234 citations
- Chinese Academy of SciencesCN27 papers
- National Astronomical ObservatoriesCN22 papers
- University of Chinese Academy of SciencesCN15 papers
- Institute of High Energy PhysicsCN12 papers
- The University of TokyoJP12 papers
- Hebei Normal UniversityCN11 papers
- Shandong UniversityCN11 papers
- Southwest Jiaotong UniversityCN11 papers
- Tibet UniversityCN11 papers
- Hirosaki UniversityJP10 papers
- Kanagawa UniversityJP10 papers
- Konan UniversityJP10 papers
Showing physics.space-phShow all
3 papers · 1 filter
physics.space-ph2020★ 23 cited
Dependence of great geomagnetic storm intensity (SYM-H-200 nT) on associated solar wind parameters
Ming-Xian Zhao, Gui-Ming Le, Qi Li +2
We use SYM-H to capture the variation in the SYM-H index during the main phase of a geomagnetic storm. We define great geomagnetic storms as those with SYM-H -200 nT. A…
physics.space-ph2020★ 21 cited
Dependence of Intensities of Major Geomagnetic Storms (Dst -100 nT) on Associated Solar Wind Parameters
Gui-Ming Le, Gui-Ang Liu, Ming-Xian Zhao
A geomagnetic storm is the result of sustained interaction between solar wind with a southward magnetic field and the magnetosphere. To investigate the influence of various solar w…
physics.space-ph2019★ 16 cited
Sun-Earth connection Event of Super Geomagnetic Storm on March 31, 2001: the Importance of Solar Wind Density
Li-Bin Cheng, Gui-Ming Le, Ming-Xian Zhao
An X1.7 flare at 10:15 UT and a halo CME with a projected speed of 942 km/s erupted from NOAA solar active region 9393 located at N20W19, were observed on 2001 March 29. When the C…