Journal article
Wave activity in Jupiter's North Equatorial Belt from near‐infrared reflectivity observations
- Abstract:
- High spatial resolution images of Jupiter at 1.58–2.28 μm are used to track and characterize a wave pattern observed in 2017 at a planetocentric latitude of 14°N. The wave pattern has a wave number of 18 and spans ∼5° in latitude. One bright crest remains stationary in System III longitude, while the remaining crests move slowly westward. The bright and dark regions of the near‐infrared wave pattern are caused by variations in the vertical location of the upper tropospheric haze layer. A comparison with thermal infrared observations shows a correlation with temperature anomalies in the upper troposphere. The results are consistent with a Rossby wave, generated by flow around a stationary vortex.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 2.5MB, Terms of use)
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(Preview, Version of record, pdf, 5.1MB, Terms of use)
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- Publisher copy:
- 10.1029/2018gl081858
Authors
- Publisher:
- American Geophysical Union
- Journal:
- Geophysical Research Letters More from this journal
- Volume:
- 46
- Issue:
- 3
- Pages:
- 1232-1241
- Publication date:
- 2019-02-13
- Acceptance date:
- 2019-02-05
- DOI:
- EISSN:
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1944-8007
- ISSN:
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0094-8276
- Language:
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English
- Pubs id:
-
pubs:976405
- UUID:
-
uuid:c74e95c1-e0be-43c7-a9bd-b611d916db81
- Local pid:
-
pubs:976405
- Source identifiers:
-
976405
- Deposit date:
-
2019-02-26
Terms of use
- Copyright holder:
- American Geophysical Union
- Copyright date:
- 2019
- Notes:
- Copyright © 2019 American Geophysical Union.
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