The DOI matches its Crossref record; 66 of the 69 references it cites were found in a registry or an index.
Atmospheric Dynamics of the Outer Planets
Abstract
Despite major differences in the solar and internal energy inputs, the atmospheres of the four Jovian planets all exhibit latitudinal banding and high-speed jet streams. Neptune and Saturn are the windiest planets, Jupiter is the most active, and Uranus is a tipped-over version of the others. Large oval storm systems exhibit complicated time-dependent behavior that can be simulated in numerical models and laboratory experiments. The largest storm system, the Great Red Spot of Jupiter, has survived for more than 300 years in a chaotic shear zone where smaller structures appear and dissipate every few days. Future space missions will add to our understanding of small-scale processes, chemical composition, and vertical structure. Theoretical hypotheses about the interiors provide input for fluid dynamical models that reproduce many observed features of the winds, temperatures, and cloud patterns. In one set of models the winds are confined to the thin layer where clouds form. In other models, the winds extend deep into the planetary fluid interiors. Hypotheses will be tested further as observations and theories become more exact and detailed comparisons are made.
Overview
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
In the citing paper
“In the Uranus and Neptune simulations, the equator-to-pole brightness temperature contrasts are 8 and 2 K, respectively, consistent with observations (Ingersoll 1990).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Ingersoll 1990
In the citing paper
“In the Saturn simulation, the equator-topole brightness temperature contrast is 7 K, consistent with observations (Ingersoll 1990;Fletcher et al. 2007).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Ingersoll 1990
In the citing paper
“In the Jupiter simulation, the equator-to-pole contrast in the brightness temperature of thermal radiation is 10 K, which is similar to, albeit larger than, the observed brightness temperature contrast or the observed temperature contrast near the emission level (Ingersoll et al. 1976;Ingersoll 1990;Ingersoll et al. 2004;Simon-Miller et al. 2006).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Ingersoll 1990
In the citing paper
“Variations in brightness temperature gradients off the equator may be weaker in the Jupiter and Saturn simulations than they are in observations, at least at some wavelengths(Ingersoll 1990; Ingersoll et al. 2004).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Ingersoll 1990
In the citing paper
“The thermal optical depths t l0 at pressure p 0 are chosen such that the observed thermal emission levels (e.g., Ingersoll 1990) of the giant planets approximately correspond to t l 5 1.”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Ingersoll 1990
Citations
Cites
Pedlosky, J. (1987) · Springer eBooks · doi:10.1007/978-1-4612-4650-3 · Cited by 3,453
The effect of solar radiation variations on the climate of the Earth
BUDYKO, M. I. (1969) · Tellus · doi:10.1111/j.2153-3490.1969.tb00466.x · Cited by 1,436
The effect of solar radiation variations on the climate of the Earth
Budyko, M. I. (1969) · Tellus A Dynamic Meteorology and Oceanography · doi:10.3402/tellusa.v21i5.10109 · Cited by 1,039
Battisti, D. S., & Hirst, A. C. (1989) · Journal of the Atmospheric Sciences · doi:10.1175/1520-0469(1989)046 · Cited by 906
A New Look at the Saturn System: The Voyager 2 Images
Smith, B. A., Soderblom, L., Batson, R., Bridges, P., Inge, J., Masursky, H., Shoemaker, E., Beebe, R., Boyce, J., Briggs, G., et al. (1982) · Science · doi:10.1126/science.215.4532.504 · Cited by 848
Self-citationEncounter with Saturn: Voyager 1 imaging science results
Smith, B. A., Soderblom, L., Beebe, R., Boyce, J., Briggs, G., Bunker, A., Collins, S. A., Hansen, C. J., Johnson, T. V., Mitchell, J. L., et al. (1981) · Science · doi:10.1126/science.212.4491.163 · Cited by 795
The Jupiter System Through the Eyes of Voyager 1
Smith, B. A., Soderblom, L. A., Johnson, T. V., Ingersoll, A. P., Collins, S. A., Shoemaker, E. M., Hunt, G. E., Masursky, H., Carr, M. H., Davies, M. E., et al. (1979) · Science · doi:10.1126/science.204.4396.951 · Cited by 781
The Maximum Intensity of Hurricanes
Emanuel, K. (1988) · Journal of the Atmospheric Sciences · doi:10.1175/1520-0469(1988)045 · Cited by 773
Moura, A. D., & Shukla, J. (1981) · Journal of the Atmospheric Sciences · doi:10.1175/1520-0469(1981)038 · Cited by 733
Voyager 2 at Neptune: Imaging Science Results
Smith, B. A., Soderblom, L. A., Banfield, D., Barnet, C. D., Basilevsky, A. T., Beebe, R. F., Bollinger, K., Boyce, J. M., Brahic, A., Briggs, G. A., et al. (1989) · Science · doi:10.1126/science.246.4936.1422 · Cited by 618
Flagged first, then by citations
3 of the 69 references couldn’t be matched to a known paper.
