In different initial corona, this paper simulates the coronal response to new magnetic flux eruption and thermal energy release at the coronal base.
英
美
-
本文從MHD方程組出發(fā);在不同的初態(tài)日冕中;數值模擬了日冕底部新磁通量噴發(fā)和熱壓力擾動(dòng)兩種驅動(dòng)機制的日冕響應.
-
国内精品美女A∨在线播放xuan