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.


BIOMARKERS

Molecular Biopsy of Human Tumors

- a resource for Precision Medicine *

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]  

  • 7. Jets.
    Rhines PB
    Chaos; 1994 Jun; 4(2):313-339. PubMed ID: 12780108
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Depth of a strong jovian jet from a planetary-scale disturbance driven by storms.
    Sánchez-Lavega A; Orton GS; Hueso R; García-Melendo E; Pérez-Hoyos S; Simon-Miller A; Rojas JF; Gómez JM; Yanamandra-Fisher P; Fletcher L; Joels J; Kemerer J; Hora J; Karkoschka E; de Pater I; Wong MH; Marcus PS; Pinilla-Alonso N; Carvalho F; Go C; Parker D; Salway M; Valimberti M; Wesley A; Pujic Z
    Nature; 2008 Jan; 451(7177):437-40. PubMed ID: 18216848
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Multiple zonal jets and drifting: thermal convection in a rapidly rotating spherical shell compared to a quasigeostrophic model.
    Rotvig J
    Phys Rev E Stat Nonlin Soft Matter Phys; 2007 Oct; 76(4 Pt 2):046306. PubMed ID: 17995105
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Successes and failures of shallow-water interpretations of Voyager wind data.
    Dowling TE
    Chaos; 1994 Jun; 4(2):213-225. PubMed ID: 12780101
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Penetrative Convection and Zonal Flow on Jupiter.
    Zhang K; Schubert G
    Science; 1996 Aug; 273(5277):941-3. PubMed ID: 8688074
    [TBL] [Abstract][Full Text] [Related]  

  • 12. An intense stratospheric jet on Jupiter.
    Flasar FM; Kunde VG; Achterberg RK; Conrath BJ; Simon-Miller AA; Nixon CA; Gierasch PJ; Romani PN; Bézard B; Irwin P; Bjoraker GL; Brasunas JC; Jennings DE; Pearl JC; Smith MD; Orton GS; Spilker LJ; Carlson R; Calcutt SB; Read PL; Taylor FW; Parrish P; Barucci A; Courtin R; Coustenis A; Gautier D; Lellouch E; Marten A; Prangé R; Biraud Y; Fouchet T; Ferrari C; Owen TC; Abbas MM; Samuelson RE; Raulin F; Ade P; Césarsky CJ; Grossman KU; Coradini A
    Nature; 2004 Jan; 427(6970):132-5. PubMed ID: 14712270
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Clusters of cyclones encircling Jupiter's poles.
    Adriani A; Mura A; Orton G; Hansen C; Altieri F; Moriconi ML; Rogers J; Eichstädt G; Momary T; Ingersoll AP; Filacchione G; Sindoni G; Tabataba-Vakili F; Dinelli BM; Fabiano F; Bolton SJ; Connerney JEP; Atreya SK; Lunine JI; Tosi F; Migliorini A; Grassi D; Piccioni G; Noschese R; Cicchetti A; Plainaki C; Olivieri A; O'Neill ME; Turrini D; Stefani S; Sordini R; Amoroso M
    Nature; 2018 Mar; 555(7695):216-219. PubMed ID: 29516997
    [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]
    of 16.