相关实验视频
Updated: Jun 29, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
由于表面磁性,明显的太阳光度大大过剩
Martin D Fivian1, Hugh S Hudson, Robert P Lin
1Space Sciences Laboratory, University of California-Berkeley, Berkeley, CA 94720, USA. mfivian@ssl.berkeley.edu
概括
太阳,就是太阳.
科学领域:
- 太阳物理 太阳物理
- 天文学 天文学
- 太空物理学 太空物理学
背景情况:
- 太阳的形状受到其旋转和内部动态的影响.
- 表面旋转预测了特定的太阳平坦度 (赤道-极点半径差).
- 之前的观察表明,预测和观察到的凸度之间存在差异.
研究的目的:
- 为了调查太阳凸度的差异.
- 识别和纠正高空度测量的系统性错误.
- 为了在没有磁效应的情况下确定太阳的凸度.
主要方法:
- 利用了Reuven Ramaty高能太阳光谱成像仪 (RHESSI) 卫星的数据.
- 分析了太阳四肢位置和极端紫外线 (EUV) 亮度之间的相关性.
- 通过计算太阳能网络中的磁性元素,纠正了曲率测量.
主要成果:
- 观测到的太阳平坦度高于单靠表面旋转预测的水平.
- 肢体亮度和更大的半径值之间发现了强烈的相关性,与磁性活动有关.
- 对于非磁性的太阳,修正后的曲率为8.01 +/- 0.14毫米弧秒.
结论:
- 观察到的过高的平坦度在很大程度上是由于磁力影响.
- 在对磁效应进行校正后,太阳的斜度与其旋转的预测保持一致.
- 这项研究完善了我们对太阳形状及其与内部过程和磁场的关系的理解.
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