Publications of Gui-Ming Le

A list of publications authored or co-authored by Gui-Ming Le, 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: 0000-0002-9906-5132

List of publications ordered by citations
Number of papers: 17 (refereed: 17)
No. of citations: 120
First author papers: 5 (refereed: 5)

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. Statistical Characteristics of Solar Cycle Distribution of N─S Asymmetry for the Source Locations of Super Geomagnetic Storms (Dst ≤ −250 nT) During 1932─2018 [0]
    Li, Qi & Le, Gui-Ming, Research in Astronomy and Astrophysics, 25, 105004
  3. Latitude Distribution and N-S Asymmetry of GLE Event Source Locations during 1942─2024 [2]
    Zhang, Xi-Wen, Le, Gui-Ming, Zhao, Xu-Dong & Li, Qi, Research in Astronomy and Astrophysics, 25, 075015
  4. 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. Latitudinal and Solar Cycle Distribution of Extreme (≥X5) Flares During 1976─2018 [1]
    Li, Qi, Zhang, Xi-Wen & Le, Gui-Ming, Research in Astronomy and Astrophysics, 24, 125007

2023

  1. Properties of the Main Phases of the Super Geomagnetic Storms (∆SYM-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. Measurement of the Gamma-Ray Energy Spectrum beyond 100 TeV from the HESS J1843-033 Region [7]
    Amenomori, M., Asano, S., Bao, Y. W., Bi, X. J., Chen, D., Chen, T. L., Chen, W. Y., Chen, Xu, Chen, Y., Cirennima, Cui, S. W., Danzengluobu, Ding, L. K., Fang, J. H., Fang, K., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gao, Qi, Gomi, A., Gou, Q. B., Guo, Y. Q., Guo, Y. Y., He, H. H., He, Z. T., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Hu, K. Y., Huang, J., Jia, H. Y., Jiang, L., Jiang, P., Jin, H. B., Kasahara, K., Katayose, Y., Kato, C., Kato, S., Kawashima, T., Kawata, K., Kozai, M., Kurashige, D., Labaciren, Le, G. M., Li, A. F., Li, H. J., Li, W. J., Li, Y., Lin, Y. H., Liu, B., Liu, C., Liu, J. S., Liu, L. Y., Liu, M. Y., Liu, W., Liu, X. L., Lou, Y.-Q., Lu, H., Meng, X. R., Meng, Y., Munakata, K., Nagaya, K., Nakamura, Y., Nakazawa, Y., Nanjo, H., Ning, C. C., Nishizawa, M., Ohnishi, M., Okukawa, S., Ozawa, S., Qian, L., Qian, X., Qian, X. L., Qu, X. B., Saito, T., Sakakibara, Y., Sakata, M., Sako, T., Sako, T. K., Shao, J., Shibata, M., Shiomi, A., Sugimoto, H., Takano, W., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, H., Wang, Y. P., Wangdui, Wu, H. R., Wu, Q., Xu, J. L., Xue, L., Yang, Z., Yao, Y. Q., Yin, J., Yokoe, Y., Yu, N. P., Yuan, A. F., Zhai, L. M., Zhang, C. P., Zhang, H. M., Zhang, J. L., Zhang, X., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhao, S. P., Zhaxisangzhu & Zhou, X. X., ApJ, 932, 120
  2. 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
  3. 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
  4. 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
  5. Can We Estimate the Intensities of Great Geomagnetic Storms (∆SYM-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. 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
  4. Dependence of Great Geomagnetic Storm (∆ 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. 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
  2. The Properties of Source Locations and Solar Cycle Distribution of GLEs During 1942-2017 [13]
    Le, Gui-Ming & Liu, Gui-Ang, Solar Physics, 295, 35

Created on Wed Apr 22 04:36:42 2026.