Identification of solar sources of major geomagnetic storms
暂无分享,去创建一个
[1] D. Haggerty,et al. Are CME “interactions” really important for accelerating major solar energetic particle events? , 2003 .
[2] N. Gopalswamy,et al. Large solar energetic particle events of cycle 23: A global view , 2003 .
[3] H. Cane,et al. A survey of interplanetary coronal mass ejections in the near-Earth solar wind during 1996-2002 , 2003 .
[4] Yuming Wang,et al. A statistical study on the geoeffectiveness of Earth‐directed coronal mass ejections from March 1997 to December 2000 , 2002 .
[5] O. S. St. Cyr,et al. Coronal mass ejections, interplanetary ejecta and geomagnetic storms , 2000 .
[6] Barbara June Thompson,et al. Relationship of halo coronal mass ejections, magnetic clouds, and magnetic storms , 2000 .
[7] J. W. Griffee,et al. Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer , 1998 .
[8] Bruce T. Tsurutani,et al. Criteria of interplanetary parameters causing intense magnetic storms (Dst < −100 nT) , 1987 .
[9] V. Bothmer,et al. Identification of Solar Sources of Major Geomagnetic Storms between 1996 and 2000 , 2003 .
[10] B. Tsurutani,et al. Interplanetary phenomena associated with very intense geomagnetic storms , 2002 .