概括
在太阳的上方对流带中,大的波动速度场会降低太阳的p-mode固有频率. 这一发现影响了对太阳对流带深度和太阳流结构的估计.
科学领域:
- * * 太阳地震学 太阳地震学
- * 太阳物理 太阳物理
- * 流体动力学 流体动力学
背景情况:
- * 太阳p模式是通过太阳内部传播的声学振荡.
- *太阳的对流区是流动等离子体运动的区域.
- *了解这些振荡是探测太阳内部结构的关键.
研究的目的:
- * 为了研究太阳对流动性流对p模式固有频率的影响.
- * 为了确定观察到的频率变化是否可以提供关于太阳对流动性流的结构的信息.
- * 评估这些影响对对流动带深度测量的影响.
主要方法:
- * 分析太阳 p 模式固有频率.
- * 与在上方对流区的大波动速度场的相关性.
- *研究频率依赖于水平波数和频率的研究.
主要成果:
- * 观察到平均太阳p模式固有频率的下降.
- * 这种效应在具有高水平波数和频率的模式中最为明显.
- *频率下降的幅度是显著的.
结论:
- * 太阳对流带中的波动速度场直接影响p-mode固有频率.
- *这些影响足以改变对流动带深度的测量.
- * 观察到的频率转移为研究太阳对流动流提供了潜在的新方法.
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