太阳周期内宇宙核的太阳调制:阿尔法磁谱仪的结果
M Aguilar1, B Alpat2, G Ambrosi2
1Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), 28040 Madrid, Spain.
Physical review letters
|February 21, 2025
概括
银河系宇宙核的流动表现出太阳周期的变化. 它们的调制取决于光谱形状,而不是速度,揭示了对太空天气影响的见解.
科学领域:
- 宇宙射线物理学 宇宙射线物理学
- 太空物理学 太空物理学
- 天体物理学 天体物理学
背景情况:
- 银河系宇宙射线 (GCR) 是来自太阳系外的高能粒子.
- 太阳活动显著影响到达地球的GCR流量.
- 了解GCR调制对于太空天气预测和仪器设计至关重要.
研究的目的:
- 在11年的太阳周期中研究宇宙核流动 (从到氧) 的时间变化.
- 确定太阳能调制对核特性 (如光谱形状和质量电荷比) 的依赖.
- 为GCR调制机制提供模型独立的见解.
主要方法:
- 从2011年5月到2022年11月对宇宙核流 (He,Li,Be,B,C,N,O) 的分析.
- 测量度范围为1.92至60.3GV的流量.
- 太阳能调制幅度,光谱指数和质量电荷比之间的相关性分析.
主要成果:
- 宇宙核流动在太阳周期中显示出类似的,依赖于刚性的时间变化.
- 较低刚度的Li,Be,B,C,N和O流量比更少调制.
- 太阳能调制的差异与光谱指数差异线性相关,独立于特定的调制模型.
- 根据质量与电荷比率 (A/Z) 观察到没有显著的调制差异.
结论:
- 银河系宇宙核的太阳调制主要取决于它们的光谱形状.
- 观察到的调制差异并不能通过对质量-电荷比的速度依赖来解释.
- 这项研究提供了对GCR调制机制的模型独立理解.
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