在太阳上的水
L Wallace1, P Bernath, W Livingston
1Kitt Peak National Observatory, National Optical Astronomy Observatories, Tucson, AZ 85726, USA.
概括
科学家们分析了太阳黑子阴影中的红外光谱,确定了许多太阳水吸收线. 这些线与热水过渡相对应,实验室光谱证实了这一点.
科学领域:
- 天文学和天体物理学
- 频谱学是一种光谱学.
- 大气科学 大气科学
背景情况:
- 太阳黑子阴影是太阳表面强烈磁活动的区域.
- 了解太阳大气层的组成需要详细的光谱分析.
- 水蒸气是各种天体物理环境中的关键分子.
研究的目的:
- 研究太阳黑子阴影中水分子的存在和过渡.
- 为了确定高分辨率红外太阳光谱中的特定吸水特征.
- 使用实验室数据来描述这些水道的性质.
主要方法:
- 在基特山峰采集高分辨率红外光谱,使用1米富里埃变换光谱仪.
- 分析太阳光谱以检测吸收特征.
- 观察到的太阳能水线与水的高温实验室排放光谱的比较.
主要成果:
- 在太阳黑子阴影光谱中检测到大量的吸水特征.
- 这些特征成功地被分配给热水的纯旋转和振动旋转过渡.
- 这些任务通过与高温水的实验室生成的光谱进行匹配来验证.
结论:
- 这项研究证实了太阳黑子中存在热水分子的存在.
- 高分辨率红外光谱是一种强大的工具,用于识别太阳特征中的分子.
- 这些发现有助于我们了解太阳大气中的化学和物理条件.
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