globalchange  > 气候减缓与适应
DOI: 10.1029/2012GL054368
论文题名:
The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves
作者: Watkins C.; Cho J.Y.-K.
刊名: Geophysical Research Letters
ISSN: 0094-9315
EISSN: 1944-9046
出版年: 2013
卷: 40, 期:3
起始页码: 472
结束页码: 476
语种: 英语
英文关键词: Jupiter ; Wind ; Zonal
Scopus关键词: Gravity waves ; Probes ; Wind ; Equatorial stratosphere ; Jupiters ; Lower stratosphere ; Lower thermosphere ; Upper troposphere ; Vertical profile ; Vertical structures ; Zonal ; Upper atmosphere ; altitude ; gravity wave ; Jupiter ; planetary atmosphere ; stratosphere ; vertical profile ; vertical seismic profile ; wind velocity ; zonal wind
英文摘要: Data from the Galileo Probe, collected during its descent into Jupiter's atmosphere, is used to obtain a vertical profile of the zonal wind from ~0.5 bar (upper troposphere) to ~0.1 μbar (lower thermosphere) at the probe entry site. This is accomplished by constructing a map of gravity wave Lomb-Scargle periodograms as a function of altitude. The profile obtained from the map indicates that the wind speed above the visible cloud deck increases with height to ~150 m s-1 and then levels off at this value over a broad altitude range. The location of the turbopause, as a region of wide wave spectrum, is also identified from the map. In addition, a cross-equatorial oscillation of a jet, which has previously been linked to the QQO in the stratosphere, is suggested by the profile. Key Points Fast zonal winds of about 150 m/s exist in Jupiter's equatorial stratosphere Jupiter's equatorial turbopause is approximately 400km above the 1 bar level The jet in Jupiter's lower stratosphere may be oscillating about the equator ©2012. American Geophysical Union. All Rights Reserved.
URL: https://www.scopus.com/inward/record.uri?eid=2-s2.0-84878191399&doi=10.1029%2f2012GL054368&partnerID=40&md5=d3a758843f03467fdb88d151450896dd
Citation statistics:
资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/6579
Appears in Collections:气候减缓与适应

Files in This Item:

There are no files associated with this item.


作者单位: School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom

Recommended Citation:
Watkins C.,Cho J.Y.-K.. The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves[J]. Geophysical Research Letters,2013-01-01,40(3).
Service
Recommend this item
Sava as my favorate item
Show this item's statistics
Export Endnote File
Google Scholar
Similar articles in Google Scholar
[Watkins C.]'s Articles
[Cho J.Y.-K.]'s Articles
百度学术
Similar articles in Baidu Scholar
[Watkins C.]'s Articles
[Cho J.Y.-K.]'s Articles
CSDL cross search
Similar articles in CSDL Cross Search
[Watkins C.]‘s Articles
[Cho J.Y.-K.]‘s Articles
Related Copyright Policies
Null
收藏/分享
所有评论 (0)
暂无评论
 

Items in IR are protected by copyright, with all rights reserved, unless otherwise indicated.