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 *

154 related articles for article (PubMed ID: 22665893)

  • 21. Small-scale dynamo magnetism as the driver for heating the solar atmosphere.
    Amari T; Luciani JF; Aly JJ
    Nature; 2015 Jun; 522(7555):188-91. PubMed ID: 26062509
    [TBL] [Abstract][Full Text] [Related]  

  • 22. Analysis of the electrolyte convection inside the concentration boundary layer during structured electrodeposition of copper in high magnetic gradient fields.
    König J; Tschulik K; Büttner L; Uhlemann M; Czarske J
    Anal Chem; 2013 Mar; 85(6):3087-94. PubMed ID: 23432054
    [TBL] [Abstract][Full Text] [Related]  

  • 23. Stripping analysis of mercury(II) ionic solutions under magneto-hydrodynamic convection.
    Panta YM; Qian S; Cheney MA
    J Colloid Interface Sci; 2008 Jan; 317(1):175-82. PubMed ID: 17919650
    [TBL] [Abstract][Full Text] [Related]  

  • 24. Numerical modelling of MHD waves in the solar chromosphere.
    Carlsson M; Bogdan TJ
    Philos Trans A Math Phys Eng Sci; 2006 Feb; 364(1839):395-404. PubMed ID: 16414886
    [TBL] [Abstract][Full Text] [Related]  

  • 25. Imaging sunspots using helioseismic methods.
    Tong CH
    Philos Trans A Math Phys Eng Sci; 2005 Dec; 363(1837):2761-75. PubMed ID: 16286289
    [TBL] [Abstract][Full Text] [Related]  

  • 26. 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]  

  • 27. Solar-type dynamo behaviour in fully convective stars without a tachocline.
    Wright NJ; Drake JJ
    Nature; 2016 Jul; 535(7613):526-8. PubMed ID: 27466124
    [TBL] [Abstract][Full Text] [Related]  

  • 28. High-frequency acoustic waves are not sufficient to heat the solar chromosphere.
    Fossum A; Carlsson M
    Nature; 2005 Jun; 435(7044):919-21. PubMed ID: 15959510
    [TBL] [Abstract][Full Text] [Related]  

  • 29. Alfvénic waves with sufficient energy to power the quiet solar corona and fast solar wind.
    McIntosh SW; De Pontieu B; Carlsson M; Hansteen V; Boerner P; Goossens M
    Nature; 2011 Jul; 475(7357):477-80. PubMed ID: 21796206
    [TBL] [Abstract][Full Text] [Related]  

  • 30. Anomalously weak solar convection.
    Hanasoge SM; Duvall TL; Sreenivasan KR
    Proc Natl Acad Sci U S A; 2012 Jul; 109(30):11928-32. PubMed ID: 22665774
    [TBL] [Abstract][Full Text] [Related]  

  • 31. Large-scale solar magnetic field mapping: I.
    Schatten KH
    Springerplus; 2013 Dec; 2(1):21. PubMed ID: 23518616
    [TBL] [Abstract][Full Text] [Related]  

  • 32. Approaching a realistic force balance in geodynamo simulations.
    Yadav RK; Gastine T; Christensen UR; Wolk SJ; Poppenhaeger K
    Proc Natl Acad Sci U S A; 2016 Oct; 113(43):12065-12070. PubMed ID: 27790991
    [TBL] [Abstract][Full Text] [Related]  

  • 33. Chromospheric alfvenic waves strong enough to power the solar wind.
    De Pontieu B; McIntosh SW; Carlsson M; Hansteen VH; Tarbell TD; Schrijver CJ; Title AM; Shine RA; Tsuneta S; Katsukawa Y; Ichimoto K; Suematsu Y; Shimizu T; Nagata S
    Science; 2007 Dec; 318(5856):1574-7. PubMed ID: 18063784
    [TBL] [Abstract][Full Text] [Related]  

  • 34. The cross-over to magnetostrophic convection in planetary dynamo systems.
    Aurnou JM; King EM
    Proc Math Phys Eng Sci; 2017 Mar; 473(2199):20160731. PubMed ID: 28413338
    [TBL] [Abstract][Full Text] [Related]  

  • 35. The quiet-Sun photosphere and chromosphere.
    Rutten RJ
    Philos Trans A Math Phys Eng Sci; 2012 Jul; 370(1970):3129-50. PubMed ID: 22665896
    [TBL] [Abstract][Full Text] [Related]  

  • 36. Thermally driven rossby-mode dynamo for solar magnetic-field reversals.
    Gilman PA
    Science; 1968 May; 160(3829):760-3. PubMed ID: 17784314
    [TBL] [Abstract][Full Text] [Related]  

  • 37. Magnetism, dynamo action and the solar-stellar connection.
    Brun AS; Browning MK
    Living Rev Sol Phys; 2017; 14(1):4. PubMed ID: 31997984
    [TBL] [Abstract][Full Text] [Related]  

  • 38. Suppression of cooling by strong magnetic fields in white dwarf stars.
    Valyavin G; Shulyak D; Wade GA; Antonyuk K; Zharikov SV; Galazutdinov GA; Plachinda S; Bagnulo S; Machado LF; Alvarez M; Clark DM; Lopez JM; Hiriart D; Han I; Jeon YB; Zurita C; Mujica R; Burlakova T; Szeifert T; Burenkov A
    Nature; 2014 Nov; 515(7525):88-91. PubMed ID: 25327247
    [TBL] [Abstract][Full Text] [Related]  

  • 39. An early lunar core dynamo driven by thermochemical mantle convection.
    Stegman DR; Jellinek AM; Zatman SA; Baumgardner JR; Richards MA
    Nature; 2003 Jan; 421(6919):143-6. PubMed ID: 12520295
    [TBL] [Abstract][Full Text] [Related]  

  • 40. Magnetostrophic balance as the optimal state for turbulent magnetoconvection.
    King EM; Aurnou JM
    Proc Natl Acad Sci U S A; 2015 Jan; 112(4):990-4. PubMed ID: 25583512
    [TBL] [Abstract][Full Text] [Related]  

    [Previous]   [Next]    [New Search]
    of 8.