Detection of solar gravity mode oscillations
Detection of solar gravity mode oscillations
复制标题
太阳重力模式振荡的检测
作者：
P. Delache;P. Scherrer
对斯坦福大学太阳观测站获得的太阳速度数据的分析表明，存在45-105 µHz（160-370 min）范围内的太阳全球振荡。这些振荡被解释为度为l = 1和l = 2的内部重力模式。一个很好的估计的阶的模式也已作出。
An analysis of solar velocity data obtained at the Stanford Solar Observatory shows the existence of solar global oscillations in the range 45–105 µHz (160–370 min). These oscillations are interpreted as internal gravity modes of degreel= 1 andl= 2. A good estimate of the order of the modes has also been made.