1. A Survey of Small‐Scale Waves and Wave‐Like Phenomena in Jupiter's Atmosphere Detected by JunoCam
- Author
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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, and Abigail Anthony
- Subjects
Juno ,Atmospheres ,010504 meteorology & atmospheric sciences ,Wave packet ,Equator ,Atmospheric Composition and Structure ,Forcing (mathematics) ,01 natural sciences ,Planetary Geochemistry ,Latitude ,Remote Sensing ,Atmosphere ,Jupiter ,Meteorology ,Geochemistry and Petrology ,Earth and Planetary Sciences (miscellaneous) ,waves ,Planetary Meteorology ,JunoCam ,Planetary Sciences: Solid Surface Planets ,Planetary Sciences: Fluid Planets ,Research Articles ,0105 earth and related environmental sciences ,Astronomy ,Planetary Atmospheres ,dynamics ,Jupiter Midway Through the Juno Mission ,Geochemistry ,Geophysics ,13. Climate action ,Space and Planetary Science ,Atmospheric Processes ,atmosphere ,Physics::Space Physics ,Zonal flow ,Cyclone ,Astrophysics::Earth and Planetary Astrophysics ,Geology ,Research Article - 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., 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
- Published
- 2020
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