We examine the solar injection of electrons and ions in eleven electron/~3He-rich SEP events with a clear velocity dispersion, the ~3He/~4He ratio > 0.1, and good count statistics. The velocity dispersion analysis shows that both electrons and ions experience nearly scatter-free propagation. Thus, we are able to obtain the electron injection profile versus energy from in situ observations for all the selected events, and the ion injection profile for one event with good enough ion statistics. We estimate the onset time and peak time of the solar ion injection from in situ observations for the other events. We find a systematic delay of the solar injection of ~3He-rich ions relative to impulsive electrons. The majority of the events have no Ha and GOES SXR flares, but all have a type Ⅲ burst and one has a coronal type Ⅱ burst. Ten events with the SOHO/LASCO coronagraph coverage have a west-limb CME that begins close to the start time of electron injection, and reaches a median altitude of ～4.2 Rs above the photosphere at the start time of ion injection. The majority of these CMEs are fast and narrow.
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机译：识字和算术磁性图。白色磁性片，可轻松放置在白板上。各种类型的图表，包括大型写作图表，Andrewa的电磁数学表格和学生魔术写作图表。图表可以水平（600x900mm）或（250x200mm）或垂直（900mmx600mm）排列。写作图表用虚线表示。粗线为蓝色，虚线为红色。 Andrewa的Magnetic Math Grid由50x50mm的蓝色方块组成;网格为594x841mm，由十七行十一列组成。
