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太阳风在67P/Churyumov-Gerasimenko彗星的二磁性腔中的质子
Charlotte Goetz1,2, Lucie Scharré3,4, Cyril Simon Wedlund5
1Department of Mathematics, Physics and Electrical Engineering Northumbria University Newcastle-upon-Tyne UK.
概括
科学家首次在彗星的二磁性腔内观察到太阳风质子. 这些意想不到的发现挑战了在特定条件下彗星与太阳风相互作用的现有模型.
科学领域:
- 彗星科学是一门彗星科学.
- 血物理学的等离子体物理学
- 太空天气 太空天气
背景情况:
- 彗星等离子体环境具有不同的区域,如太阳风离子腔和二磁性腔.
- 以前的理解表明,太阳风离子在二磁性腔附近或内部不存在.
研究的目的:
- 报道了在二磁性腔内部对太阳风质子的首次观测.
- 为了描述这些质子签名,并调查潜在的透机制.
- 增强对在非标准条件下彗星与太阳风相互作用的理解.
主要方法:
- 分析了五个具有意想不到质子特征的观测事件.
- 质子能量的特征,方向,位置和时间.
- 排除了诸如电荷转移和中性气体爆发等常见的解释.
主要成果:
- 在二磁性腔内检测到的太阳风质子的五个实例被确定.
- 这些质子表现出与太阳风起源相一致的能量和方向.
- 这些事件发生在中间气体生产速度和低彗星中心距离时.
结论:
- 太阳风质子在二磁性腔中的存在是异常的.
- 特定的太阳风条件,其中速度与行星间磁场平行,被认为是原因.
- 这种配置抑制了质量加载和偏移,允许质子透.
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