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 *

140 related articles for article (PubMed ID: 32831610)

  • 1. Acoustic and inertial modes in planetary-like rotating ellipsoids.
    Vidal J; Cébron D
    Proc Math Phys Eng Sci; 2020 Jul; 476(2239):20200131. PubMed ID: 32831610
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Acoustic modes of rapidly rotating ellipsoids subject to centrifugal gravity.
    Vidal J; Cébron D
    J Acoust Soc Am; 2021 Aug; 150(2):1467. PubMed ID: 34470306
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Inertial modes in a rotating triaxial ellipsoid.
    Vantieghem S
    Proc Math Phys Eng Sci; 2014 Aug; 470(2168):20140093. PubMed ID: 25104908
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Completeness of inertial modes of an incompressible inviscid fluid in a corotating ellipsoid.
    Backus G; Rieutord M
    Phys Rev E; 2017 May; 95(5-1):053116. PubMed ID: 28618529
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Characterization of columnar inertial modes in rapidly rotating spheres and spheroids.
    Maffei S; Jackson A; Livermore PW
    Proc Math Phys Eng Sci; 2017 Aug; 473(2204):20170181. PubMed ID: 28878558
    [TBL] [Abstract][Full Text] [Related]  

  • 6. Experimental observation of the geostrophic turbulence regime of rapidly rotating convection.
    Bouillaut V; Miquel B; Julien K; Aumaître S; Gallet B
    Proc Natl Acad Sci U S A; 2021 Nov; 118(44):. PubMed ID: 34697234
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Selection of inertial modes in spherical Couette flow.
    Kelley DH; Triana SA; Zimmerman DS; Lathrop DP
    Phys Rev E Stat Nonlin Soft Matter Phys; 2010 Feb; 81(2 Pt 2):026311. PubMed ID: 20365655
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Compressibility effects in Rayleigh-Taylor instability-induced flows.
    Gauthier S; Le Creurer B
    Philos Trans A Math Phys Eng Sci; 2010 Apr; 368(1916):1681-704. PubMed ID: 20211880
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Waves in planetary dynamos.
    Hori K; Nilsson A; Tobias SM
    Rev Mod Plasma Phys; 2023; 7(1):5. PubMed ID: 36588584
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Acoustic Eigenvalues of a Quasispherical Resonator: Second Order Shape Perturbation Theory for Arbitrary Modes.
    Mehl JB
    J Res Natl Inst Stand Technol; 2007; 112(3):163-73. PubMed ID: 27110463
    [TBL] [Abstract][Full Text] [Related]  

  • 11. A remnant planetary core in the hot-Neptune desert.
    Armstrong DJ; Lopez TA; Adibekyan V; Booth RA; Bryant EM; Collins KA; Deleuil M; Emsenhuber A; Huang CX; King GW; Lillo-Box J; Lissauer JJ; Matthews E; Mousis O; Nielsen LD; Osborn H; Otegi J; Santos NC; Sousa SG; Stassun KG; Veras D; Ziegler C; Acton JS; Almenara JM; Anderson DR; Barrado D; Barros SCC; Bayliss D; Belardi C; Bouchy F; Briceño C; Brogi M; Brown DJA; Burleigh MR; Casewell SL; Chaushev A; Ciardi DR; Collins KI; Colón KD; Cooke BF; Crossfield IJM; Díaz RF; Mena ED; Demangeon ODS; Dorn C; Dumusque X; Eigmüller P; Fausnaugh M; Figueira P; Gan T; Gandhi S; Gill S; Gonzales EJ; Goad MR; Günther MN; Helled R; Hojjatpanah S; Howell SB; Jackman J; Jenkins JS; Jenkins JM; Jensen ELN; Kennedy GM; Latham DW; Law N; Lendl M; Lozovsky M; Mann AW; Moyano M; McCormac J; Meru F; Mordasini C; Osborn A; Pollacco D; Queloz D; Raynard L; Ricker GR; Rowden P; Santerne A; Schlieder JE; Seager S; Sha L; Tan TG; Tilbrook RH; Ting E; Udry S; Vanderspek R; Watson CA; West RG; Wilson PA; Winn JN; Wheatley P; Villasenor JN; Vines JI; Zhan Z
    Nature; 2020 Jul; 583(7814):39-42. PubMed ID: 32612222
    [TBL] [Abstract][Full Text] [Related]  

  • 12. The Elbert range of magnetostrophic convection. I. Linear theory.
    Horn S; Aurnou JM
    Proc Math Phys Eng Sci; 2022 Aug; 478(2264):20220313. PubMed ID: 35966215
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Modeling of slightly-compressible isentropic flows and its compressibility effects on fluid-structure interactions.
    Zhang LT; Krane MH; Yu F
    Comput Fluids; 2019 Mar; 182():108-117. PubMed ID: 31327880
    [TBL] [Abstract][Full Text] [Related]  

  • 14. The breakdown of the anelastic approximation in rotating compressible convection: implications for astrophysical systems.
    Calkins MA; Julien K; Marti P
    Proc Math Phys Eng Sci; 2015 Mar; 471(2175):20140689. PubMed ID: 25792951
    [TBL] [Abstract][Full Text] [Related]  

  • 15. Excitation of inertial modes in an experimental spherical Couette flow.
    Rieutord M; Triana SA; Zimmerman DS; Lathrop DP
    Phys Rev E Stat Nonlin Soft Matter Phys; 2012 Aug; 86(2 Pt 2):026304. PubMed ID: 23005851
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Convection driven zonal flows and vortices in the major planets.
    Busse FH
    Chaos; 1994 Jun; 4(2):123-134. PubMed ID: 12780095
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Turbulent convective length scale in planetary cores.
    Guervilly C; Cardin P; Schaeffer N
    Nature; 2019 Jun; 570(7761):368-371. PubMed ID: 31217600
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Zonal wind driven by inertial modes.
    Tilgner A
    Phys Rev Lett; 2007 Nov; 99(19):194501. PubMed ID: 18233079
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Determination of the instantaneous geostrophic flow within the three-dimensional magnetostrophic regime.
    Hardy CM; Livermore PW; Niesen J; Luo J; Li K
    Proc Math Phys Eng Sci; 2018 Oct; 474(2218):20180412. PubMed ID: 30839837
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Plesio-geostrophy for Earth's core: I. Basic equations, inertial modes and induction.
    Jackson A; Maffei S
    Proc Math Phys Eng Sci; 2020 Nov; 476(2243):20200513. PubMed ID: 33362418
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 7.