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 *

237 related articles for article (PubMed ID: 17677760)

  • 21. Solar origins of solar wind properties during the cycle 23 solar minimum and rising phase of cycle 24.
    Luhmann JG; Petrie G; Riley P
    J Adv Res; 2013 May; 4(3):221-8. PubMed ID: 25685422
    [TBL] [Abstract][Full Text] [Related]  

  • 22. Generalized similarity in finite range solar wind magnetohydrodynamic turbulence.
    Chapman SC; Nicol RM
    Phys Rev Lett; 2009 Dec; 103(24):241101. PubMed ID: 20366193
    [TBL] [Abstract][Full Text] [Related]  

  • 23. Inertial-Range Reconnection in Magnetohydrodynamic Turbulence and in the Solar Wind.
    Lalescu CC; Shi YK; Eyink GL; Drivas TD; Vishniac ET; Lazarian A
    Phys Rev Lett; 2015 Jul; 115(2):025001. PubMed ID: 26207472
    [TBL] [Abstract][Full Text] [Related]  

  • 24. Continuous plasma outflows from the edge of a solar active region as a possible source of solar wind.
    Sakao T; Kano R; Narukage N; Kotoku J; Bando T; Deluca EE; Lundquist LL; Tsuneta S; Harra LK; Katsukawa Y; Kubo M; Hara H; Matsuzaki K; Shimojo M; Bookbinder JA; Golub L; Korreck KE; Su Y; Shibasaki K; Shimizu T; Nakatani I
    Science; 2007 Dec; 318(5856):1585-8. PubMed ID: 18063788
    [TBL] [Abstract][Full Text] [Related]  

  • 25. 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]  

  • 26. Measurement of the electric fluctuation spectrum of magnetohydrodynamic turbulence.
    Bale SD; Kellogg PJ; Mozer FS; Horbury TS; Reme H
    Phys Rev Lett; 2005 Jun; 94(21):215002. PubMed ID: 16090328
    [TBL] [Abstract][Full Text] [Related]  

  • 27. Reconnection-Driven Magnetohydrodynamic Turbulence in a Simulated Coronal-Hole Jet.
    Uritsky VM; Roberts MA; DeVore CR; Karpen JT
    Astrophys J; 2017 Mar; 837(No 2):. PubMed ID: 29430025
    [TBL] [Abstract][Full Text] [Related]  

  • 28. MHD waves and oscillations in the solar plasma. Introduction.
    Erdélyi R
    Philos Trans A Math Phys Eng Sci; 2006 Feb; 364(1839):289-96. PubMed ID: 16414880
    [TBL] [Abstract][Full Text] [Related]  

  • 29. Coronal magnetohydrodynamic waves and oscillations: observations and quests.
    Aschwanden MJ
    Philos Trans A Math Phys Eng Sci; 2006 Feb; 364(1839):417-32; discussion 432. PubMed ID: 16414888
    [TBL] [Abstract][Full Text] [Related]  

  • 30. 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]  

  • 31. 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]  

  • 32. Amplitude fluctuations for optical waves propagation through non-Kolmogorov coronal solar wind turbulence channels.
    Xu G; Song Z
    Opt Express; 2018 Apr; 26(7):8566-8580. PubMed ID: 29715822
    [TBL] [Abstract][Full Text] [Related]  

  • 33. Induced emission of Alfvén waves in inhomogeneous streaming plasma: implications for solar corona heating and solar wind acceleration.
    Galinsky VL; Shevchenko VI
    Phys Rev Lett; 2013 Jul; 111(1):015004. PubMed ID: 23863008
    [TBL] [Abstract][Full Text] [Related]  

  • 34. Models of coronal heating, turbulence and fast reconnection.
    Velli M; Pucci F; Rappazzo F; Tenerani A
    Philos Trans A Math Phys Eng Sci; 2015 May; 373(2042):. PubMed ID: 25897086
    [TBL] [Abstract][Full Text] [Related]  

  • 35. Self-Similar Theory of Thermal Conduction and Application to the Solar Wind.
    Horaites K; Boldyrev S; Krasheninnikov SI; Salem C; Bale SD; Pulupa M
    Phys Rev Lett; 2015 Jun; 114(24):245003. PubMed ID: 26196982
    [TBL] [Abstract][Full Text] [Related]  

  • 36. Probabilistic Solar Wind Forecasting Using Large Ensembles of Near-Sun Conditions With a Simple One-Dimensional "Upwind" Scheme.
    Owens MJ; Riley P
    Space Weather; 2017 Nov; 15(11):1461-1474. PubMed ID: 29398982
    [TBL] [Abstract][Full Text] [Related]  

  • 37. 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]  

  • 38. Two-dimensional kinetic turbulence in the solar wind.
    Valentini F; Califano F; Veltri P
    Phys Rev Lett; 2010 May; 104(20):205002. PubMed ID: 20867033
    [TBL] [Abstract][Full Text] [Related]  

  • 39. Three-dimensional magnetic field topology in a region of solar coronal heating.
    Solanki SK; Lagg A; Woch J; Krupp N; Collados M
    Nature; 2003 Oct; 425(6959):692-5. PubMed ID: 14562096
    [TBL] [Abstract][Full Text] [Related]  

  • 40. Probability distributions of turbulent energy.
    Momeni M; Müller WC
    Phys Rev E Stat Nonlin Soft Matter Phys; 2008 May; 77(5 Pt 2):056401. PubMed ID: 18643170
    [TBL] [Abstract][Full Text] [Related]  

    [Previous]   [Next]    [New Search]
    of 12.