REFERENCES
Andrews DG, Holton JR, Leovy CB. 1987. Middle Atmosphere Dynamics. Orlando, FL:
Academic Press
Andrews DG, McIntyre ME. 1976. Planetary waves in horizontal and vertical shear: thegeneralized Eliassen-Palm relation and the mean zonal acceleration. J. Atmos. Sci. 33:2031‒
48
Arnold NP, Tziperman E, Farrell B. 2012. Abrupt transition to strong superrotation driven
by equatorial wave resonance in an idealized GCM. J. Atmos. Sci. 69:626‒40Baldwin MP, Gray LJ, Dunkerton TJ, Hamilton K, Haynes PH, et al. 2001. The quasi-biennial
oscillation. Rev. Geophys. 39:179‒229
Bird MK, Allison M, Asmar SW, Atkinson DH, Avruch IM, et al. 2005. The vertical profile ofwinds on Titan. Nature 438:800‒2Cornillon, P. C., E. Firing, A. F. Thomson, L. M. Ivanov, I Kamenkovich, C. E. Buckingham,
Y. D. Afanasyev. (2019) "Oceans" in Zonal Jets. Phenomenology, Genesis, Physics (eds. B.
Galperin and P. Read), pp46-71. Cambridge University Press, New York.
Del Genio AD, Rossow WB. 1990. Planetary-scale waves and the cyclic nature of cloud top
dynamics on Venus. J. Atmos. Sci. 47:293‒318
Del Genio AD, Zhou W. 1996. Simulations of superrotation on slowly rotating planets:
sensitivity to rotation and initial conditions. Icarus 120:332‒43
Dias Pinto JR, Mitchell JL. 2014. Atmospheric superrotation in an idealized GCM: parameter
dependence of the eddy response. Icarus 238:93‒109
Douglas, H. A., Mason, P. J., Hinch, E. J. (1972) Motion due to a moving heat source, J Fluid
Mech., 54, 469-480.
Edmon HJ Jr., Hoskins BJ, McIntyre ME. 1980. Eliassen-Palm cross sections for thetroposphere. J. Atmos. Sci. 37:2600‒16Fels SB, Lindzen RS. 1974. The interaction of thermally excited gravity waves with mean flows.
Geophys. Fluid Dyn. 6:149‒91
Fultz, D. 1956. Studies in experimental hydrodynamics (I), Final Report Hydrodynamics
Laboratory, University of Chicago, B7-B40.
Gierasch PJ. 1975. Meridional circulation and the maintenance of the Venus atmosphericrotation. J. Atmos. Sci. 32:1038‒44A.E. Gill, Some simple solutions for heat-induced tropical circulation. Q. J. R. Meteorol. Soc.
106, 447‒462 (1980)
Glatzmaier GA, Roberts PH. 1996. Rotation and magnetism of Earthʼs inner core. Science274:1887‒91
Hammond, M., Tsai, S-M, Pierrehumbert, RT (2020) The equatorial jet speed on Tidallylocked planets. I. Terrestrial planets.. Atrophys. J., 901, 78
Hammond, M., Lewis, NT (2021) The rotational and divergent components of atmosphericcirculation on tidally locked planets. PNAS, 118,e2022705118
M. Heimpel, J. Aurnou, J. Wicht, Simulation of equatorial and high-latitude jets on Jupiter ina deep convection model. Nature 438, 193‒196 (2005)
Held IM, Hou AY. 1980. Nonlinear axially symmetric circulations in a nearly inviscid
atmosphere. J. Atmos. Sci. 37:515‒33
K. Heng, A.P. Showman, Atmospheric dynamics of hot exoplanets. Annu. Rev. Earth Planet.
Sci. 43, 509‒540 (2015)
Hide R. 1969. Dynamics of the atmospheres of the major planets, with an appendix on theviscous boundary layer at the rigid bounding surface of an electrically-conducting rotating
fluid in the presence of a magnetic field. J. Atmos. Sci. 26:841‒53T. Horinouchi et al., How waves and turbulence maintain the super-rotation of Venusʼatmosphere. Science 368, 405‒409 (2020). https://doi.org/10.1126/science.aaz4439
S.M. Hörst, Titanʼs atmosphere and climate. J. Geophys. Res. 122, 432‒482 (2017).
