The Global Atmospheric Circulation of Saturn

A. Showman, A. Ingersoll, R. Achterberg, Y. Kaspi
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引用次数: 16

Abstract

Over the past decade, the Cassini spacecraft has provided an unprecedented observational record of the atmosphere of Saturn, which in many ways now surpasses Jupiter as the best-observed giant planet. These observations, along with data from the Voyager spacecraft and Earth-based telescopes, demonstrate that Saturn, like Jupiter, has an atmospheric circulation dominated by zonal (east-west) jet streams, including a broad, fast eastward equatorial jet and numerous weaker jets at higher latitudes. Imaging from Voyager, Cassini, and groundbased telescopes also document a wide range of tropospheric features, including vortices, waves, turbulence, and moist convective storms. At large scales, the clouds, ammonia gas, and other chemical tracers exhibit a zonally banded pattern whose relationships to the zonal jets remains poorly understood. Infrared observations constrain the stratospheric thermal structure and allow the derivation of stratospheric temperatures; these exhibit not only the expected seasonal changes but a wealth of variations that are likely dynamical in origin and highlight dynamical coupling between the stratosphere and the underlying troposphere. In parallel to these observational developments, significant advances in theory and modeling have occurred over the past decade, especially regarding the dynamics of zonal jets, and we survey these new developments in the context of both Jupiter and Saturn. Highly idealized two-dimensional models illuminate the dynamics that give rise to zonal jets in rapidly rotating atmospheres stirred by convection or other processes, while more realistic three-dimensional models of the atmosphere and interior are starting to identify the particular conditions under which Jupiterand Saturn-like flows—including the fast equatorial superrotation, multiple jets at higher latitudes, storms, and vortices—can occur. Future data analysis and models have the potential to greatly increase our understanding over the next decade.
土星的全球大气环流
在过去的十年里,卡西尼号宇宙飞船提供了前所未有的土星大气观测记录,土星在许多方面都超过了木星,成为观测得最好的巨行星。这些观测以及旅行者号宇宙飞船和地面望远镜的数据表明,土星和木星一样,有一个由纬向(东西)喷射流主导的大气环流,包括一个宽阔、快速的东赤道喷射流和高纬度地区许多较弱的喷射流。旅行者号、卡西尼号和地面望远镜的成像也记录了对流层的各种特征,包括漩涡、波浪、湍流和潮湿的对流风暴。在大尺度上,云、氨气和其他化学示踪剂表现出带状带状的模式,其与纬向喷流的关系仍然知之甚少。红外观测约束了平流层的热结构,使平流层的温度得以推导;这些变化不仅显示了预期的季节变化,而且还显示了大量的可能源于动力的变化,并突出了平流层与底层对流层之间的动力耦合。在这些观测发展的同时,在过去的十年里,理论和建模也取得了重大进展,特别是关于纬向喷流的动力学,我们将在木星和土星的背景下调查这些新的发展。高度理想化的二维模型阐明了在对流或其他过程搅动下快速旋转的大气中产生纬向喷流的动力学,而更现实的大气和内部三维模型开始确定类似木星和土星的气流——包括快速赤道超旋转、高纬度地区的多重喷流、风暴和漩涡——可能发生的特殊条件。未来的数据分析和模型有可能在未来十年大大增加我们的理解。
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