太阳振荡的湍动随机激发及激发源的位置都已得到研究，不过现在问题还未完全解决。
The stochastic excitation mechanism by turbulence and the location of the excitation sources are well studied, but not completely understood.
利用理论结果的计算表明，对流层的湍动对流完全有可能激发足够的波能去补充日冕中等离子体对流和辐射造成的能量损失。
Evaluation results show that the turbulence in convection zone is capable of generating enough wave energy to supply coronal energy lose due to convection and radiation.
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