https://doi.org/10.1002/2016JE005240
Hourdin F, Talagrand O, Sadourny R, Courtin R, Gautier D, McKay CP. 1995. Numericalsimulation of the general circulation of the atmosphere of Titan. Icarus 117:358‒74
Hubbard WB, Sicardy B, Miles R, Hollis AJ, Forrest RW, et al. 1993. The occultation of 28
Sgr by Titan. Astron. Astrophys. 269:541‒63
M. Imai, T. Kouyama, Y. Takahashi, A. Yamazaki, S.Watanabe,M. Yamada, T. Imamura, T.
Satoh, M. Nakamura, S. Murakami, K. Ogohara, T. Horinouchi, Planetary-scale variations inwinds and UV brightness at the Venusian cloud top: periodicity and temporal evolution. J.
Geophys. Res. 124(10), 2635‒2659 (2019). https://doi.org/10.1029/2019JE006065
K´alnay de Rivas E. 1975. Further numerical calculations of the circulation of the atmosphereof Venus. J. Atmos. Sci. 32:1017‒24
Kerzhanovich VV, Marov MI. 1983. The atmospheric dynamics of Venus according toDoppler
measurements by the Venera entry probes. In Venus, ed. DM Hunten, L Colin, TM Donahue,
VI Moroz, pp. 766‒78. Tucson: Univ. Ariz. Press
King-Hele DG. 1964. The rotational speed of the upper atmosphere, determined fromchanges in satellite orbits. Planet. Space Sci. 12:835‒53
H.A. Knutson et al., A map of the day-night contrast of the extrasolar planet HD 189733b.
Nature 447, 183‒186 (2007)
Laraia AL, Schneider T. 2015. Superrotation in terrestrial atmospheres. J. Atmos. Sci.
72:4281‒96
Lebonnois S, Burgalat J, Rannou P, Charnay B. 2012a. Titan Global Climate Model: new 3dimensional version of the IPSL Titan GCM. Icarus 218:707‒22
Lebonnois S, Covey C, GrossmanA,ParishH, Schubert G, et al. 2012b. Angular momentum

budget in General Circulation Models of superrotating atmospheres: a critical diagnostic. J.
Geophys. Res. 117:E12004
Lebonnois S, Flasar FM, Tokano T, Newman CE. 2014. The general circulation of Titanʼslower and middle atmosphere. In Titan: Interior, Surface, Atmosphere and Space
Environment, ed. I Mueller-Wodarg, C Griffith, E Lellouch, T Cravens, pp. 122‒57. New
York: Cambridge Univ. Press
Lebonnois S, Hourdin, F, Eymet, V, Crespin, A, Fournier R, Forget F. 2010. Superrotation ofVenusʼ atmosphere analyzed with a full general circulation model. J. Geophys. Res.
115:E06006
Lebonnois S, Lee C, Yamamoto M, Dawson J, Lewis SR, et al. 2013. Models of Venus
atmosphere. In Towards Understanding the Climate of Venus: Application of Terrestrial
Models to Our Sister Planet, ed. L Bengtsson, RM Bonnet, D Grinspoon, S Koumoutsaris,S Lebonnois, D Titov, pp. 129‒56. New York: Springer-Verlag
Lebonnois S, Sugimoto N, Gilli G. 2016. Wave analysis in the atmosphere of Venus below
100-km altitude, simulated by the LMD Venus GCM. Icarus 278:38‒51
Lee C, Lewis SR, Read PL. 2005. A numerical model of the atmosphere of Venus. Adv. SpaceRes. 36:2142‒45
Leovy C.B., Friedson A.J., Orton G.S. (1991) The quasiquadrennial oscillation of Jupiterʼsequatorial stratosphere Nature, 354 (380).
