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土星上的一场巨型雷暴。

A giant thunderstorm on Saturn.

机构信息

Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6, A-8042 Graz, Austria.

出版信息

Nature. 2011 Jul 6;475(7354):75-7. doi: 10.1038/nature10205.

DOI:10.1038/nature10205
PMID:21734705
Abstract

Lightning discharges in Saturn's atmosphere emit radio waves with intensities about 10,000 times stronger than those of their terrestrial counterparts. These radio waves are the characteristic features of lightning from thunderstorms on Saturn, which last for days to months. Convective storms about 2,000 kilometres in size have been observed in recent years at planetocentric latitude 35° south (corresponding to a planetographic latitude of 41° south). Here we report observations of a giant thunderstorm at planetocentric latitude 35° north that reached a latitudinal extension of 10,000 kilometres-comparable in size to a 'Great White Spot'-about three weeks after it started in early December 2010. The visible plume consists of high-altitude clouds that overshoot the outermost ammonia cloud layer owing to strong vertical convection, as is typical for thunderstorms. The flash rates of this storm are about an order of magnitude higher than previous ones, and peak rates larger than ten per second were recorded. This main storm developed an elongated eastward tail with additional but weaker storm cells that wrapped around the whole planet by February 2011. Unlike storms on Earth, the total power of this storm is comparable to Saturn's total emitted power. The appearance of such storms in the northern hemisphere could be related to the change of seasons, given that Saturn experienced vernal equinox in August 2009.

摘要

土星大气层中的闪电释放出的无线电波强度比其在地球上的对应物强约 10000 倍。这些无线电波是土星雷暴闪电的特征,其持续时间为数天到数月。近年来,在行星对地纬度 35°的南部(相当于行星纬度 41°的南部)观测到了大小约为 2000 公里的对流风暴。在这里,我们报告了在行星对地纬度 35°的北部观测到的一场巨型雷暴的情况,这场雷暴始于 2010 年 12 月初,大约三周后,其南北向的延伸达到了 10000 公里——大小与一个“大白斑”相当。可见羽流由高空云层组成,由于强烈的垂直对流,云层超出了最外层氨云层,这是雷暴的典型特征。这场风暴的闪光率比以前的风暴高一个数量级,记录到的峰值率大于每秒 10 次。这场主要风暴向东延伸出一条长长的尾巴,还有额外的但较弱的风暴细胞,到 2011 年 2 月,这些风暴细胞已经环绕了整个星球。与地球上的风暴不同,这场风暴的总功率与土星的总发射功率相当。鉴于土星在 2009 年 8 月经历了春分,这种风暴出现在北半球可能与季节变化有关。

相似文献

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A giant thunderstorm on Saturn.土星上的一场巨型雷暴。
Nature. 2011 Jul 6;475(7354):75-7. doi: 10.1038/nature10205.
2
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Long-lasting, deep effect of Saturn's giant storms.土星巨大风暴的持久深远影响。

本文引用的文献

1
Deep winds beneath Saturn's upper clouds from a seasonal long-lived planetary-scale storm.土星高层云下的深层风来自一场季节性的、长期存在的行星尺度风暴。
Nature. 2011 Jul 6;475(7354):71-4. doi: 10.1038/nature10203.
2
Planetary radio astronomy observations from voyager 1 near saturn.旅行者 1 号在土星附近进行的行星射电天文学观测。
Science. 1981 Apr 10;212(4491):239-43. doi: 10.1126/science.212.4491.239.
3
Cassini Imaging Science: initial results on Saturn's atmosphere.卡西尼号成像科学:土星大气的初步结果。
Sci Adv. 2023 Aug 11;9(32):eadg9419. doi: 10.1126/sciadv.adg9419.
4
Cassini Exploration of the Planet Saturn: A Comprehensive Review.卡西尼号对土星的探测:全面综述
Space Sci Rev. 2020;216:122. doi: 10.1007/s11214-020-00751-1. Epub 2020 Oct 26.
5
How Well Do We Understand the Belt/Zone Circulation of Giant Planet Atmospheres?我们对巨行星大气的纬向条带环流了解多少?
Space Sci Rev. 2020;216(2):30. doi: 10.1007/s11214-019-0631-9. Epub 2020 Mar 12.
6
Evolution of Stratospheric Chemistry in the Saturn Storm Beacon Region.土星风暴信标区域平流层化学的演变
Icarus. 2015 Nov 15;261:149-168. doi: 10.1016/j.icarus.2015.08.012. Epub 2015 Aug 14.
7
Vortices in Saturn's Northern Hemisphere (2008-2015) Observed by Cassini ISS.卡西尼号成像科学子系统观测到的土星北半球的涡旋(2008 - 2015年)
J Geophys Res Planets. 2016 Sep;121(9):1814-1826. doi: 10.1002/2016JE005122. Epub 2016 Sep 8.
8
Deep winds beneath Saturn's upper clouds from a seasonal long-lived planetary-scale storm.土星高层云下的深层风来自一场季节性的、长期存在的行星尺度风暴。
Nature. 2011 Jul 6;475(7354):71-4. doi: 10.1038/nature10203.
9
Saturn: storm-clouds brooding on towering heights.土星:高耸云端、孕育着风暴的云团。
Nature. 2011 Jul 6;475(7354):44-5. doi: 10.1038/475044a.
Science. 2005 Feb 25;307(5713):1243-7. doi: 10.1126/science.1107691.