摘要: Ulysses observations reveal that most coronal mass ejections (CMES) observed in the solar wind far from the Sun at high heliographic latitudes have large radial widths and are still expanding as they pass the spacecraft. CME radia... 展开
作者 | Gosling, J. T. Riley, P. McComas, D. J. Pizzo, V. J. | ||
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原报告号 | N19980205837 | 总页数 | 14 |
主办者 | Department of Energy, Washington, DC.^National Aeronautics and Space Administration, Washington, DC. | ||
报告类别/文献类型 | NASA / NTIS科技报告 | ||
关键词 | Coronal mass ejection Ulysses mission Expansion Simulation Solar corona Satellite observation Solar wind Radial distribution Solar activity effects Sun Internal pressure Astronomical observatories Solar wind velocity Interplanetary magnetic fields Models Spaceborne astronomy Spectroheliographs |