1970年3月7日发生的日食中的火箭紫外线闪光光谱
R J Speer1, W R Garton, J F Morgan
1Imperial College of Science and Technology, London.
Nature
|April 18, 1970
概括
这是第一次在完全日食期间捕捉到极端紫外线闪光谱. 这一突破性的成就为太阳动态外层大气层提供了新的见解.
科学领域:
- 太阳物理 太阳物理
- 天文学 天文学
- 天体物理学 天体物理学
背景情况:
- 完全日食为研究太阳的冠冕提供了独特的机会.
- 极端紫外线 (EUV) 观测对于理解太阳大气动态至关重要.
研究的目的:
- 在完全日食的所有阶段获得和分析极端紫外线闪光谱.
- 在日食期间调查太阳冠冕和染色层的光谱特征.
主要方法:
- 使用专门的仪器来捕获极端紫外线范围内的高分辨率光谱.
- 在完全日食期间协调观测,以覆盖所有阶段.
主要成果:
- 在完全日食期间在极端紫外线中成功获得了前所未有的闪光光谱.
- 分析揭示了与日食不同阶段相对应的独特光谱特征.
结论:
- 这项研究标志着有史以来首次在完全日食期间获得EUV闪光光谱.
- 获得的数据将大大提高我们对太阳大气过程和演变的理解.
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