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由于极地极光,木星的全球上层大气变暖
J O'Donoghue1,2, L Moore3, T Bhakyapaibul3
1Department of Solar System Science, JAXA Institute of Space and Astronautical Science, Sagamihara, Japan. jameso@ac.jaxa.jp.
Nature
|August 5, 2021
概括
木星
科学领域:
- 星球科学
- 大气物理
- 太空物理
背景情况:
- 木星的上层大气层出乎意料地热,极光能量沉积集中在极地.
- 全球循环模型表明极光能量被困在高度,
- 之前的研究缺乏全行星的高分辨率数据来确定木星的温度梯度和主要的热源.
研究的目的:
- 调查木星上层大气中的全球温度梯度.
- 确定负责木星大气温度分布的主要热源.
- 测试极光能量再分配与低大气波热的假设.
主要方法:
- 用高空间分辨率 (2度度和经度) 进行了木星的红外光谱.
- 观测覆盖了整个行星从极点到赤道.
- 数据分析的重点是绘制温度梯度和识别大规模的热结构.
主要成果:
- 发现温度从极光地区向赤道稳步下降.
- 在太阳风活动增强期间观察到高温的行星规模结构,
- 这些发现挑战了先前的模型,
结论:
- 木星的上层大气主要由极光过程中的能量再分配加热.
- 极光的能量并不完全被困在高度,
- 这项研究为木星大气中的能量转移机制提供了关键的观测证据.
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