Research works printed but not linked: 12
- CONNERNEY, JEP, SATURN: 354 (1984).
- DOWLING, T.E., JUPITERS GREAT RED SPOT AS A SHALLOW-WATER SYSTEM, JOURNAL OF THE ATMOSPHERIC SCIENCES 46: 3256 (1989). · DOI
- HESS, S.L., COMPENDIUM METEOROLO: 391 (1951).
- INGERSOLL, A.P., JUPITER: 197 (1976).
- INGERSOLL, A.P., SATURN: 195 (1984).
- KAISER, M.L., SATURN: 378 (1984).
- PRINN, R.G., SATURN: 88 (1984).
- SROMOVSKY, L.A., JOVIAN WINDS FROM VOYAGER-2 .2. ANALYSIS OF EDDY TRANSPORTS, JOURNAL OF THE ATMOSPHERIC SCIENCES 39: 1433 (1982). · DOI
- TERRILE, R.J., ICARUS 30: 247 (1977).
- TOMASKO, M.G., SATURN: 150 (1984).
- WILLIAMS, G.P., THE STABILITY AND GENESIS OF ROSSBY VORTICES, JOURNAL OF THE ATMOSPHERIC SCIENCES 45: 207 (1988). · DOI
- Williams, G. P., Nature 257:778 (1975).
Cited by
Sorted by citations
Schou, J., Antia, H. M., Basu, S., Bogart, R. S., Bush, R. I., Chitre, S. M., Christensen-Dalsgaard, J., Mauro, M. P. D., Dziembowski, W. A., Eff‐Darwich, A., et al. (1998) · The Astrophysical Journal · doi:10.1086/306146 · Cited by 998
Porco, C., West, R., Squyres, S., McEwen, A., Thomas, P., Murray, C., Delgenio, A., Ingersoll, A., Johnson, T., Neukum, G., et al. (2004) · Space Science Reviews · doi:10.1007/s11214-004-1456-7 · Cited by 402
“By creating movies of the Saturn atmosphere in motion, we can observe the life cycle of vortices as they merge, split, or oscillate (Ingersoll, 1990; Polvani et al., 1990; Li et al., 2004; see movies of the Jupiter atmosphere at http://ciclops.org).”
MethodJovian atmospheric dynamics: an update after Galileo and Cassini
Vasavada, A. R., & Showman, A. P. (2005) · Reports on Progress in Physics · doi:10.1088/0034-4885/68/8/r06 · Cited by 329
TRANSPORT BY COHERENT BAROTROPIC VORTICES
Provenzale, A. (1999) · Annual Review of Fluid Mechanics · doi:10.1146/annurev.fluid.31.1.55 · Cited by 325
“as the Great Red Spot on Jupiter (e.g. Ingersoll 1990, Dowling 1995), dark and bright star spots where rotation and magnetic fields both play a role (Dowling & Spiegel 1990), and perhaps vortex spots on astrophysical disks (Abramowicz et al 1991, Bracco et al 1998).”
BackgroundSimulation of equatorial and high-latitude jets on Jupiter in a deep convection model
Heimpel, M., Aurnou, J., & Wicht, J. (2005) · Nature · doi:10.1038/nature04208 · Cited by 291
Rapidly rotating turbulent Rayleigh-Bénard convection
Julien, K. A., Legg, S. A., McWilliams, J. C., & Werne, J. A. (1996) · Journal of Fluid Mechanics · doi:10.1017/s0022112096002789 · Cited by 268
Statistical mechanics, Euler’s equation, and Jupiter’s Red Spot
Miller, J., Weichman, P. B., & Cross, M. C. (1992) · Physical Review A · doi:10.1103/physreva.45.2328 · Cited by 242
The emergence of jets and vortices in freely evolving, shallow-water turbulence on a sphere
Cho, J. Y., & Polvani, L. M. (1996) · Physics of Fluids · doi:10.1063/1.868929 · Cited by 235
Observation of moist convection in Jupiter's atmosphere
Gierasch, P. J., Ingersoll, A. P., Banfield, D., Ewald, S. P., Helfenstein, P., Simon, A. A., Vasavada, A. R., Breneman, H. H., Senske, D. A., & Galileo Imaging Team (2000) · Nature · doi:10.1038/35001017 · Cited by 212
“jpg" NDATA ITEM> ]> The energy source driving Jupiter's active meteorology is not understoo”
The Changing Face of the Extrasolar Giant Planet HD 209458b
Cho, J. Y., Kristen Menou, A., Hansen, B. M. S., & Seager, S. (2003) · The Astrophysical Journal · doi:10.1086/375016 · Cited by 204
“Generally,1/2(K gH) /f R p is required for a Jupiter-like multiple-jet circulationL /R K 1D p pattern without pronounced polar vortices at the cloud-top.”
