solar-ray electron

Most extreme high level of electron flux at geostationary orbit occurred during the geomagnetic storm recovery phase with the solar wind proton density lower than 4 cm-3 and strong substorm activity.

绝大多数高通量事件都是出现在磁暴恢复相期间，且太阳风质子密度低于4个/cm3并伴有亚暴时才会发生。

Low solar wind density and the strong substorm are the two key parameters leading to the 2 MeV electron flux at geostationary orbit reach very high level during the geomagnetic storm recovery phase.

在磁暴恢复相期间，低的太阳风密度和强的亚暴是导致地球同步轨道能量大于2MeV电子通量的达到极高值的两个关键参数。

However, organic solar cells based on carbon nanotubes is the carbon nanotubes powder and organic materials blends, the combination between carbon nanotubes is weak, resulting in greater resistance and high electron hole on the composite, making the efficiency of the solar cell is low.

然而，基于碳纳米管的有机太阳能电池是将粉末状的碳纳米管与有机材料共混，碳纳米管之间的结合较弱，因此导致较大的电阻且电子空穴对容易发生复合，使得太阳能电池的效率很低。

Effect of bound electron capture on~ 7Be solar neutrino flux

束缚电子对~7Be太阳中微子流量的影响

Solar flares with duration 1.5 hours do not disturb the electron content.

持续时间小于1.5小时的耀斑对电子含量影响甚微；