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 *

122 related articles for article (PubMed ID: 21490669)

  • 21. Magnetic reconnection in the interior of interplanetary coronal mass ejections.
    Fermo RL; Opher M; Drake JF
    Phys Rev Lett; 2014 Jul; 113(3):031101. PubMed ID: 25083630
    [TBL] [Abstract][Full Text] [Related]  

  • 22. Flare-productive active regions.
    Toriumi S; Wang H
    Living Rev Sol Phys; 2019; 16(1):3. PubMed ID: 31178676
    [TBL] [Abstract][Full Text] [Related]  

  • 23. Are there Alfvén waves in the solar atmosphere?
    Erdélyi R; Fedun V
    Science; 2007 Dec; 318(5856):1572-4. PubMed ID: 18063783
    [TBL] [Abstract][Full Text] [Related]  

  • 24. Explosive events on the Sun.
    Harra LK
    Philos Trans A Math Phys Eng Sci; 2002 Dec; 360(1801):2757-71. PubMed ID: 12630406
    [TBL] [Abstract][Full Text] [Related]  

  • 25. Probe of the solar magnetic field using the "cosmic-ray shadow" of the sun.
    Amenomori M; Bi XJ; Chen D; Chen TL; Chen WY; Cui SW; Danzengluobu ; Ding LK; Feng CF; Feng Z; Feng ZY; Gou QB; Guo YQ; Hakamada K; He HH; He ZT; Hibino K; Hotta N; Hu H; Hu HB; Huang J; Jia HY; Jiang L; Kajino F; Kasahara K; Katayose Y; Kato C; Kawata K; Labaciren ; Le GM; Li AF; Li HJ; Li WJ; Liu C; Liu JS; Liu MY; Lu H; Meng XR; Mizutani K; Munakata K; Nanjo H; Nishizawa M; Ohnishi M; Ohta I; Onuma H; Ozawa S; Qian XL; Qu XB; Saito T; Saito TY; Sakata M; Sako TK; Shao J; Shibata M; Shiomi A; Shirai T; Sugimoto H; Takita M; Tan YH; Tateyama N; Torii S; Tsuchiya H; Udo S; Wang H; Wu HR; Xue L; Yamamoto Y; Yang Z; Yasue S; Yuan AF; Yuda T; Zhai LM; Zhang HM; Zhang JL; Zhang XY; Zhang Y; Zhang Y; Zhang Y; Zhaxisangzhu ; Zhou XX
    Phys Rev Lett; 2013 Jul; 111(1):011101. PubMed ID: 24027782
    [TBL] [Abstract][Full Text] [Related]  

  • 26. Evolution of the Toroidal Flux of CME Flux Ropes during Eruption.
    Xing C; Cheng X; Ding M
    Innovation (Camb); 2020 Nov; 1(3):100059. PubMed ID: 34557723
    [TBL] [Abstract][Full Text] [Related]  

  • 27. Downward pumping of magnetic flux as the cause of filamentary structures in sunspot penumbrae.
    Thomas JH; Weiss NO; Tobias SM; Brummell NH
    Nature; 2002 Nov; 420(6914):390-3. PubMed ID: 12459777
    [TBL] [Abstract][Full Text] [Related]  

  • 28. Recent advances in coronal heating.
    De Moortel I; Browning P
    Philos Trans A Math Phys Eng Sci; 2015 May; 373(2042):. PubMed ID: 25897095
    [TBL] [Abstract][Full Text] [Related]  

  • 29. On the prevalence of small-scale twist in the solar chromosphere and transition region.
    De Pontieu B; van der Voort LR; McIntosh SW; Pereira TM; Carlsson M; Hansteen V; Skogsrud H; Lemen J; Title A; Boerner P; Hurlburt N; Tarbell TD; Wuelser JP; De Luca EE; Golub L; McKillop S; Reeves K; Saar S; Testa P; Tian H; Kankelborg C; Jaeggli S; Kleint L; Martinez-Sykora J
    Science; 2014 Oct; 346(6207):1255732. PubMed ID: 25324398
    [TBL] [Abstract][Full Text] [Related]  