BackgroundInfluentialConstraints on deep seated zonal winds inside Jupiter and Saturn.
LIU, J., GOLDREICH, P., & STEVENSON, D. (2008) · Icarus · doi:10.1016/j.icarus.2007.11.036 · Cited by 208
Formation of Jets and Equatorial Superrotation on Jupiter
Schneider, T., & Liu, J. (2008) · Journal of the Atmospheric Sciences · doi:10.1175/2008jas2798.1 · Cited by 169
Galileo's First Images of Jupiter and the Galilean Satellites
Belton, M. J. S., Head, J. W., III, Ingersoll, A. P., Greeley, R., McEwen, A. S., Klaasen, K. P., Senske, D. A., Pappalardo, R. T., Collins, G. C., Vasavada, A. R., et al. (1996) · Science · doi:10.1126/science.274.5286.377 · Cited by 161
ATMOSPHERIC DYNAMICS OF BROWN DWARFS AND DIRECTLY IMAGED GIANT PLANETS
Showman, A. P., & Kaspi, Y. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/776/2/85 · Cited by 153
“…wind speeds measured for the giant planets in the solar system, which range from typical speeds of ∼30 m s−1 on Jupiter to ∼300 m s−1 on Neptune (e.g., Ingersoll 1990).5 Later, we show that the large-scale winds in the convective interior of a brown dwarf are likely to be weak (Section 3.3), but…”
BackgroundInfluentialThe deep wind structure of the giant planets: Results from an anelastic general circulation model
Kaspi, Y., Flierl, G. R., & Showman, A. P. (2009) · Icarus · doi:10.1016/j.icarus.2009.03.026 · Cited by 149
Structure and Spacing of Jets in Barotropic Turbulence
Farrell, B. F., & Ioannou, P. J. (2007) · Journal of the Atmospheric Sciences · doi:10.1175/jas4016.1 · Cited by 149
Vortices in Protoplanetary Disks
Godon, P., & Livio, M. (1999) · The Astrophysical Journal · doi:10.1086/307720 · Cited by 145
“It is believed, for example, that the Great Red Spot in the atmosphere of Jupiter is a steady solitary vortex also sustained by the merging of small vortices (Marcus 1993 ; see also Ingersoll 1990).”
BackgroundKumar, A., Minnett, P. J., Podestá, G., & Evans, R. H. (2003) · Journal of the Atmospheric Sciences · doi:10.1175/1520-0469(2003)060 · Cited by 44
The Morphogenesis of Bands and Zonal Winds in the Atmospheres on the Giant Outer Planets
Cho, J. Y.-K., & Polvani, L. M. (1996) · Science · doi:10.1126/science.273.5273.335 · Cited by 131
Inviscid damping of asymmetries on a two-dimensional vortex
Schecter, D. A., Dubin, D. H. E., Cass, A. C., Driscoll, C. F., Lansky, I. M., & O’Neil, T. M. (2000) · Physics of Fluids · doi:10.1063/1.1289505 · Cited by 127
Vortex crystals from 2D Euler flow: Experiment and simulation
Schecter, D. A., Dubin, D. H. E., Fine, K. S., & Driscoll, C. F. (1999) · Physics of Fluids · doi:10.1063/1.869961 · Cited by 125
Temperature and Composition of Saturn's Polar Hot Spots and Hexagon
Fletcher, L. N., Irwin, P. G. J., Orton, G. S., Teanby, N. A., Achterberg, R. K., Bjoraker, G. L., Read, P. L., Simon-Miller, A. A., Howett, C., de Kok, R., et al. (2008) · Science · doi:10.1126/science.1149514 · Cited by 125
Zonal flow regimes in rotating anelastic spherical shells: An application to giant planets
Gastine, T., Wicht, J., & Aurnou, J. M. (2013) · Icarus · doi:10.1016/j.icarus.2013.02.031 · Cited by 118
“Uranus interior, Neptune interior 1. Introduction Surface zonal jets on the giant planets Jupiter, Saturn, Uranus and Neptune have been investigated since the 1970’s by tracking cloud features (e.g. Ingersoll, 1990). On each planet, these zonal winds form a differential rotation profile with alternating prograde (i.e. e…”
BackgroundZonal flow driven by deep convection in the major planets
Christensen, U. R. (2001) · Geophysical Research Letters · doi:10.1029/2000gl012643 · Cited by 123
Mechanisms of Jet Formation on the Giant Planets
Liu, J., & Schneider, T. (2010) · Journal of the Atmospheric Sciences · doi:10.1175/2010jas3492.1 · Cited by 135
“…observed temperature contrast near the emission level (Ingersoll et al. 1976; Ingersoll 1990; Ingersoll et al. 2004; Simon-Miller et al. 2006).4 In the Saturn simulation, the equator-topole brightness temperature contrast is 7 K, consistent with observations (Ingersoll 1990; Fletcher et al. 2007).”
