太阳耀斑对火星电离层的影响
Michael Mendillo1, Paul Withers, David Hinson
1Center for Space Physics, Boston University, Boston, MA 02215, USA.
概括
太阳耀斑显著增强火星的电离层高达200%. 这些效应是由紫外线上的增强软X射线流驱动的,由火星全球测量器观察到.
科学领域:
- 行星科学 行星科学
- 太阳物理 太阳物理
- 大气科学 大气科学
背景情况:
- 行星大气对太阳X射线和紫外线 (UV) 耀斑产生反应.
- 这些太阳耀斑效应的连续,可靠的测量主要适用于地球.
- 了解其他行星上的这些大气反应对于比较行星学至关重要.
研究的目的:
- 报告和分析太阳耀斑对火星电离层的影响.
- 量化太阳耀斑事件引起的火星电离层增强.
- 为了研究在火星上的太阳耀斑期间软X射线和紫外线辐射的相对贡献.
主要方法:
- 利用来自火星全球测量器航天器的数据.
- 分析了2001年4月的观测结果,特别关注太阳耀斑事件.
- 采用大气模型来了解耀斑效应的高度依赖.
主要成果:
- 在太阳耀斑事件期间观察到火星离子层增强高达200%.
- 确定软X射线流中的相对增强明显超过紫外线流中的相对增强.
- 建立了太阳耀斑强度和火星上的电离层反应之间的联系.
结论:
- 太阳耀斑对火星的电离层有实质性和可测量的影响.
- 软X射线在推动火星上这些电离层增强方面比紫外线辐射发挥更为主导作用.
- 对太阳-地球和太阳-火星大气反应的比较研究是必不可少的.
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