These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.
304 related articles for article (PubMed ID: 16281029)
1. Simulation of equatorial and high-latitude jets on Jupiter in a deep convection model. Heimpel M; Aurnou J; Wicht J Nature; 2005 Nov; 438(7065):193-6. PubMed ID: 16281029 [TBL] [Abstract][Full Text] [Related]
2. A strong decrease in Saturn's equatorial jet at cloud level. Sánchez-Lavega A; Pérez-Hoyos S; Rojas JF; Hueso R; French RG Nature; 2003 Jun; 423(6940):623-5. PubMed ID: 12789333 [TBL] [Abstract][Full Text] [Related]
3. Moist convection as an energy source for the large-scale motions in Jupiter's atmosphere. Galileo Imaging Team. Ingersoll AP; Gierasch PJ; Banfield D; Vasavada AR Nature; 2000 Feb; 403(6770):630-2. PubMed ID: 10688192 [TBL] [Abstract][Full Text] [Related]
4. Jupiter's Great Red Spot and zonal winds as a self-consistent, one-layer, quasigeostrophic flow. Marcus PS; Lee C Chaos; 1994 Jun; 4(2):269-286. PubMed ID: 12780104 [TBL] [Abstract][Full Text] [Related]
5. Jupiter's zonal winds: are they bands of homogenized potential vorticity organized as a monotonic staircase? Marcus PS; Shetty S Philos Trans A Math Phys Eng Sci; 2011 Feb; 369(1937):771-95. PubMed ID: 21242133 [TBL] [Abstract][Full Text] [Related]
6. Banded surface flow maintained by convection in a model of the rapidly rotating giant planets. Sun ZP; Schubert G; Glatzmaier GA Science; 1993 Apr; 260(5108):661-4. PubMed ID: 17812225 [TBL] [Abstract][Full Text] [Related]
14. Deep rotating convection generates the polar hexagon on Saturn. Yadav RK; Bloxham J Proc Natl Acad Sci U S A; 2020 Jun; 117(25):13991-13996. PubMed ID: 32513703 [TBL] [Abstract][Full Text] [Related]
15. Magnetic damping of jet flows in quasi-two-dimensional Rayleigh-Bénard convection. Aggarwal A; Aurnou JM; Horn S Phys Rev E; 2022 Oct; 106(4-2):045104. PubMed ID: 36397562 [TBL] [Abstract][Full Text] [Related]
16. Computer simulations of Jupiter's deep internal dynamics help interpret what Juno sees. Glatzmaier GA Proc Natl Acad Sci U S A; 2018 Jul; 115(27):6896-6904. PubMed ID: 29941563 [TBL] [Abstract][Full Text] [Related]
17. Atmospheric dynamics of the outer planets. Ingersoll AP Science; 1990 Apr; 248(4953):308-15. PubMed ID: 17784483 [TBL] [Abstract][Full Text] [Related]
18. Origin of Jupiter's cloud-level zonal winds remains a puzzle even after Juno. Kong D; Zhang K; Schubert G; Anderson JD Proc Natl Acad Sci U S A; 2018 Aug; 115(34):8499-8504. PubMed ID: 30087183 [TBL] [Abstract][Full Text] [Related]
19. Jupiter's first 100 miles. Reichhardt T Aerosp Am; 1996 Apr; 34(4):22-5, 36. PubMed ID: 11538723 [TBL] [Abstract][Full Text] [Related]
20. Infrared observations of the jovian system from voyager 2. Hanel R; Conrath B; Flasar M; Herath L; Kunde V; Lowman P; Maguire W; Pearl J; Pirraglia J; Samuelson R; Gautier D; Gierasch P; Horn L; Kumar S; Ponnamperuma C Science; 1979 Nov; 206(4421):952-6. PubMed ID: 17733912 [TBL] [Abstract][Full Text] [Related] [Next] [New Search]