BackgroundMethodResultInfluentialTurbulence theories and statistical closure approaches
Zhou, Y. (2021) · Physics Reports · doi:10.1016/j.physrep.2021.07.001 · Cited by 126
Less absorbed solar energy and more internal heat for Jupiter
Li, L., Jiang, X., West, R. A., Gierasch, P. J., Pérez-Hoyos, S., Sánchez-Lavega, A., Fletcher, L. N., Fortney, J. J., Knowles, B., Porco, C. C., et al. (2018) · Nature Communications · doi:10.1038/s41467-018-06107-2 · Cited by 110
The effects of vigorous mixing in a convective model of zonal flow on the ice giants.
Aurnou, J., Heimpel, M., & Wicht, J. (2007) · Icarus · doi:10.1016/j.icarus.2007.02.024 · Cited by 107
Uranus and Neptune: Shape and rotation
Helled, R., Anderson, J. D., & Schubert, G. (2010) · Icarus · doi:10.1016/j.icarus.2010.06.037 · Cited by 99
Abramowicz, M. A., Lanza, A., Spiegel, E. A., & Szuszkiewicz, E. (1992) · Nature · doi:10.1038/356041a0 · Cited by 93
Atmospheric Circulation of ExoplanetsPreprint
Showman, A. P., Cho, J. Y. K., & Kristen Menou, A. (2009) · arXiv (Cornell University) · doi:10.48550/arxiv.0911.3170 · Cited by 113
A strong decrease in Saturn's equatorial jet at cloud level
Sánchez-Lavega, A., Pérez-Hoyos, S., Rojas, J. F., Hueso, R., & French, R. G. (2003) · Nature · doi:10.1038/nature01653 · Cited by 78
Vortex merging in quasi-geostrophic flows
von Hardenberg, J., McWilliams, J. C., Provenzale, A., Shchepetkin, A. F., & Weiss, J. B. (2000) · Journal of Fluid Mechanics · doi:10.1017/s0022112000008442 · Cited by 78
The geostrophic regime of rapidly rotating turbulent convection
Kunnen, R. (2021) · Journal of Turbulence · doi:10.1080/14685248.2021.1876877 · Cited by 71
“Moving away from our own planet, further examples are found in the giant gas planets with their characteristic zonal flows [8,9].”
BackgroundDynamical properties of vortical structures on the beta-plane
Sutyrin, G. G., Hesthaven, J. S., Lynov, J.-P., & Rasmussen, J. J. (1994) · Journal of Fluid Mechanics · doi:10.1017/s002211209400128x · Cited by 69
Formation of Jets by Baroclinic Instability on Gas Planet Atmospheres
Kaspi, Y., & Flierl, G. R. (2007) · Journal of the Atmospheric Sciences · doi:10.1175/jas4009.1 · Cited by 60
Perryman, M. A. C. (2011) · Cambridge University Press eBooks · doi:10.1017/cbo9780511994852.011 · Cited by 71
Spiga, A., Guerlet, S., Millour, E., Indurain, M., Meurdesoif, Y., Cabanes, S., Dubos, T., Leconte, J., Boissinot, A., Lebonnois, S., et al. (2019) · Icarus · doi:10.1016/j.icarus.2019.07.011 · Cited by 55
“between Jupiter and Saturn in their banded jets (Ingersoll, 1990; Dowling, 1995; Kaspi et al., 2018), eddy activity (Salyk et al.”
