实验室模拟彗星的电荷交换产生的X射线辐射
P Beiersdorfer1, K R Boyce, G V Brown
1Lawrence Livermore National Laboratory, 7000 East Avenue, L-260, Livermore, CA 94550, USA. beiersdorfer@llnl.gov
概括
高电荷离子的实验室X射线光谱揭示了复杂的辐射. 一个新的电荷交换模型成功地解释了彗星线性.
科学领域:
- 空间物理 空间物理
- 等离子体物理学的物理学
- 原子物理 原子物理
背景情况:
- 太阳风与彗星大气层的相互作用产生复杂的X射线辐射.
- 以前的模型很难准确地预测这些柔软的X射线光谱.
研究的目的:
- 模拟和分析来自电荷交换反应的X射线辐射.
- 开发和验证彗星X射线光谱的新模型.
主要方法:
- 实验室实验使用微热量计探测器记录X射线辐射.
- 模拟涉及高电荷碳,和氧离子的电荷交换反应.
- 开发一种新的充电交换排放模型.
主要成果:
- 观察到的X射线光谱很复杂,与现有的预测不匹配.
- 开发的电荷交换辐射模型成功地复制了线性彗星C/1999 S4.4的软X射线光谱.
结论:
- 新模型提供了对彗星X射线发射过程的更好理解.
- 这项工作验证了模型解释诸如钱德拉X射线天文台等任务的观测的能力.
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