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接近红外的吸收光谱学用于天体物理学上重要的离子
Kirsten Dowd1, Eric Doyle1, Padraig Dunne1
1School of Physics, University College Dublin, Dublin, 4 Ireland.
概括
这项研究引入了一个新的实验室天体物理学实验,用于近红外光吸收光谱. 这种新的技术在亚等离子体中发现了29条新的光谱线,为天文学提升了原子数据.
科学领域:
- 实验室天体物理学
- 原子光谱学是一种原子光谱学.
- 血物理学的等离子体物理学
背景情况:
- 准确的原子数据对于解释天文观测至关重要.
- 复杂的地面和空间光谱仪需要精确的原子结构信息.
研究的目的:
- 开发和演示一种新的实验室天体物理学实验,用于获得光吸收光谱.
- 在近红外 (NIR) 区域测量中性和近中性原子物种的光谱线.
- 为了突出在多消息传递器天文学中需要新的原子结构数据.
主要方法:
- 使用超连续光纤激光器探测了含有目标离子的激光生成等离子.
- 使用0.75m光谱仪和CMOS摄像头记录了吸收光谱.
- 伊特等离子体的光谱在700-1100纳米范围内在形成后11微秒内得到.
主要成果:
- 在NIR区域成功记录了等离子体的光吸收光谱.
- 在708到832nm之间,检测到26个以前已识别的光谱线和29个以前未识别的线.
- 该实验证明了识别新光谱特征的能力.
结论:
- 开发的技术对于在实验室等离子体中产生光吸收光谱是有效的.
- 识别新的光谱线为原子结构数据库提供了有价值的数据.
- 这项研究通过提供必要的原子数据来支持天文观测的进步.
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