  • 30. High-frequency torsional Alfvén waves as an energy source for coronal heating.
    Srivastava AK; Shetye J; Murawski K; Doyle JG; Stangalini M; Scullion E; Ray T; Wójcik DP; Dwivedi BN
    Sci Rep; 2017 Mar; 7():43147. PubMed ID: 28256538
    [TBL] [Abstract][Full Text] [Related]  

  • 31. A Twisted Flux Rope Model for Coronal Mass Ejections and Two-Ribbon Flares.
    Amari T; Luciani JF; Mikic Z; Linker J
    Astrophys J; 2000 Jan; 529(1):L49-L52. PubMed ID: 10615034
    [TBL] [Abstract][Full Text] [Related]  

  • 32. Understanding the Physical Nature of Coronal "EIT Waves".
    Long DM; Bloomfield DS; Chen PF; Downs C; Gallagher PT; Kwon RY; Vanninathan K; Veronig AM; Vourlidas A; Vršnak B; Warmuth A; Žic T
    Sol Phys; 2017; 292(1):7. PubMed ID: 28035169
    [TBL] [Abstract][Full Text] [Related]  

  • 33. Ground-based observation of emission lines from the corona of a red-dwarf star.
    Schmitt JH; Wichmann R
    Nature; 2001 Aug; 412(6846):508-10. PubMed ID: 11484044
    [TBL] [Abstract][Full Text] [Related]  

  • 34. Solar Open Flux Migration from Pole to Pole: Magnetic Field Reversal.
    Huang GH; Lin CH; Lee LC
    Sci Rep; 2017 Aug; 7(1):9488. PubMed ID: 28842682
    [TBL] [Abstract][Full Text] [Related]  

  • 35. The role of turbulence in coronal heating and solar wind expansion.
    Cranmer SR; Asgari-Targhi M; Miralles MP; Raymond JC; Strachan L; Tian H; Woolsey LN
    Philos Trans A Math Phys Eng Sci; 2015 May; 373(2041):. PubMed ID: 25848083
    [TBL] [Abstract][Full Text] [Related]  

  • 36. What can large-scale magnetohydrodynamic numerical experiments tell us about coronal heating?
    Peter H
    Philos Trans A Math Phys Eng Sci; 2015 May; 373(2042):. PubMed ID: 25897097
    [TBL] [Abstract][Full Text] [Related]  

  • 37. An overview of coronal seismology.
    De Moortel I
    Philos Trans A Math Phys Eng Sci; 2005 Dec; 363(1837):2743-60. PubMed ID: 16286288
    [TBL] [Abstract][Full Text] [Related]  

  • 38. Destruction of Sun-grazing comet C/2011 N3 (SOHO) within the low solar corona.
    Schrijver CJ; Brown JC; Battams K; Saint-Hilaire P; Liu W; Hudson H; Pesnell WD
    Science; 2012 Jan; 335(6066):324-8. PubMed ID: 22267810
    [TBL] [Abstract][Full Text] [Related]  

  • 39. Geometric considerations of the evolution of magnetic flux ropes.
    Berdichevsky DB; Lepping RP; Farrugia CJ
    Phys Rev E Stat Nonlin Soft Matter Phys; 2003 Mar; 67(3 Pt 2):036405. PubMed ID: 12689169
    [TBL] [Abstract][Full Text] [Related]  

  • 40. Solar Prominence Modelling and Plasma Diagnostics at ALMA Wavelengths.
    Rodger A; Labrosse N
    Sol Phys; 2017; 292(9):130. PubMed ID: 32009680
    [TBL] [Abstract][Full Text] [Related]  

    [Previous]   [Next]    [New Search]
    of 7.