2021
DOI: 10.1029/2021gl094235
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Oscillations and Stability of the Jupiter Polar Cyclones

Abstract: Juno performed 4 year of observations of the Jupiter polar cyclones. We discuss implications for their stability and vertical structure The cyclones have similar intrinsic oscillation frequencies, and perturbations seem to propagate from one cyclone to the closer one.Cyclones are extremely stable, individually and as a whole; they slowly spin and the South one is twice as fast as the North one

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Cited by 12 publications
(44 citation statements)
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References 27 publications
(59 reference statements)
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“…A finite deformation radius complicates our model because the conversion between kinetic and potential energies resulting from finite implies that the initial root-mean-square velocity, U defined in [ 5 ], is not constant during the evolution. We take comfort in recent observations and numerical results ( 3 , 14 , 39 , 40 ) indicating that polar cyclones might have a strong barotropic component.…”
Section: Discussionsupporting
confidence: 80%
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“…A finite deformation radius complicates our model because the conversion between kinetic and potential energies resulting from finite implies that the initial root-mean-square velocity, U defined in [ 5 ], is not constant during the evolution. We take comfort in recent observations and numerical results ( 3 , 14 , 39 , 40 ) indicating that polar cyclones might have a strong barotropic component.…”
Section: Discussionsupporting
confidence: 80%
“…Once the permanent central cyclone is established, the octet crystallizes into solid-body rotation ( Movie S3 ). The solid-body rotation is not perfect: Vortices have small epicyclic oscillations about their mean position, reminiscent of the oscillations of the cyclones about their mean position at the South Pole of Jupiter ( 3 , 4 ). The oscillations may result from differences in strength between the eight cyclones; e.g., the smallest cyclones have the largest excursions.…”
Section: Results: the Polar Capmentioning
confidence: 99%
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“…The locations of the CPCs have been monitored since Juno's arrival at Jupiter (Adriani et al., 2020; Mura et al., 2021; Tabataba‐Vakili et al., 2020). While the average locations of the cyclones match the calculations of Gavriel and Kaspi (2021) (hereafter GK21), the individual cyclones were found to oscillate around these stable positions, where perturbations seem to pass on between neighboring cyclones (Mura et al., 2021). In addition, an average westward drift of approximately 7.5° (3°) per year was measured on the cyclones at the south (north) pole (Adriani et al., 2020; Mura et al., 2021).…”
Section: Introductionmentioning
confidence: 99%
“…The general structure of the polar cyclones is maintained along the PJ passages: the pentagon of circumpolar cyclones is always present, although the entire structure rotated from PJ 4 until the more recent orbits of Juno spacecraft (Mura et al, 2021) and the angular distance between CPC 1 and CPC 5 widened during PJ 33.…”
Section: Accepted Articlementioning
confidence: 99%