Lewis SR, Read PL. 2003. Equatorial jets in the dusty Martian atmosphere. J. Geophys. Res.
108:5034
Lewis, N. T., Colyer, G. J., Read, P. L. (2021) Characterising regimes of atmosphericcirculation in terms of their global superrotation. J. Atmos. Sci., 78, 1245-1258.
Li, X., Read, P.L., 2000. A mechanistic model of the quasi-quadrennial oscillation in Jupiterʼsstratosphere. Planet. Space Sci. 48, 637‒669.
Y. Lian, A.P. Showman, Generation of equatorial jets by large-scale latent heating on the giant

planets. Icarus 207, 373‒393 (2010)
Longuet-Higgins MS. 1968. The eigenfunctions of Laplaceʼs tidal equations over a sphere.
Philos. Trans. R. Soc. A 262:511‒607
Lora JM, Lunine JI, Russell JL. 2015. GCM simulations of Titanʼs middle and lower
atmosphere and comparison to observations. Icarus 250:516‒28
Matsuda, Y., 1980: Dynamics of the four-day circulation in the Venus atmosphere. J. Meteor.
Soc. Japan, 58, 443̶470.
Matsuda, Y., 1982: A further study of dynamics of the four day circulation in the Venus
atmosphere. J. Meteor. Soc. Japan, 60, 245̶254.
Matsuno, T. 1966. Quasi-geostrophic motions in the equatorial area. J Meteorol. Soc. Japan,44, 25-43.
Maxworthy, T., 1975. A wave-driven model of the Jovian equatorial jet. Planet. Space Sci. 23,1222‒1233.
Mendonca JM, Read PL. 2016. Exploring the Venus global super-rotation using acomprehensive general circulation model. Planet. Space Sci. 134:1‒18
Mitchell JL, Vallis GK. 2010. The transition to superrotation in terrestrial atmospheres. J.
Geophys. Res. 115:E12008
Mitchell, J. L., T. Birner, G. Lapeyre, N. Nakamura, P. L. Read, G. Riviere, A.
Sánchez-Lavega, G. K. Vallis, (2019) Terrestrial Atmospheres, in Zonal Jets. Phenomenology,Genesis, Physics (eds. B. Galperin and P. Read), pp 9-45. Cambridge University Press, NewYork.
Newman CE, Lee C, Lian Y, Richardson MI, Toigo AD. 2011. Stratospheric superrotation inthe TitanWRF model. Icarus 213:636‒54
Orton G.S., Friedson A.J., Baines K.H., Martin T.Z., West R.A., Caldwell J., Hammel H.B.,
Bergstralh J.T., Malcom M.E., Golisch W.F., et al. (1991) Thermal maps of Jupiter: spatialorganization and time dependence of stratospheric temperatures, 1980 to 1990. Science, 252,
pp. 537-542
N. Otobe, S. Sakai, S. Yoden, and M. Shiotani, “Visualization and WKB analysis of the internalgravity wave in the QBO experiment,” Nagare: Jpn. Soc. Fluid Mech. 17 (1998); available at
http://www2.nagare.or.jp/mm/98/otobe/index.htm.
A. Piccialli, D.V. Titov, D. Grassi, I. Khatuntsev, P. Drossart, G. Piccioni, A. Migliorini,
Cyclostrophic winds from the Visible and Infrared Thermal Imaging Spectrometer
temperature sounding: a preliminary analysis. J. Geophys. Res. 113, E00B11 (2008).
https://doi.org/10.1029/2008JE003127
R. T. Pierrehumbert, M. Hammond, Atmospheric circulation of tide-locked exoplanets.
Annu. Rev. Fluid Mech. 51, 275‒303 (2019).
Plumb, R. A., McEwan, A. D. (1978) The instability of a forced standing wave in a viscous,stratified fluid: a laboratory analogue of the Quasi-Biennial Oscillation, J. Atmos. Sci., 35,1827-1839.
