active solar region

基本解釋

Just as a sunspot was turning away from Earth on Sept. 8, the active region erupted, producing a solar flare and a fantastic prominence.
9月8日正當(dāng)太陽(yáng)黑子開(kāi)始遠(yuǎn)離地球的時(shí)候，活躍區(qū)域又發(fā)生一次爆發(fā)，同時(shí)出現(xiàn)一個(gè)明顯的突起。
The main characteristics of the perturbations can be explained by the variations of the ionizing sources which were located in the solar active region.
利用當(dāng)時(shí)太陽(yáng)活動(dòng)區(qū)離化源的變化可以解釋擾動(dòng)的主要特征。
Spicules line the above frame of solar active region 11092 that crossed the Sun last month, but are particularly evident converging on the sunspot on the lower left.
這些針狀體在上個(gè)月穿過(guò)太陽(yáng)的太陽(yáng)活躍區(qū)域 11092 號(hào)中形成一條條線，不過(guò)聚集在左下角太陽(yáng)黑子上的針狀體特別的明顯。