在旅行者2号飞越期间,天王星磁层的异常状态
Jamie M Jasinski1, Corey J Cochrane1, Xianzhe Jia2
1NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.
概括
旅行者2号在极端的太阳风压缩期间遇到了天王星,而不是它的典型状态. 这种压缩的磁层可以解释天王星的磁层.
科学领域:
- 行星科学 行星科学
- 空间物理 空间物理
- 磁层物理 磁层物理
背景情况:
- 1986年旅行者2号飞越天王星时,发现了一个斜的,偏离中心的磁场,导致其被解释为极端磁层.
- 天王星的磁层以强烈的电子辐射带和缺少等离子体的环境为特征.
- 外部太阳风对天王星磁层的影响在很大程度上被忽视了.
研究的目的:
- 为了重新评估旅行者2号对天王星磁层的数据.
- 为了调查太阳风条件在飞越过程中的作用.
- 挑战长期以来关于天王星磁层的观点,认为天王星的磁层本质上是极端的.
主要方法:
- 重新检查和分析原来的旅行者2号数据集从天王星飞越.
- 在不同的太阳风条件下建模潜在的磁层配置.
- 估计观察到的压缩状态的频率.
主要成果:
- 旅行者2号观察到天王星的磁层处于高度压缩的状态,可能在5%以下的时间内存在.
- 上游太阳风动态压力显著降低 (~20倍低) 会导致一个截然不同的磁层配置.
- 观察到的压缩可能会暂时增加能量电子流,并耗尽磁层等离子体.
结论:
- 天王星磁层的"极端"性质可能是旅行者2号在异常太阳风条件下发生的飞越的工件.
- 太阳风的外部强迫是理解天王星磁层动态的一个关键因素.
- 未来的研究应该考虑太阳风压力对行星磁层的可变影响.
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