Rogers, J. H. The Large Planet Jupiter (Cambridge Univ. Press, 1995).
Fletcher, L. N. Cycles of exercise within the Jovian ambiance. Geophys. Res. Lett. 44, 4725–4729 (2017).
Google Scholar
Stoker, C. R. Moist convection: a mechanism for producing the vertical construction of the Jovian equatorial plumes. Icarus 67, 106–125 (1986).
Google Scholar
Gierasch, P. J. et al. Commentary of moist convection in Jupiter’s ambiance. Nature 403, 628–630 (2000).
Google Scholar
Gillett, F. C., Low, F. J. & Stein, W. A. The two.8-14-micron spectrum of Jupiter. Astrophys. J. 157, 925–934 (1969).
Google Scholar
Westphal, J. A. Observations of localized 5-micron radiation from Jupiter. Astrophys. J. 157, L63–L64 (1969).
Google Scholar
Giles, R. S., Fletcher, L. N. & Irwin, P. G. J. Cloud construction and composition of Jupiter’s troposphere from 5-μm Cassini VIMS spectroscopy. Icarus 257, 457–470 (2015).
Google Scholar
Bjoraker, G. L., Wong, M. H., de Pater, I. & Ádámkovics, M. Jupiter’s deep cloud construction revealed utilizing Keck observations of spectrally resolved line shapes. Astrophys. J. 810, 122 (2015).
Google Scholar
West, R. A. et al. in Jupiter: The Planet, Satellites and Magnetosphere (eds Bagenal, F., Dowling, T. E. & McKinnon, W. B.) 79–104 (Cambridge Univ. Press, 2004).
Antuñano, A. et al. Infrared characterization of Jupiter’s equatorial disturbance cycle. Geophys. Res. Lett. 45, 10987–10995 (2018).
Google Scholar
Antuñano, A. et al. Jupiter’s atmospheric variability from long-term ground-based observations at 5 μm. Astron. J. 158, 130 (2019).
Google Scholar
Braginsky, S. I. Torsional magnetohydrodynamic vibrations within the Earth’s core and variations in day size. Geomag. Aeron. 10, 3–12 (1970).
Hori, Okay., Teed, R. J. & Jones, C. A. Anelastic torsional oscillations in Jupiter’s metallic hydrogen area. Earth Planet. Sci. Lett. 519, 50–60 (2019).
Google Scholar
Connerney, J. E. P. et al. A brand new mannequin of Jupiter’s magnetic discipline on the completion of Juno’s prime mission. J. Geophys. Res. Planets 127, e2021JE007055 (2022).
Google Scholar
French, M. et al. Ab initio simulations for materials properties alongside the Jupiter adiabat. Astrophys. J. Suppl. Ser. 202, 5 (2012).
Google Scholar
Tsang, Y.-Okay. & Jones, C. A. Characterising Jupiter’s dynamo radius utilizing its magnetic vitality spectrum. Earth Planet. Sci. Lett. 530, 115879 (2020).
Moore, Okay. M. et al. A fancy dynamo inferred from the hemispheric dichotomy of Jupiter’s magnetic discipline. Nature 561, 76–78 (2018).
Google Scholar
Teed, R. J., Jones, C. A. & Tobias, S. M. The transition to Earth-like torsional oscillations in magnetoconvection simulations. Earth Planet. Sci. Lett. 419, 22–31 (2015).
Google Scholar
Tollefson, J. et al. Adjustments in Jupiter’s zonal wind profile previous and through the Juno mission. Icarus 296, 163–178 (2017).
Google Scholar
Wong, M. H. et al. Excessive-resolution UV/optical/IR imaging of Jupiter in 2016–2019. Astrophys. J. Suppl. Ser. 247, 58 (2020).
Google Scholar
Kaspi, Y. et al. Jupiter’s atmospheric jet streams prolong 1000’s of kilometres deep. Nature 555, 223–226 (2018).
Google Scholar
Galanti, E. & Kaspi, Y. Mixed magnetic and gravity measurements probe the deep zonal flows of the gasoline giants. Mon. Not. R. Astron. Soc. 501, 2352–2362 (2021).
Google Scholar
Moore, Okay. M. et al. Time variation of Jupiter’s inner magnetic discipline according to zonal wind advection. Nat. Astron. 3, 730–735 (2019).
Google Scholar
Bloxham, J. et al. Differential rotation in Jupiter’s inside revealed by simultaneous inversion for the magnetic discipline and zonal flux velocity. J. Geophys. Res. Planets 127, e2021JE007138 (2022).
Google Scholar
Jin, T.-C., Wu, J.-Z., Zhang, Y.-Z., Liu, Y.-L. & Zhou, Q. Shear-induced modulation of convection over tough plates. J. Fluid Mech. 936, A28 (2022).
Google Scholar
Showman, A. P., Kaspi, Y. & Flierl, G. R. Scaling legal guidelines for convection and jet speeds in large planets. Icarus 211, 1258–1273 (2011).
