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Journal article

An intense narrow equatorial jet in Jupiter's lower stratosphere observed by JWST

Abstract:

The atmosphere of Jupiter has east–west zonal jets that alternate as a function of latitude as tracked by cloud motions at tropospheric levels. Above and below the cold tropopause at ~100 mbar, the equatorial atmosphere is covered by hazes at levels where thermal infrared observations used to characterize the dynamics of the stratosphere lose part of their sensitivity. James Webb Space Telescope observations of Jupiter in July 2022 show these hazes in higher detail than ever before and reveal the presence of an intense (140 m s−1) equatorial jet at 100–200 mbar (70 m s−1 faster than the zonal winds at the cloud level) that is confined to ±3° of the equator and is located below stratospheric thermal oscillations that extend at least from 0.1 to 40 mbar and repeat in multiyear cycles. This suggests that the new jet is a deep part of Jupiter’s Equatorial Stratospheric Oscillation and may therefore vary in strength over time.

Publication status:
Published
Peer review status:
Peer reviewed

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Files:
Publisher copy:
10.1038/s41550-023-02099-2

Authors



Publisher:
Springer Nature
Journal:
Nature Astronomy More from this journal
Publication date:
2023-10-19
Acceptance date:
2023-09-11
DOI:
EISSN:
2397-3366


Language:
English
Keywords:
Pubs id:
1556052
Local pid:
pubs:1556052
Deposit date:
2023-11-29

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