一个行星间的冲击,由行星极光风暴追踪,从太阳到土星
Renée Prangé1, Laurent Pallier, Kenneth C Hansen
1LESIA, Observatoire de Paris, 5 place Jules Janssen, 92195 Meudon, France. renee.prange@obspm.fr
Nature
|November 5, 2004
概括
来自太阳爆发的行星间冲击引发地球上的极光风暴,并增强木星和土星等外行星上的极光活动. 这些冲击在整个太阳系中保持它们的特性,影响行星空间环境.
科学领域:
- 空间物理 空间物理
- 行星科学 行星科学
- 太阳物理 太阳物理
背景情况:
- 太阳活动,包括冠状质量喷射 (CMEs),产生行星间冲击.
- 这些冲击对地球磁层产生影响,导致极光风暴,并用于太空天气预报.
- 在外行星上也观察到极光,这表明类似的太阳-地球相互作用.
研究的目的:
- 为了研究行星间冲击对土星极光的影响.
- 追踪太阳能驱动冲击在整个太阳系的传播和影响.
- 了解行星之间的冲击对行星极光的反应.
主要方法:
- 对地球,木星和土星上的极光活动的观测数据分析.
- 极光事件与记录的行星间冲击通道的相关性.
- 将冲击的起源追溯到特定的太阳冠状质量弹射 (CME) 事件.
主要成果:
- 在土星上发现强烈的,短暂的极性辐射,与行星间冲击有关.
- 在地球上观察到极光风暴,在木星上极光活动增强,与冲击的过渡相吻合.
- 冲击成功触发了土星上不寻常的极地极光活动.
结论:
- 星际冲击保留了它们的特性和触发整个太阳系行星极光活动的能力.
- 太阳能驱动的冲击是多个行星上的极光现象的重要驱动因素.
- 行星极光对冲击的反应表现出度和当地时间依赖的变化.
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