Google Scholar
Aurnou, J. M., Horn, S. & Julien, Okay. Connections between nonrotating, slowly rotating, and quickly rotating turbulent convective transport scalings. Phys. Rev. Res 2, 043115 (2015).
Hueso, R. & Sánchez-Lavega, A. A 3-dimensional mannequin of moist convection for the enormous planets: the Jupiter case. Icarus 151, 257–274 (2001).
Google Scholar
Sugiyama, Okay. et al. Intermittent cumulonimbus exercise breaking the three-layer cloud construction of Jupiter. Geophys. Res. Lett. 38, L13201 (2011).
Google Scholar
Debras, F. & Chabrier, G. New fashions of Jupiter within the context of Juno and Galileo. Astrophys. J. 872, 100 (2019).
Google Scholar
Gastine, T. & Wicht, J. Secure stratification promotes a number of zonal jets in a turbulent Jovian dynamo mannequin. Icarus 368, 114514 (2021).
Orton, G. S. et al. Surprising long-term variability in Jupiter’s tropospheric temperatures. Nat. Astron. 7, 190–197 (2023).
Google Scholar
Schmid, P. J. Dynamic mode decomposition of numerical and experimental information. J. Fluid Mech. 656, 5–28 (2010).
Google Scholar
Rowley, C. W., Mezić, I., Bagheri, S., Schlatter, P. & Henningson, D. S. Spectral evaluation of nonlinear flows. J. Fluid Mech. 641, 115–127 (2009).
Google Scholar
Tu, J. H., Rowley, C. W. & Luchtenburg, D. M. On dynamic mode decomposition: principle and purposes. J. Comput. Dyn. 1, 391–421 (2014).
Google Scholar
Kutz, J. N., Brunton, S. L., Brunton, B. W. & Proctor, J. L. Dynamic Mode Decomposition: Knowledge-Pushed Modeling of Complicated Methods (SIAM, 2016).
Gillet, N., Jault, D., Canet, E. & Fournier, A. Quick torsional waves and robust magnetic discipline inside the Earth’s core. Nature 465, 74–77 (2010).
Google Scholar
Higgins, C. A., Carr, T. D. & Reyes, F. A brand new dedication of Jupiter’s radio rotation interval. Geophys. Res. Lett. 23, 2653–2656 (1996).
Google Scholar
Gaulme, P., Schmider, F.-X., Homosexual, J., Guillot, T. & Jacob, C. Detection of Jovian seismic waves: a brand new probe of its inside construction. Astron. Astrophys. 531, A104 (2011).
Glatzmaier, G. A. Laptop simulations of Jupiter’s deep inner dynamics assist interpret what Juno sees. Proc. Nat. Acad. Sci. 115, 6896–6904 (2018).
Google Scholar
Wahl, S. M. et al. Evaluating Jupiter inside construction fashions to Juno gravity measurements and the function of a dilute core. Geophys. Res. Lett. 44, 4649–4659 (2017).
Google Scholar
Stevenson, D. J. Jupiter’s inside as revealed by Juno. Annu. Rev. Earth Planet. Sci. 48, 465–489 (2020).
Google Scholar
Pontin, C. M., Barker, A. J., Hollerbach, R., André, Q. & Mathis, S. Wave propagation in semiconvective areas of large planets. Mon. Not. R. Astron. Soc. 493, 5788–5806 (2020).
Google Scholar
Roberts, P. H. & Aurnou, J. M. On the idea of core-mantle coupling. Geophys. Astrophys. Fluid Dyn. 106, 157–230 (2012).
Google Scholar
Connerney, J. E. P. et al. A brand new mannequin of Jupiter’s magnetic discipline from Juno’s first 9 orbits. Geophys. Res. Lett. 45, 2590–2596 (2018).
Google Scholar
Scargle, J. D. Research in astronomical time collection evaluation. II. Statistical features of spectral evaluation of erratically spaced information. Astrophys. J 263, 835–853 (1982).
Google Scholar
Avila, A. M. & Mezić, I. Knowledge-driven evaluation and forecasting o f freeway site visitors dynamics. Nat. Commun. 11, 2090 (2020).
Google Scholar
Hori, Okay., Tobias, S. M. & Teed, R. J. Dynamic mode decomposition to retrieve torsional Alfvén waves. In Proceedings of the Japan Society of Fluid Mechanics Annual Assembly 2020. Preprint at https://doi.org/10.48550/arXiv.2009.13095 (2020).
Jovanović, M. R., Schmid, P. J. & Nichols, J. W. Sparsity-promoting dynamic mode decomposition. Phys. Fluids 26, 024103 (2014).
Google Scholar
Gavish, M. & Donoho, D. L. The optimum onerous threshold for singular values is (4/sqrt{3}). IEEE Trans. Inf. Concept 60, 5040–5053 (2014).
Gillet, N., Jault, D. & Canet, E. Excitation of travelling torsional regular modes in an Earth’s core mannequin. Geophys. J. Int. 210, 1503–1516 (2017).
Google Scholar