概括
银河系宇宙射线质子变化持续到高的日光学度,即使太阳风条件稳定. 这些变化是由旋转的相互作用区域驱动的,可以传播到更高的度.
科学领域:
- 太空物理空间物理学
- 太空物理学 太空物理学
- 宇宙射线物理学 宇宙射线物理学
背景情况:
- 银河系宇宙射线 (GCRs) 在穿越日球时受到太阳活动的调节.
- 了解GCR调制对于太空天气预测和了解日球中的粒子传播至关重要.
研究的目的:
- 研究银河系宇宙射线质子的日球调制的程度和机制.
- 为了确定GCR强度的变化是否可以达到高地图度.
主要方法:
- 关于GCR质子传播的三维模拟.
- 模拟太阳风速度和磁场数据的分析.
- 检查GCR强度变化在不同的地图度.
主要成果:
- GCR质子强度的对应变化持续到高的日光学度.
- 这些变化发生在具有稳定的太阳风速度和磁场的区域.
- 来自低度的GCR变异可以传播到显著更高的度.
结论:
- 球调制效应,特别是来自旋转相互作用区域的效应,不仅限于低球度.
- GCR的变化可以扩展到远远超出日光学电流表的区域.
- 类似的调制模式可能会影响低能粒子,影响它们的加速和传播.
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