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木星上的一个脉动的极光X射线热点
G R Gladstone1, J H Waite, D Grodent
1Southwest Research Institute, San Antonio, Texas 78228, USA. randy@whistler.space.swri.edu
Nature
|March 5, 2002
概括
木星的X射线极光不是主要由内磁层离子引起的. 新的观测揭示了外部磁层中一个脉动的"热点",这表明未知的过程驱动了这些强烈的极光辐射.
科学领域:
- 行星科学 行星科学
- 空间物理 空间物理
- 天体物理学 天体物理学
背景情况:
- 木星的X射线极光以前被认为是来自内磁层的有活力的硫和氧离子.
- 这种降水被认为是地球极地X射线排放的主要驱动因素.
研究的目的:
- 通过使用高空间分辨率观测,调查木星X射线极光发射的来源和特征.
- 挑战和完善对木星极光激发机制的现有模型.
主要方法:
- 对木星北极极光区域的高空间分辨率X射线观测.
- 分析发射位置,时间变化以及与其他电磁现象的相关性.
主要成果:
- 大多数北极极光X射线源自一个独特的"热点"极向内磁层连接度.
- 这个热点显示了固定的磁度和经度,与异常的红外和紫外线辐射同时存在.
- X射线脉冲发生在45分钟的周期内,与高度无线电和电子爆发相匹配.
结论:
- 激发木星X射线极光的粒子的主要来源是外部磁层,而不是内部磁层.
- 这些发现使以前关于重离子稳定沉的理论无效.
- 无法解释的外部磁层过程可能会产生这些局部,可变和宽带的X射线辐射.
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