"Heejeong separated the data into when the solar wind was fluctuating a lot and when it was fluctuating a little," he added.

“金熙真把太阳风活动剧烈和相对稳定时得到的数据分开，”他又说道，“当行星际磁场波动不大时，她得到的结果和我们熟悉的一样。