InfluentialThe Galileo probe mission to Jupiter: Science overview
Young, R. E. (1998) · Journal of Geophysical Research Atmospheres · doi:10.1029/98je01051 · Cited by 58
The Galileo Probe: How it Has Changed Our Understanding of Jupiter
Young, R. (2003) · New Astronomy Reviews · doi:10.1016/s1387-6473(02)00272-5 · Cited by 60
Observations of zonal flow created by potential vorticity mixing in a rotating fluid
Aubert, J., Jung, S., & Swinney, H. L. (2002) · Geophysical Research Letters · doi:10.1029/2002gl015422 · Cited by 56
From zonal flow to convection rolls in Rayleigh–Bénard convection with free-slip plates
Wang, Q., Chong, K. L., Stevens, R. J. A. M., Verzicco, R., & Lohse, D. (2020) · Journal of Fluid Mechanics · doi:10.1017/jfm.2020.793 · Cited by 54
“…examples include zonal flow in the atmosphere of Jupiter (Heimpel et al. 2005; Kaspi et al. 2018; Kong et al. 2018) and other three Jovian planets (Ingersoll 1990; Sun et al. 1993; Cho & Polvani 1996; Yano et al. 2003), in the oceans (Maximenko et al. 2005; Richards et al. 2006; Nadiga 2006), and…”
BackgroundA laboratory model for deep-seated jets on the gas giants
Cabanes, S., Aurnou, J., Favier, B., & Le Bars, M. (2017) · Nature Physics · doi:10.1038/nphys4001 · Cited by 52
Ingersoll, A. P., Adumitroaie, V., Allison, M., Atreya, S., Bellotti, A., Bolton, S. J., Brown, S., Gulkis, S., Janssen, M., Levin, S. M., et al. (2017) · Geophysical Research Letters · doi:10.1002/2017gl074277 · Cited by 32
Li, L., Conrath, B. J., Gierasch, P. J., Achterberg, R. K., Nixon, C. A., Simon, A. A., Flasar, F. M., Banfield, D., Baines, K. H., West, R. A., et al. (2010) · Journal of Geophysical Research Atmospheres · doi:10.1029/2010je003631 · Cited by 47
Neptune and Triton: Essential pieces of the Solar System puzzle
Masters, A., Achilleos, N., Agnor, C. B., Campagnola, S., Charnoz, S., Christophe, B., Coates, A. J., Fletcher, L. N., Jones, G. H., Lamy, L., et al. (2014) · Planetary and Space Science · doi:10.1016/j.pss.2014.05.008 · Cited by 48
A theory for the emergence of coherent structures in beta-plane turbulence
Bakas, N. A., & Ioannou, P. J. (2014) · Journal of Fluid Mechanics · doi:10.1017/jfm.2013.663 · Cited by 40
Generation of zonal flows by Rossby waves in the atmosphere
Onishchenko, O. G., Pokhotelov, O. A., Sagdeev, R. Z., Shukla, P. K., & Stenflo, L. (2004) · Nonlinear processes in geophysics · doi:10.5194/npg-11-241-2004 · Cited by 47
Formation of Jets by Baroclinic Turbulence
Farrell, B. F., & Ioannou, P. J. (2008) · Journal of the Atmospheric Sciences · doi:10.1175/2008jas2611.1 · Cited by 41
“Coherent jets that are not forced at the jet scale are often observed in turbulent flows, with a familiar geophysical-scale example being the banded winds of the gaseous planets (Ingersoll 1990; Vasavada and Showman 2005; Sánchez-Lavega et al. 2008).”
