The DOI matches its Crossref record; 15 of the 15 references it cites were found in a registry or an index.
A simple model of convection in the Jovian atmosphere
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
“on one hand, the alternating jets on gas giant planets are 'shallow', existing above 10 bars or so [15-17]; on the other hand, zonal jets are 'deep', extending to tens of thousands of bars [18-22].”
From Deep rotating convection generates the polar hexagon on Saturn (2020) · cites this paper as [18]
In the citing paper
“Existing models posit as the driver of the flow either the differential radiative heating of the upper atmosphere (e.g., Williams 1979Williams , 2003b) ) or the intrinsic heat fluxes emanating from the deep interior (e.g., Busse 1976;Heimpel et al. 2005;Aurnou et al. 2007;Chan and Mayr 2008;Kaspi et al. 2009).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Busse 1976
In the citing paper
“Under these circumstances, convective plumes are columns aligned with M V surfaces because, as above, rapid rotation inhibits motion perpendicular to M V surfaces in the absence of viscous or other stresses (e.g., Busse 1976Busse , 1978;;Kaspi et al. 2009;Jones et al. 2009).”
From Mechanisms of Jet Formation on the Giant Planets (2010) · cites this paper as Busse 1976
Citations
Cites
Hydrodynamic and Hydromagnetic Stability
Chandrasekhar, S., & Gillis, J. (1962) · Physics Today · doi:10.1063/1.3058072 · Cited by 10,517
Hydrodynamic and hydromagnetic stability
Chandrasekhar, S. (1961) · CERN Document Server (European Organization for Nuclear Research) · Cited by 6,543
Thermal instabilities in rapidly rotating systems
Busse, F. H. (1970) · Journal of Fluid Mechanics · doi:10.1017/s0022112070001921 · Cited by 740
Self-citationA study of Bénard convection with and without rotation
Rossby, T. (1969) · Journal of Fluid Mechanics · doi:10.1017/s0022112069001674 · Cited by 609
On the thermal instability of a rotating-fluid sphere containing heat sources
Roberts, P. H. (1968) · Philosophical Transactions of the Royal Society of London Series A Mathematical and Physical Sciences · doi:10.1098/rsta.1968.0007 · Cited by 359
Differential Rotation in Stellar Convection Zones
Busse, F. H. (1970) · The Astrophysical Journal · doi:10.1086/150337 · Cited by 183
Self-citationLaboratory Simulation of Thermal Convection in Rotating Planets and Stars
Busse, F. H., & Carrigan, C. R. (1976) · Science · doi:10.1126/science.191.4222.81 · Cited by 133
Self-citationPodolak, M., & Cameron, A. G. W. (1974) · Icarus · doi:10.1016/0019-1035(74)90113-4 · Cited by 112
Structure of Jupiter and Saturn
Hubbard, W. B., & Smoluchowski, R. (1973) · Space Science Reviews · doi:10.1007/bf00166644 · Cited by 74
On the Thermal Instability of a Highly Rotating Fluid Sphere.
Roberts, P. H. (1965) · The Astrophysical Journal · doi:10.1086/148106 · Cited by 54
Cited by
Sorted by citations
Zonal flows in plasma—a review
Diamond, P. H., Itoh, S. ‐., Itoh, K., & Hahm, T. S. (2005) · Plasma Physics and Controlled Fusion · doi:10.1088/0741-3335/47/5/r01 · Cited by 1,942
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
Cassini Imaging of Jupiter's Atmosphere, Satellites, and Rings
Porco, C. C., West, R. A., McEwen, A. S., C, A. D. D. G., Ingersoll, A. P., Thomas, P. C., Squyres, S. W., Luke Dones, B., Murray, C. D., Johnson, T. V., et al. (2003) · Science · doi:10.1126/science.1079462 · Cited by 489
A quarter-century of H-mode studies
Wagner, F. (2007) · Plasma Physics and Controlled Fusion · doi:10.1088/0741-3335/49/12b/s01 · Cited by 411
ZONAL FLOWS AND LONG-LIVED AXISYMMETRIC PRESSURE BUMPS IN MAGNETOROTATIONAL TURBULENCE
Johansen, A., Youdin, A. N., & Klahr, H. H. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/697/2/1269 · Cited by 405
“Busse (1976) proposed that these flows arise from an inverse cascade of thermally driven convection in giant planet interiors.”
Background
Metadata
- Authors
- Busse, F. H.
- Affiliations
- University of California, Los Angeles (US)
- Corresponding author
- Busse, F.H.
- ORCID
- Busse, F.H.
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 1976-10
- Volume
- 29
- Issue
- 2
- Pages
- 255-260
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2074802867
- Cited by
- 278
- References
- 15
- Citations by year
- 2026: 3 · 2025: 4 · 2024: 5 · 2023: 8 · 2022: 9 · 2021: 6 · 2020: 11 · 2019: 9 · 2018: 34 · 2017: 10 · 2016: 8 · 2015: 9 · 2014: 4 · 2013: 5 · 2012: 7
- FWCI
- 2.52
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Icarus (publishedVersion)
- ERef Bayreuth (University of Bayreuth) (submittedVersion)
- Funders
- National Science Foundation
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Engineering › Computational Mechanics › Fluid Dynamics and Turbulent Flows
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- Jupiter atmosphere, convection, latitudinal structure, internal heating, Boussinesq approximation, eddy viscosity, turbulent flow
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
