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 *

126 related articles for article (PubMed ID: 39196945)

  • 1. Inertial range of magnetorotational turbulence.
    Kawazura Y; Kimura SS
    Sci Adv; 2024 Aug; 10(35):eadp4965. PubMed ID: 39196945
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Magnetorotational Turbulence and Dynamo in a Collisionless Plasma.
    Kunz MW; Stone JM; Quataert E
    Phys Rev Lett; 2016 Dec; 117(23):235101. PubMed ID: 27982637
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Inertial-range dynamics and scaling laws of two-dimensional magnetohydrodynamic turbulence in the weak-field regime.
    Blackbourn LA; Tran CV
    Phys Rev E Stat Nonlin Soft Matter Phys; 2014 Aug; 90(2):023012. PubMed ID: 25215825
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Dynamic Phase Alignment in Inertial Alfvén Turbulence.
    Milanese LM; Loureiro NF; Daschner M; Boldyrev S
    Phys Rev Lett; 2020 Dec; 125(26):265101. PubMed ID: 33449762
    [TBL] [Abstract][Full Text] [Related]  

  • 5. A large-scale dynamo and magnetoturbulence in rapidly rotating core-collapse supernovae.
    Mösta P; Ott CD; Radice D; Roberts LF; Schnetter E; Haas R
    Nature; 2015 Dec; 528(7582):376-9. PubMed ID: 26618868
    [TBL] [Abstract][Full Text] [Related]  

  • 6. Spectrum of magnetohydrodynamic turbulence.
    Boldyrev S
    Phys Rev Lett; 2006 Mar; 96(11):115002. PubMed ID: 16605832
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Global Simulations of Differentially Rotating Magnetized Disks: Formation of Low-beta Filaments and Structured Coronae.
    Machida M; Hayashi MR; Matsumoto R
    Astrophys J; 2000 Mar; 532(1):L67-L70. PubMed ID: 10702134
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Periodic magnetorotational dynamo action as a prototype of nonlinear magnetic-field generation in shear flows.
    Herault J; Rincon F; Cossu C; Lesur G; Ogilvie GI; Longaretti PY
    Phys Rev E Stat Nonlin Soft Matter Phys; 2011 Sep; 84(3 Pt 2):036321. PubMed ID: 22060506
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Compressible Magnetohydrodynamic Turbulence in the Earth's Magnetosheath: Estimation of the Energy Cascade Rate Using in situ Spacecraft Data.
    Hadid LZ; Sahraoui F; Galtier S; Huang SY
    Phys Rev Lett; 2018 Feb; 120(5):055102. PubMed ID: 29481187
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Origin of nonlinearity and plausible turbulence by hydromagnetic transient growth in accretion disks: Faster growth rate than magnetorotational instability.
    Nath SK; Mukhopadhyay B
    Phys Rev E Stat Nonlin Soft Matter Phys; 2015 Aug; 92(2):023005. PubMed ID: 26382501
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Scale locality of magnetohydrodynamic turbulence.
    Aluie H; Eyink GL
    Phys Rev Lett; 2010 Feb; 104(8):081101. PubMed ID: 20366924
    [TBL] [Abstract][Full Text] [Related]  

  • 12. Identification of a non-axisymmetric mode in laboratory experiments searching for standard magnetorotational instability.
    Wang Y; Gilson EP; Ebrahimi F; Goodman J; Caspary KJ; Winarto HW; Ji H
    Nat Commun; 2022 Aug; 13(1):4679. PubMed ID: 35945242
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Nonhelical inverse transfer of a decaying turbulent magnetic field.
    Brandenburg A; Kahniashvili T; Tevzadze AG
    Phys Rev Lett; 2015 Feb; 114(7):075001. PubMed ID: 25763960
    [TBL] [Abstract][Full Text] [Related]  

  • 14. First observation of fluid-like eddy-dominant bursty bulk flow turbulence in the Earth's tail plasma sheet.
    Zhang LQ; Wang C; Baumjohann W; Wang RS; Wang JY; Burch JL; Khotyaintsev YV
    Sci Rep; 2023 Nov; 13(1):19201. PubMed ID: 37932297
    [TBL] [Abstract][Full Text] [Related]  

  • 15. Hydrodynamic turbulence cannot transport angular momentum effectively in astrophysical disks.
    Ji H; Burin M; Schartman E; Goodman J
    Nature; 2006 Nov; 444(7117):343-6. PubMed ID: 17108959
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Exact law for homogeneous compressible Hall magnetohydrodynamics turbulence.
    Andrés N; Galtier S; Sahraoui F
    Phys Rev E; 2018 Jan; 97(1-1):013204. PubMed ID: 29448457
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Fully resolved array of simulations investigating the influence of the magnetic Prandtl number on magnetohydrodynamic turbulence.
    McKay ME; Berera A; Ho RDJG
    Phys Rev E; 2019 Jan; 99(1-1):013101. PubMed ID: 30780321
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Local model for angular-momentum transport in accretion disks driven by the magnetorotational instability.
    Pessah ME; Chan CK; Psaltis D
    Phys Rev Lett; 2006 Dec; 97(22):221103. PubMed ID: 17155789
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Two-dimensional state in driven magnetohydrodynamic turbulence.
    Bigot B; Galtier S
    Phys Rev E Stat Nonlin Soft Matter Phys; 2011 Feb; 83(2 Pt 2):026405. PubMed ID: 21405916
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Unified treatment of mean-field dynamo and angular-momentum transport in magnetorotational instability-driven turbulence.
    Mondal T; Bhat P
    Phys Rev E; 2023 Dec; 108(6-2):065201. PubMed ID: 38243446
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 7.