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Updated: Jul 10, 2026

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Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
木星的夜边空气发光和极光
G Randall Gladstone1, S Alan Stern, David C Slater
1Southwest Research Institute, San Antonio, TX 78238, USA. rgladstone@swri.edu
概括
新地平线号的数据显示,木星的紫外线夜光不足令人惊,与旅行者号的观测不同. 木星是木星,木星是木星,木星是木星.
科学领域:
- 行星科学 行星科学
- 航空学是航空学的.
- 磁层物理 磁层物理
背景情况:
- 木星的夜间大气表现出极光和空气发光的排放.
- 旅行者航天器在1979年之前的观测记录了紫外线夜光.
- 近太空环境和上大气层的相互作用是复杂的.
研究的目的:
- 用新地平线号的数据研究木星夜边的空气发光和极光.
- 为了将当前的观测与旅行者任务的历史数据进行比较.
- 了解推动木星大气排放的变化和机制.
主要方法:
- 来自新地平线飞越的紫外线和可见辐射数据的分析.
- 排放模式与沉电子流和能量的相关性.
- 在木星的夜面发射的空间映射.
主要成果:
- 观察到一个意想不到的紫外线夜间发光排放的缺席.
- 沉的电子流和能量随着夜边当地时间的变化而减少.
- 来自Io-木星相互作用的可见辐射延伸到很高的海拔,表明低能电子沉.
结论:
- 木星的夜间大气排放是高度可变的,并未完全理解.
- 木星磁层的黄昏侧面是电子沉的潜在来源区域.
- 白天的观测并不能可靠地预测夜间的现象.
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