BackgroundOn the vertical wind shear of Saturn's Equatorial Jet at cloud level
Pérez-Hoyos, S., & Sánchez-Lavega, A. (2005) · Icarus · doi:10.1016/j.icarus.2005.07.011 · Cited by 44
Statistical mechanical theory of the great red spot of jupiter
Michel, J., & Robert, R. (1994) · Journal of Statistical Physics · doi:10.1007/bf02179454 · Cited by 44
Multiple jets and zonal flow on Jupiter
JONES, C. A., Rotvig, J., & Abdulrahman, A. (2003) · Geophysical Research Letters · doi:10.1029/2003gl016980 · Cited by 44
Thermal shallow water models of geostrophic turbulence in Jovian atmospheres
Warneford, E. S., & Dellar, P. J. (2014) · Physics of Fluids · doi:10.1063/1.4861123 · Cited by 42
The climate system and the second law of thermodynamics
Singh, M. S., & O’Neill, M. E. (2022) · Reviews of Modern Physics · doi:10.1103/revmodphys.94.015001 · Cited by 50
A high‐resolution, three‐dimensional model of Jupiter's Great Red Spot
Cho, J. Y., Juárez, M. D. L. T., Ingersoll, A. P., & Dritschel, D. G. (2001) · Journal of Geophysical Research Atmospheres · doi:10.1029/2000je001287 · Cited by 41
Bastin, M. E., & Read, P. L. (1998) · Physics of Fluids · doi:10.1063/1.869530 · Cited by 40
Asymptotic expansions and monopolar solitary Rossby vortices in barotropic and two-layer models
Stegner, A., & Zeitlin, V. (1996) · Geophysical & Astrophysical Fluid Dynamics · doi:10.1080/03091929608208965 · Cited by 39
Dynamics of the atmospheres of the outer planets: Post‐Voyager measurement objectives
Gierasch, P. J., & Conrath, B. J. (1993) · Journal of Geophysical Research Atmospheres · doi:10.1029/92je01897 · Cited by 39
Suárez, G., Vos, J. M., Metchev, S., Faherty, J. K., & Cruz, K. L. (2023) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/acec4b · Cited by 38
Solar flux in Saturn's atmosphere: Penetration and heating rates in the aerosol and cloud layers
Pérez-Hoyos, S., & Sánchez-Lavega, A. (2005) · Icarus · doi:10.1016/j.icarus.2005.10.009 · Cited by 38
A stochastic structural stability theory model of the drift wave–zonal flow system
Farrell, B. F., & Ioannou, P. J. (2009) · Physics of Plasmas · doi:10.1063/1.3258666 · Cited by 36
“sion devices. 1. Introduction Coherent jets that are not forced at the jet scale are often observed in turbulent flows with a familiar geophysical example being the zonal winds of the gaseous planets (Ingersoll 1990). This phenomenon of spontaneous jet formation in turbulence has been extensively investigated in observ…”
Origins of atmospheric zonal winds
Yano, J., Talagrand, O., & Drossart, P. (2003) · Nature · doi:10.1038/421036a · Cited by 37
Atmospheres on Nonsynchronized Eccentric-tilted Exoplanets. I. Dynamical Regimes
Ohno, K., & Zhang, X. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab06cc · Cited by 35
“For example, Neptune (supposed to be in regime III) shows a strong westward jet at the equator in the troposphere (Ingersoll 1990; Liu & Schneider 2010), and Jupiters stratosphere (supposed to be in regime II) shows a strong four-year quasi-periodic oscillation at the equator (Leovy et al. 1991;…”
BackgroundForce balance in rapidly rotating Rayleigh–Bénard convection
Guzmán, A. J. A., Madonia, M., Cheng, J. S., Ostilla–Mónico, R., Clercx, H. J. H., & Kunnen, R. (2021) · Journal of Fluid Mechanics · doi:10.1017/jfm.2021.802 · Cited by 36
“…as deep convection in the interior of gaseous planets (Busse & Carrigan 1976; Busse 1994; Yadav & Bloxham 2020) and zonal flows in their atmosphere (Ingersoll 1990; Sanchez-Lavega, Rojas & Sada 2000; Porco et al. 2003; Heimpel & Aurnou 2007; Heimpel, Gastine & Wicht 2016; Cabanes et al. 2017), as…”
BackgroundTemporal behavior of cloud morphologies and motions in Saturn's atmosphere
Sánchez-Lavega, A., Lecacheux, J., Colas, F., & Laques, P. (1993) · Journal of Geophysical Research Atmospheres · doi:10.1029/93je01777 · Cited by 36
S3T stability of the homogeneous state of barotropic beta-plane turbulence
Bakas, N., Constantinou, N. C., & Ioannou, P. (2014) · Journal of the Atmospheric Sciences · doi:10.1175/jas-d-14-0213.1 · Cited by 32
On the Mechanism Underlying the Spontaneous Emergence of Barotropic Zonal Jets
