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A Survey of Small‐Scale Waves and Wave‐Like Phenomena in Jupiter's Atmosphere Detected by JunoCam

Authors :
Stephen M. Levin
Michael Caplinger
Amy Simon
Thomas W. Momary
Candice Hansen
Fachreddin Tabataba-Vakili
Gerald Eichstädt
Glenn S. Orton
Michael H. Wong
Andrew P. Ingersoll
James Sinclair
Michael A. Ravine
Shawn Brueshaber
Hamish Nicholson
Leigh N. Fletcher
Scott Bolton
John H. Rogers
Dakota Smith
Chloe Thepenier
Abigail Anthony
Source :
Journal of Geophysical Research. Planets, Journal of Geophysical Research: Planets
Publication Year :
2020
Publisher :
American Geophysical Union (AGU), 2020.

Abstract

In the first 20 orbits of the Juno spacecraft around Jupiter, we have identified a variety of wave‐like features in images made by its public‐outreach camera, JunoCam. Because of Juno's unprecedented and repeated proximity to Jupiter's cloud tops during its close approaches, JunoCam has detected more wave structures than any previous surveys. Most of the waves appear in long wave packets, oriented east‐west and populated by narrow wave crests. Spacing between crests were measured as small as ~30 km, shorter than any previously measured. Some waves are associated with atmospheric features, but others are not ostensibly associated with any visible cloud phenomena and thus may be generated by dynamical forcing below the visible cloud tops. Some waves also appear to be converging, and others appear to be overlapping, possibly at different atmospheric levels. Another type of wave has a series of fronts that appear to be radiating outward from the center of a cyclone. Most of these waves appear within 5° of latitude from the equator, but we have detected waves covering planetocentric latitudes between 20°S and 45°N. The great majority of the waves appear in regions associated with prograde motions of the mean zonal flow. Juno was unable to measure the velocity of wave features to diagnose the wave types due to its close and rapid flybys. However, both by our own upper limits on wave motions and by analogy with previous measurements, we expect that the waves JunoCam detected near the equator are inertia‐gravity waves.<br />Key Points In the first 20 orbits of the Juno mission, over 150 waves and wave‐like features have been detected by the JunoCam public‐outreach cameraA wide variety of wave morphologies were detected over a wide latitude range, but the great majority were found near Jupiter's equatorBy analogy with previous studies of waves in Jupiter's atmosphere, most of the waves detected are likely to be inertia‐gravity waves

Details

ISSN :
21699100 and 21699097
Volume :
125
Database :
OpenAIRE
Journal :
Journal of Geophysical Research: Planets
Accession number :
edsair.doi.dedup.....c63a52ea28b3b34a01967e806307d1a1
Full Text :
https://doi.org/10.1029/2019je006369