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The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves
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| Zeitschriftentitel: | Geophysical Research Letters |
|---|---|
| Personen und Körperschaften: | , |
| In: | Geophysical Research Letters, 40, 2013, 3, S. 472-476 |
| Format: | E-Article |
| Sprache: | Englisch |
| veröffentlicht: |
American Geophysical Union (AGU)
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| Schlagwörter: |
| author_facet |
Watkins, C. Cho, J. Y‐K. Watkins, C. Cho, J. Y‐K. |
|---|---|
| author |
Watkins, C. Cho, J. Y‐K. |
| spellingShingle |
Watkins, C. Cho, J. Y‐K. Geophysical Research Letters The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves General Earth and Planetary Sciences Geophysics |
| author_sort |
watkins, c. |
| spelling |
Watkins, C. Cho, J. Y‐K. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1029/2012gl054368 <jats:p>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<jats:sup>‐1</jats:sup> 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.</jats:p> The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves Geophysical Research Letters |
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American Geophysical Union (AGU) |
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Geophysical Research Letters |
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| title |
The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_unstemmed |
The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_full |
The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_fullStr |
The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_full_unstemmed |
The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_short |
The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_sort |
the vertical structure of jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| topic |
General Earth and Planetary Sciences Geophysics |
| url |
http://dx.doi.org/10.1029/2012gl054368 |
| publishDate |
2013 |
| physical |
472-476 |
| description |
<jats:p>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<jats:sup>‐1</jats:sup> 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.</jats:p> |
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| author | Watkins, C., Cho, J. Y‐K. |
| author_facet | Watkins, C., Cho, J. Y‐K., Watkins, C., Cho, J. Y‐K. |
| author_sort | watkins, c. |
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| container_title | Geophysical Research Letters |
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| description | <jats:p>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<jats:sup>‐1</jats:sup> 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.</jats:p> |
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| spelling | Watkins, C. Cho, J. Y‐K. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1029/2012gl054368 <jats:p>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<jats:sup>‐1</jats:sup> 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.</jats:p> The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves Geophysical Research Letters |
| spellingShingle | Watkins, C., Cho, J. Y‐K., Geophysical Research Letters, The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves, General Earth and Planetary Sciences, Geophysics |
| title | The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_full | The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_fullStr | The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_full_unstemmed | The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_short | The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_sort | the vertical structure of jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| title_unstemmed | The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves |
| topic | General Earth and Planetary Sciences, Geophysics |
| url | http://dx.doi.org/10.1029/2012gl054368 |