Bakas, N. A., & Ioannou, P. J. (2013) · Journal of the Atmospheric Sciences · doi:10.1175/jas-d-12-0102.1 · Cited by 32
Garcia‐Melendo, E., Sánchez-Lavega, A., & Dowling, T. E. (2005) · Icarus · doi:10.1016/j.icarus.2005.02.012 · Cited by 34
Emergence of Jets from Turbulence in the Shallow-Water Equations on an Equatorial Beta Plane
Farrell, B. F., & Ioannou, P. J. (2009) · Journal of the Atmospheric Sciences · doi:10.1175/2009jas2941.1 · Cited by 29
Porco, C. C., West, R. A., SQUYRES, S. W., McEwen, A. S., Thomas, P. C., Murray, C. D., C, A. D. D. G., Ingersoll, A. P., Johnson, T. V., Neukum, G., et al. (2005) · Kluwer Academic Publishers eBooks · doi:10.1007/1-4020-3874-7_6 · Cited by 33
Rossby solitary vortices, on giant planets and in the laboratory
Nezlin, M. V. (1994) · Chaos An Interdisciplinary Journal of Nonlinear Science · doi:10.1063/1.166003 · Cited by 33
Marcos, C. D. L. F., & Barge, P. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04228.x · Cited by 30
Emitted power of Jupiter based on Cassini CIRS and VIMS observations
Li, L., Baines, K. H., Smith, M. A., West, R. A., Pérez-Hoyos, S., Trammell, H. J., Simon, A. A., Conrath, B. J., Gierasch, P. J., Orton, G. S., et al. (2012) · Journal of Geophysical Research Atmospheres · doi:10.1029/2012je004191 · Cited by 29
The global energy balance of Titan
Li, L., Nixon, C. A., Achterberg, R. K., Smith, M. A., Gorius, N., Jiang, X., Conrath, B. J., Gierasch, P. J., Simon, A. A., Flasar, F. M., et al. (2011) · Geophysical Research Letters · doi:10.1029/2011gl050053 · Cited by 28
Nezlin, M. V., & Sutyrin, G. G. (1994) · Surveys in Geophysics · doi:10.1007/bf00665687 · Cited by 28
Structural stability theory of two-dimensional fluid flow under stochastic forcing
Bakas, N. A., & Ioannou, P. J. (2011) · Journal of Fluid Mechanics · doi:10.1017/jfm.2011.228 · Cited by 27
Catling, D. C. (2015) · Elsevier eBooks · doi:10.1016/b978-0-444-53802-4.00185-8 · Cited by 30
Uranus and Neptune are key to understand planets with hydrogen atmospheres
Guillot, T. (2021) · Experimental Astronomy · doi:10.1007/s10686-021-09812-x · Cited by 27
A generalized Rhines effect and storms on Jupiter
Theiss, J. (2006) · Geophysical Research Letters · doi:10.1029/2005gl025379 · Cited by 28
The Galileo Probe Atmosphere Structure Instrument
SEIFF, A., & Knight, T. C. D. (1992) · Springer eBooks · doi:10.1007/978-94-011-2512-3_8 · Cited by 26
Statistical State Dynamics: A New Perspective on Turbulence in Shear Flow
Farrell, B. F., & Ioannou, P. J. (2019) · Cambridge University Press eBooks · doi:10.1017/9781107358225.025 · Cited by 25
Neptune's Stratospheric Winds from Three Central Flash Occultations
French, R. G., McGhee, C. A., & Sicardy, B. (1998) · Icarus · doi:10.1006/icar.1998.6001 · Cited by 25
Cabanes, S., Spiga, A., & Young, R. M. B. (2020) · Icarus · doi:10.1016/j.icarus.2020.113705 · Cited by 24
“Jupiter, Saturn, Uranus and Neptune (Ingersoll, 1990) are unmistakable markers of powerful, self-organized, atmospheric dynamics, insofar as they have been difficult to access by direct measurements.”
BackgroundA Comparative Study of Jovian Cyclonic Features from a Six-Year (1994–2000) Survey
Morales-Juberías, R. (2002) · Icarus · doi:10.1006/icar.2002.6973 · Cited by 23
Sloping convection: A paradigm for large-scale waves and eddies in planetary atmospheres?
HIDE, R., Lewis, S. R., Jr., & Read, P. L. (1994) · Chaos An Interdisciplinary Journal of Nonlinear Science · doi:10.1063/1.166000 · Cited by 23
Miesch, M. S. (2001) · The Astrophysical Journal · doi:10.1086/323527 · Cited by 23
“Banded zonal Ñows are a well-known feature in the atmospheres of the giant planets (e.g., Ingersoll 1990).”
BackgroundPlanetary vortices and Jupiter's vertical structure
WILLIAMS, G. P. (1997) · Journal of Geophysical Research Atmospheres · doi:10.1029/97je00520 · Cited by 22
The Global Atmospheric Circulation of Saturn
Showman, A. P., Ingersoll, A. P., Achterberg, R. K., & Kaspi, Y. (2018) · Cambridge University Press eBooks · doi:10.1017/9781316227220.011 · Cited by 21
“It also complements other reviews of Jupiter48 and the giant planets generally, including Ingersoll (1990),49 Marcus (1993) Dowling (1995a), Ingersoll et al. (2004), and50 Vasavada and Showman (2005).”
