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Saturn in the 21st Century最新文献

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The Global Atmospheric Circulation of Saturn 土星的全球大气环流
Pub Date : 2018-11-30 DOI: 10.1017/9781316227220.011
A. Showman, A. Ingersoll, R. Achterberg, Y. Kaspi
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.
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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引用次数: 16
Global Configuration and Seasonal Variations of Saturn’s Magnetosphere 土星磁层的全球结构和季节变化
Pub Date : 2018-11-30 DOI: 10.1017/9781316227220.006
N. Krupp, P. Kollmann, M. Thomsen, D. G. Mitchell, Xianzhe Jia, Adam Masters, Philippe Zarka
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引用次数: 3
Saturn’s Polar Atmosphere 土星的极地大气
Pub Date : 2018-11-30 DOI: 10.1017/9781316227220.012
K. Sayanagi, K. Baines, U. Dyudina, L. N. Fletcher, A. Sánchez‐Lavega, R. West
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引用次数: 2
Index 指数
Pub Date : 2018-11-30 DOI: 10.1017/9781316227220.015
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引用次数: 0
Saturn’s Seasonally Changing Atmosphere 土星季节性变化的大气层
Pub Date : 2018-11-30 DOI: 10.1017/9781316227220.010
L. N. Fletcher, T. Greathouse, S. Guerlet, J. Moses, R. West
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引用次数: 7
The Future Exploration of Saturn 未来对土星的探索
Pub Date : 2018-11-30 DOI: 10.1017/9781316227220.014
K. Baines, S. Atreya, F. Crary, S. Edgington, T. Greathouse, H. Melin, O. Mousis, G. Orton, T. Spilker, A. Wesley
Despite the lack of another Flagship-class mission like Cassini-Huygens, 1 prospects for the future exploration of Saturn are nevertheless encouraging. Both NASA 2 and the European Space Agency (ESA) are exploring the possibilities of focused 3 interplanetary missions to (1) drop one or more in-situ atmospheric entry probes into 4 Saturn and (2) explore the satellites Titan and Enceladus which would provide 5 opportunities for both in-situ investigations of Saturn's magnetosphere and detailed 6 remote-sensing observations of Saturn. Additionally, a new generation of powerful 7 Earth-based and near-Earth telescopes with advanced instrumentation spanning the ultra8 violet to the far-infrared promise to provide systematic observations of Saturn’s 9 seasonally-changing composition and thermal structure, cloud structures and wind fields. 10 Finally, new advances in amateur telescopic observations brought on largely by the 11 availability of low-cost powerful computers, low-noise, large-format cameras, and 12 attendant sophisticated software promise to provide regular observations of Saturn in 13 remarkable detail. 14 14.
尽管没有像卡西尼-惠更斯号这样的旗舰级任务,但未来探索土星的前景仍然令人鼓舞。美国宇航局和欧洲航天局(ESA)都在探索有针对性的行星际任务的可能性:(1)向土星发射一个或多个原位大气进入探测器;(2)探索土卫六和土卫二卫星,这将为对土星磁层的原位调查和对土星的详细遥感观测提供机会。此外,新一代强大的地面和近地望远镜配备了先进的仪器,从紫外到远红外,有望对土星季节性变化的组成和热结构、云结构和风场提供系统的观测。最后,业余望远镜观测的新进展主要是由于低成本、功能强大的计算机、低噪音、大画幅的照相机以及伴随而来的复杂软件的出现而带来的,这些新进展保证了对土星进行定期的、细致的观测。14日14。
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引用次数: 0
Saturn’s Variable Thermosphere 土星的可变热层
Pub Date : 2018-11-30 DOI: 10.1017/9781316227220.009
D. Strobel, T. Koskinen, I. Müller-Wodarg
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引用次数: 6
The Mysterious Periodicities of Saturn 土星的神秘周期
Pub Date : 2018-11-30 DOI: 10.1017/9781316227220.005
J. F. Carbary, M. Hedman, T. Hill, X. Jia, W. Kurth, L. Lamy, G. Provan
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引用次数: 2
Introduction to Saturn in the 21st Century 21世纪的土星简介
Pub Date : 2018-11-30 DOI: 10.1017/9781316227220.001
K. Baines, F. Flasar, N. Krupp, T. Stallard
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引用次数: 1
Saturn’s Magnetic Field and Dynamo 土星的磁场和发电机
Pub Date : 2018-11-30 DOI: 10.1017/9781316227220.004
U. Christensen
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引用次数: 2
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Saturn in the 21st Century
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