S.F. Potter, G.K. Vallis, J.L. Mitchell, Spontaneous superrotation and the role of Kelvin wavelike variability in an idealized dry GCM. J. Atmos. Sci. 71, 596‒614 (2014)
Read, P. L. (1985) `Finite amplitude, neutral baroclinic eddies and mean flows in aninternally heated rotating fluid: I. numerical simulations and quasi-geostrophic "free modes"',Dyn. Atmos. Oceans, 9, 135-207
Read, P. L., 1986a: Super-rotation and diffusion of axial angular momentum. I. ʻʻSpeed limitsʼʼ
for axisymmetric flow in a rotating cylindrical fluid annulus. Quart. J. Roy. Meteor. Soc., 112,231‒251, https://doi.org/10.1002/qj.49711247113.
Read PL. 1986b. Super-rotation and diffusion of axial angular momentum. II. A review ofquasi-axisymmetric models of planetary atmospheres. Q. J. R. Meteorol. Soc. 112:253‒72
Lewis, S.R. and Read, P.L. (2003) Equatorial jets in the dusty Martian atmosphere, J. Geophys.
Res., 108 (E4), 5034

Read, P. L. & Lewis, S. R. (2004) The Martian Climate Revisited: Atmosphere andEnvironment of a Desert Planet. Springer-Praxis.
P.L. Read, S. Lebonnois, Superrotation on Venus, on Titan, and elsewhere. Annu. Rev. Earth
Planet. Sci. 46, 175‒202 (2018). https://doi.org/10.1146/annurev-earth-082517-010137
Rishbeth, H., 1971. Polarization 8elds produced by winds in the equatorial F-region.
Planetary and Space Science 19, 357‒369.
Rossow WB. 1983. A general circulation model of a Venus-like atmosphere. J. Atmos. Sci.
40:273‒302
Rossow WB, Williams GP. 1979. Large-scale motion in the Venus stratosphere. J. Atmos. Sci.
36:1377‒89
Ruan, T., N. T. Lewis, S. R. Lewis, L. Montabone, P. L. Read. 2019. Investigating thesemiannual oscillation on Mars using data assimilation. Icarus, 333, 404-414.
Sánchez-Lavega, A, L. A. Sromovsky, A. P. Showman, A. D. Del Genio, R. M. B. Young, R.
Hueso, E. Garcia-Melendo, Y. Kaspi, G. S. Orton, N. Barrado-Izagirre, D. S. Choi, J. M.
Barbara, (2019) Gas Giants, in Zonal Jets. Phenomenology, Genesis, Physics (eds. B.
Galperin and P. Read), pp 73-105. Cambridge University Press, New York.
A. Sánchez-Lavega, S. Lebonnois, T. Imamura, P. Read, D. Luz, The atmospheric dynamicsof Venus. Space Sci. Rev. 212, 1541‒1616 (2017). https://doi.org/10.1007/s11214-0170389-x
Saravanan R. 1993. Equatorial superrotation and maintenance of the general circulation in
two-level models. J. Atmos. Sci. 50:1211‒27
Sardeshmukh PD, Hoskins BJ. 1988. The generation of global rotational flow by steadyidealized tropical divergence. J. Atmos. Sci. 45:1228‒51
Schofield JT, Taylor FW. 1983. Measurements of the mean, solar-fixed temperature and cloud
structure of the middle atmosphere of Venus. Q. J. R. Meteorol. Soc. 109:57‒80

Schubert, G., Whitehead, J. A. (1969) The moving flame experiment with liquid mercury:possible implications for the Venus atmosphere. Science, 163, 71-72.
B. Semin, G. Facchini, F. Pétrélis, and S. Fauve, (2016) Generation of a mean flow by aninternal wave, Phys. Fluids, 28, 096601.
B. Semin, N. Garroum, F. P´etr´elis, and S. Fauve, (2018) Nonlinear saturation of the large
scale flow in a laboratory model of the quasibiennial oscillation, Phys. Rev. Lett., 121, 134502
Shamir, O., Garfinkel, C. I., Gerber, E. P., Paldor, N. (2023) The Matsuno-Gill model on thesphere, J Fluid Mech., 964, A32.
