-Ming & Mao, Tian, Research in Astronomy and Astrophysics, 22, 015002
  3. N-S Asymmetry and Solar Cycle Distribution of Superactive Regions from 1976 to 2017 [5]
    Zhao, Ming-Xian, Le, Gui-Ming & Liu, Yong-Hua, Universe, 8, 605
  4. A New Index to Describe the Response of Geomagnetic Disturbance to the Energy Injection from the Solar Wind [6]
    Zhao, Ming-Xian, Wang, Jing-Song & Zhao, Xiao-Wei, Universe, 8, 506
  5. Can We Estimate the Intensities of Great Geomagnetic Storms (ΔSYM-H ≤ -200 nT) with the Burton Equation or the O'Brien and McPherron Equation? [10]
    Zhao, Ming-Xian, Le, Gui-Ming & Lu, Jianyong, ApJ, 928, 18

2021

  1. Source Locations and Solar-Cycle Distribution of the Major Geomagnetic Storms (Dst ≤−100 nT) from 1932 to 2018 [8]
    Le, Gui-Ming, Zhao, Ming-Xian, Zhang, Wen-Tao & Liu, Gui-Ang, Solar Physics, 296, 187
  2. Statistical and Solar Cycle Distribution of Daily Flux ≥109cm−2 d−1 sr−1 for E >2 MeV Electrons Observed by GOES During 1987 - 2019 [6]
    Le, Gui-Ming, Zhang, Yi-Ning & Zhao, Ming-Xian, Solar Physics, 296, 16
  3. Extreme space weather events caused by super active regions during solar cycles 21-24 [6]
    Le, Gui-Ming, Liu, Gui-Ang, Zhao, Ming-Xian, Mao, Tian & Xu, Ping-Guo, Research in Astronomy and Astrophysics, 21, 130
  4. Characteristics of source locations and solar cycle distribution of the strong solar proton events (≥1000 pfu) from 1976 to 2018 [10]
    Le, Gui-Ming, Zhao, Ming-Xian, Qi-Li, Liu, Gui-Ang, Mao, Tian & Xu, Ping-Guo, MNRAS, 502, 2043
  5. Dependence of Great Geomagnetic Storm (Δ SYM-H≤−200 nT) on Associated Solar Wind Parameters [20]
    Zhao, Ming-Xian, Le, Gui-Ming, Li, Qi, Liu, Gui-Ang & Mao, Tian, Solar Physics, 296, 66

2020

  1. Sun-Earth connection event of super geomagnetic storm on 2001 March 31: the importance of solar wind density [16]
    Cheng, Li-Bin, Le, Gui-Ming & Zhao, Ming-Xian, Research in Astronomy and Astrophysics, 20, 036
  2. Dependence of Major Geomagnetic Storm Intensity (Dst ≤−100 nT) on Associated Solar Wind Parameters [16]
    Le, Gui-Ming, Liu, Gui-Ang & Zhao, Ming-Xian, Solar Physics, 295, 108
  3. A study on the dynamic spectral indices for SEP events on 2000 July 14 and 2005 January 20 [3]
    Zhao, Ming-Xian & Le, Gui-Ming, Research in Astronomy and Astrophysics, 20, 037

2018

  1. Investigation of the possible source for the solar energetic particle event on 2017 September 10 [19]
    Zhao, Ming-Xian, Le, Gui-Ming & Chi, Yu-Tian, Research in Astronomy and Astrophysics, 18, 074

2016

  1. Support Vector Machine combined with Distance Correlation learning for Dst forecasting during intense geomagnetic storms [26]
    Lu, J. Y., Peng, Y. X., Wang, M., Gu, S. J. & Zhao, M. X., Planetary and Space Science, 120, 48

2015

  1. A three-dimensional high Mach number asymmetric magnetopause model from global MHD simulation [53]
    Liu, Z.-Q., Lu, J. Y., Wang, C., Kabin, K., Zhao, J. S., Wang, M., Han, J. P., Wang, J. Y. & Zhao, M. X., Journal of Geophysical Research (Space Physics), 120, 5645
  2. Pressure balance across the magnetopause: Global MHD results [18]
    Lu, J. Y., Wang, M., Kabin, K., Zhao, J. S., Liu, Z.-Q., Zhao, M. X. & Li, G., Planetary and Space Science, 106, 108
  3. The dipole tilt angle dependence of the bow shock for southward IMF: MHD results [17]
    Wang, M., Lu, J. Y., Yuan, H. Z., Kabin, K., Liu, Z.-Q., Zhao, M. X. & Li, G., Planetary and Space Science, 106, 99

2014

  1. MHD simulation of energy transfer across magnetopause during sudden changes of the IMF orientation [17]
    Jing, H., Lu, J. Y., Kabin, K., Zhao, J. S., Liu, Z.-Q., Yang, Y. F., Zhao, M. X. & Wang, M., Planetary and Space Science, 97, 50

2013

  1. The IMF dependence of the magnetopause from global MHD simulations [34]
    Lu, J. Y., Liu, Z.-Q., Kabin, K., Jing, H., Zhao, M. X. & Wang, Y., Journal of Geophysical Research (Space Physics), 118, 3113

2012

  1. Dipole tilt control of the magnetopause for southward IMF from global magnetohydrodynamic simulations [35]
    Liu, Z.-Q., Lu, J. Y., Kabin, K., Yang, Y. F., Zhao, M. X. & Cao, X., Journal of Geophysical Research (Space Physics), 117, A07207
  2. Nonlinear dispersive scale Alfvén waves inmagnetosphere-ionosphere coupling: Physical processes and simulation results [3]
    Zhao, MingXian & Lu, JianYong, Chinese Science Bulletin, 57, 1384

2011

  1. Three dimensional shape of the magnetopause: Global MHD results [51]
    Lu, J. Y., Liu, Z.-Q., Kabin, K., Zhao, M. X., Liu, D. D., Zhou, Q. & Xiao, Y., Journal of Geophysical Research (Space Physics), 116, A09237

2010

  1. A sensitive geomagnetic activity index for space weather operation [7]
    Du, D., Xu, W. Y., Zhao, M. X., Chen, B., Lu, J. Y. & Yang, G. L., Space Weather, 8, S12006
  2. Vertical ozone profiles deduced from measurements of SBUS on FY-3 satellite [9]
    Huang, FuXiang, Liu, NianQing, Zhao, MingXian, Wang, ShuRong & Huang, Yu, Chinese Science Bulletin, 55, 943

Created on Wed Apr 8 04:39:23 2026.