搜索结果: 1-1 共查到“太阳系物理学 Non-radial modes”相关记录1条 . 查询时间(0.062 秒)
In cool stars that oscillate like the Sun, non-radial modes become mixed as the stars evolve. The mixing is caused by the coupling between g-modes in the stellar core and p-modes in the envelope, whic...