ResultHigh Winds of Neptune: A Possible Mechanism
SUOMI, V. E., Limaye, S. S., & Johnson, D. R. (1991) · Science · doi:10.1126/science.251.4996.929 · Cited by 21
Deep two-dimensional turbulence: An idealized model for atmospheric jets of the giant outer planets
Yano, J., Talagrand, O., & Drossart, P. (2005) · Geophysical & Astrophysical Fluid Dynamics · doi:10.1080/03091920412331336398 · Cited by 21
Yang, Y., Verzicco, R., Lohse, D., & Stevens, R. J. A. M. (2020) · Physical Review Fluids · doi:10.1103/physrevfluids.5.053501 · Cited by 20
Magnetic Suppression of Zonal Flows on a Beta Plane
Constantinou, N. C., & Parker, J. B. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aace53 · Cited by 19
“Zonal flows, or latitudinal bands of east-west alternating fluid flow, commonly form in the atmospheres of rotating planets (Ingersoll 1990; Vasavada & Showman 2005).”
BackgroundAnisotropic turbulence and Rossby waves in an easterly jet: An experimental study
Galperin, B., Hoemann, J., Espa, S., & Nitto, G. D. (2014) · Geophysical Research Letters · doi:10.1002/2014gl060767 · Cited by 19
Dynamics and Interaction between a Large-Scale Vortex and the Great Red Spot in Jupiter
Sánchez-Lavega, A., Hueso, R., Lecacheux, J., Colas, F., Rojas, J. F., Gómez, J. M., Miyazaki, I., & Parker, D. C. (1998) · Icarus · doi:10.1006/icar.1998.6006 · Cited by 19
Short-term changes in the belt/zone structure of Saturn's Southern Hemisphere (1996–2004)
Pérez-Hoyos, S., Sánchez-Lavega, A., & French, R. G. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20065972 · Cited by 18
Point vortex dynamics within a background vorticity patch
Jin, D. Z., & Dubin, D. H. E. (2001) · Physics of Fluids · doi:10.1063/1.1343484 · Cited by 18
Statistical Mechanics and Hydrodynamical Turbulence
Robert, R. (1995) · Birkhäuser Basel eBooks · doi:10.1007/978-3-0348-9078-6_149 · Cited by 18
Cassini spacecraft reveals global energy imbalance of Saturn
Wang, X., Li, L., Jiang, X., Fry, P. M., West, R. A., Nixon, C. A., Guan, L., Gamalathge, T. D. K., Albright, R. J., Colwell, J. E., et al. (2024) · Nature Communications · doi:10.1038/s41467-024-48969-9 · Cited by 15
Farrell, B. F., & Ioannou, P. J. (2017) · Physical Review Fluids · doi:10.1103/physrevfluids.2.073801 · Cited by 13
Turbulence and coherent structures in non-neutral plasmas
Romé, M., & Lepreti, F. (2011) · The European Physical Journal Plus · doi:10.1140/epjp/i2011-11038-4 · Cited by 14
Metadata
- Authors
- Ingersoll, A. P.
- Affiliations
- California Institute of Technology (US)
- Corresponding author
- Ingersoll, Andrew P.
- ORCID
- Ingersoll, Andrew P.
- Venue
- Science
- Published
- 1990-04-20
- Volume
- 248
- Issue
- 4953
- Pages
- 308-315
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2101776268
- Cited by
- 199
- References
- 69
- Citations by year
- 2026: 1 · 2025: 4 · 2024: 6 · 2023: 3 · 2022: 6 · 2021: 5 · 2020: 8 · 2019: 6 · 2018: 10 · 2017: 9 · 2016: 3 · 2015: 3 · 2014: 7 · 2013: 6 · 2012: 2
- FWCI
- 10.40
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Science (publishedVersion)
- PubMed (publishedVersion)
- CaltechAUTHORS (California Institute of Technology) (submittedVersion)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Engineering › Computational Mechanics › Fluid Dynamics and Turbulent Flows
- Keywords
- Jovian planets, planetary atmospheres, atmospheric dynamics, jet stream, Great Red Spot, Jupiter, Saturn, Uranus, Neptune, cloud formation, planetary interiors, fluid dynamical model, space missions
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review