Showman AP,Cho J, Menou K. 2010. Atmospheric circulation of extrasolar planets. In
Exoplanets, ed.S Seager, pp. 471‒516. Tucson: Univ. Ariz. PressA.P. Showman, L.M. Polvani, The Matsuno-Gill model and equatorial superrotation.
Geophys. Res. Lett. 37, L18811 (2010)
Sicardy B, Ferri F, Roques F, Lecacheux J, Pau S, et al. 1999. The structure of Titanʼsstratosphere from the 28 Sgr occultation. Icarus 142:357‒90Starr VP. 1968. The Physics of Negative Viscosity Phenomena. New York: McGraw-Hill
Suarez MJ, Duffy DG. 1992. Terrestrial super-rotation: a bifurcation of the generalcirculation. J. Atmos. Sci. 49:1541‒54
Sugimoto N, Takagi M, Matsuda Y. 2014a. Baroclinic instability in the Venus atmospheresimulated by GCM. J. Geophys. Res. Planets 119:1950‒68
N.A. Teanby, M. Sylvestre, J. Sharkey, C.A. Nixon, S. Vinatier, P.G.J. Irwin, Seasonalevolution of Titanʼs stratosphere during the Cassini mission. Geophys. Res. Lett. 46, 3079‒
3089 (2019). https://doi.org/10.1029/2018GL081401
T. Tokano, F.M. Neubauer, M. Laube, C.P. McKay, Seasonal variation of Titanʼs atmosphericstructure simulated by a general circulation model. Planet. Space Sci. 47, 493‒520 (1999)

Vallis, G. K. (2017) Atmospheric and Oceanic Fluid Dynamics: fundamentals and large-scale
circulation. Cambridge University Press, New York.
Wang P, Mitchell JL. 2014. Planetary ageostrophic instability leads to superrotation. Geophys.
Res. Lett. 41:4118‒26
Wang, Y., P. L. Read, F. Tabataba-Vakili, and R. M. B. Young, 2018: Comparative terrestrial
atmospheric circulation regimes in simplified global circulation models. Part I: From
cyclostrophic super-rotation to geostrophic turbulence. Quart. J. Roy. Meteor. Soc., 144,
2537‒2557, https://doi.org/10.1002/qj.3350.
Whitehead, J. A., (1975) Mean flow generated by circulation on a beta-plane: an analogy withthe moving flame experiment, Tellus, 27, 358-364.
Williams, G. P., 2003: Barotropic instability and equatorial superrotation. J. Atmos. Sci., 60,
2136‒2152, https://doi.org/10.1175/1520-0469(2003)060,2136:BIAES.2.0.CO;2.
H. Yamamoto, S. Yoden, Theoretical estimation of the superrotation strength in an idealizedquasiaxisymmetric model of planetary atmospheres. J. Meteorol. Soc. Jpn. 91, 119‒141 (2013).
https://doi.org/10.2151/jmsj.2013-203
Yamamoto, H., K. Ishioka, and S. Yoden, 2009: Axisymmetric steady solutions in an idealized
model of atmospheric general circulations: Hadley circulation and super-rotation. Theor.
Appl. Mech. Japan, 57, 147‒158, https://doi.org/10.11345/nctam.57.147.
M. Yamamoto, M. Takahashi, Super-rotation and equatorial waves in a T21 Venus-like
AGCM. Geophys. Res. Lett. 30, 1449 (2003). https://doi.org/10.1029/2003GL016924
Yamazaki, Y. H., Read, P. L., Skeet, D. R. (2005) Hadley circulations and Kelvin wave-driven
equatorial jets in the atmospheres of Jupiter and Saturn, Plan. Space Sci., 53 508‒525
Yoden, S., Holton, J. R. (1988) A new look at equatorial Quasi-Biennial models, J. Atmos. Sci.,
45, 2703-2717.
R.M.B. Young, P.L. Read, Y.Wang, Simulating Jupiterʼs weather layer. Part I: jet spin-up in adry atmosphere. Icarus 326, 225‒252 (2019)