本文研究太阳从可见光至近红外连续谱中的五分钟振荡。
The five-minute oscillations in the solar continuum arc analyzed in this paper.
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.
太阳振荡研究现已成为研究太阳内部性质的新手段，也成为检验太阳模型构造时输入物理参量的最重要工具。
Helioseismology has become a new tool for the study of the solar interior as well as one of the most important devices to determine the quality of the the input physics that enters the solar models.
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