太阳扭曲振荡的太阳地震测量
S V Vorontsov1, J Christensen-Dalsgaard, J Schou
1Astronomy Unit, Queen Mary, University of London, Mile End Road, London E1 4NS, UK.
概括
太阳的扭转振荡涉及整个对流膜. 这些表面旋转带随着11年的太阳周期迁移,内部相从中度向极点和赤道传播.
科学领域:
- 太阳物理学和太阳物理研究.
- 研究太阳内部动力学和旋转.
背景情况:
- 扭曲振荡,不同的太阳旋转带,在太阳表面观察到.
- 这些振荡在整个11年的太阳周期中沿度迁移.
研究的目的:
- 为了研究太阳内部旋转的时间变化.
- 为了确定太阳对流膜内的扭曲振荡的程度和行为.
主要方法:
- 分析太阳 p 模式频率.
- 数据采集了近6年的数据,使用太阳和球观测台 (SOHO) 卫星上的迈克尔森多普勒成像仪 (MDI) 仪器.
主要成果:
- 整个太阳对流膜都涉及到扭曲振荡.
- 内部旋转变化显示了从中度向极和赤道的相位传播.
- 这些模式在对流膜的任何深度都存在.
结论:
- 扭曲振荡是一种在整个太阳对流膜中延伸的现象,不仅仅局限于表面.
- 观察到的内部相传播为推动太阳周期的动力学提供了新的见解.
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