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 *

234 related articles for article (PubMed ID: 19905703)

  • 1. Universality of solar-wind turbulent spectrum from MHD to electron scales.
    Alexandrova O; Saur J; Lacombe C; Mangeney A; Mitchell J; Schwartz SJ; Robert P
    Phys Rev Lett; 2009 Oct; 103(16):165003. PubMed ID: 19905703
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Gyrokinetic simulations of solar wind turbulence from ion to electron scales.
    Howes GG; TenBarge JM; Dorland W; Quataert E; Schekochihin AA; Numata R; Tatsuno T
    Phys Rev Lett; 2011 Jul; 107(3):035004. PubMed ID: 21838370
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Spectrum of kinetic plasma turbulence at 0.3-0.9 astronomical units from the Sun.
    Alexandrova O; Jagarlamudi VK; Hellinger P; Maksimovic M; Shprits Y; Mangeney A
    Phys Rev E; 2021 Jun; 103(6-1):063202. PubMed ID: 34271660
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Evidence of a cascade and dissipation of solar-wind turbulence at the electron gyroscale.
    Sahraoui F; Goldstein ML; Robert P; Khotyaintsev YV
    Phys Rev Lett; 2009 Jun; 102(23):231102. PubMed ID: 19658919
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Detection of small-scale structures in the dissipation regime of solar-wind turbulence.
    Perri S; Goldstein ML; Dorelli JC; Sahraoui F
    Phys Rev Lett; 2012 Nov; 109(19):191101. PubMed ID: 23215371
    [TBL] [Abstract][Full Text] [Related]  

  • 6. 3D simulations of fluctuation spectra in the hall-MHD plasma.
    Shaikh D; Shukla PK
    Phys Rev Lett; 2009 Jan; 102(4):045004. PubMed ID: 19257431
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Three dimensional anisotropic κ spectra of turbulence at subproton scales in the solar wind.
    Sahraoui F; Goldstein ML; Belmont G; Canu P; Rezeau L
    Phys Rev Lett; 2010 Sep; 105(13):131101. PubMed ID: 21230758
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Multiscale Nature of the Dissipation Range in Gyrokinetic Simulations of Alfvénic Turbulence.
    Told D; Jenko F; TenBarge JM; Howes GG; Hammett GW
    Phys Rev Lett; 2015 Jul; 115(2):025003. PubMed ID: 26207474
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Dissipation and heating in solar wind turbulence: from the macro to the micro and back again.
    Kiyani KH; Osman KT; Chapman SC
    Philos Trans A Math Phys Eng Sci; 2015 May; 373(2041):. PubMed ID: 25848077
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Cross-scale effects in solar-wind turbulence.
    Valentini F; Veltri P; Califano F; Mangeney A
    Phys Rev Lett; 2008 Jul; 101(2):025006. PubMed ID: 18764190
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Permutation entropy and statistical complexity analysis of turbulence in laboratory plasmas and the solar wind.
    Weck PJ; Schaffner DA; Brown MR; Wicks RT
    Phys Rev E Stat Nonlin Soft Matter Phys; 2015 Feb; 91(2):023101. PubMed ID: 25768612
    [TBL] [Abstract][Full Text] [Related]  

  • 12. Density fluctuation spectrum of solar wind turbulence between ion and electron scales.
    Chen CH; Salem CS; Bonnell JW; Mozer FS; Bale SD
    Phys Rev Lett; 2012 Jul; 109(3):035001. PubMed ID: 22861861
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Intermittency, scaling, and the Fokker-Planck approach to fluctuations of the solar wind bulk plasma parameters as seen by the WIND spacecraft.
    Hnat B; Chapman SC; Rowlands G
    Phys Rev E Stat Nonlin Soft Matter Phys; 2003 May; 67(5 Pt 2):056404. PubMed ID: 12786284
    [TBL] [Abstract][Full Text] [Related]  

  • 14. Fluidization of collisionless plasma turbulence.
    Meyrand R; Kanekar A; Dorland W; Schekochihin AA
    Proc Natl Acad Sci U S A; 2019 Jan; 116(4):1185-1194. PubMed ID: 30610178
    [TBL] [Abstract][Full Text] [Related]  

  • 15. Global scale-invariant dissipation in collisionless plasma turbulence.
    Kiyani KH; Chapman SC; Khotyaintsev YV; Dunlop MW; Sahraoui F
    Phys Rev Lett; 2009 Aug; 103(7):075006. PubMed ID: 19792654
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Kinetic simulations of magnetized turbulence in astrophysical plasmas.
    Howes GG; Dorland W; Cowley SC; Hammett GW; Quataert E; Schekochihin AA; Tatsuno T
    Phys Rev Lett; 2008 Feb; 100(6):065004. PubMed ID: 18352484
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Nonlocal contributions to the turbulent cascade in magnetohydrodynamic plasmas.
    Friedrich J; Wilbert M; Marino R
    Phys Rev E; 2024 Apr; 109(4-2):045208. PubMed ID: 38755856
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Scaling laws of turbulence and heating of fast solar wind: the role of density fluctuations.
    Carbone V; Marino R; Sorriso-Valvo L; Noullez A; Bruno R
    Phys Rev Lett; 2009 Aug; 103(6):061102. PubMed ID: 19792547
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Magnetic discontinuities in magnetohydrodynamic turbulence and in the solar wind.
    Zhdankin V; Boldyrev S; Mason J; Perez JC
    Phys Rev Lett; 2012 Apr; 108(17):175004. PubMed ID: 22680875
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Spontaneous chiral symmetry breaking of Hall magnetohydrodynamic turbulence.
    Meyrand R; Galtier S
    Phys Rev Lett; 2012 Nov; 109(19):194501. PubMed ID: 23215387
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 12.