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Updated: Mar 7, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
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在2024年5月的太阳超级风暴期间,火星的电离层反应
Jacob Parrott1, Beatriz Sánchez-Cano2, Håkan Svedhem3
1Imperial College London, London, UK. Jacob.parrott@esa.int.
Nature communications
|March 5, 2026
概括
一次大规模的太阳耀斑导致火星下层离子层扩大了278%. 这次太阳能事件揭示了软X射线流和电离层密度之间的新关系.
科学领域:
- 行星科学 行星科学
- 空间物理 空间物理
- 航空学是航空学的.
背景情况:
- 太阳能事件对行星离子层产生重大影响.
- 在火星上观察这些事件是具有挑战性的,因为它们的性质是不可预测的.
研究的目的:
- 为了分析大型太阳耀斑对火星电离层的影响.
- 为了研究软X射线流和电离层密度之间的关系.
主要方法:
- 使用了一种偶然的相互无线电隐蔽观测.
- 在现场分析软X射线辐射强度测量.
主要成果:
- 观测到火星上最大的下层电离层,扩展到其典型尺寸的278%.
- 测量了太阳耀斑后软X射线流量增加了三倍.
- 推断了软X射线流和电离层密度之间的修订关系,受光谱硬化影响.
结论:
- 太阳耀斑可以大大增强火星的下层电离层.
- 软X射线流对电离层密度的影响比以前理解的要复杂得多,这取决于光谱特征.
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