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 *

177 related articles for article (PubMed ID: 25897091)

  • 1. Wave heating of the solar atmosphere.
    Arregui I
    Philos Trans A Math Phys Eng Sci; 2015 May; 373(2042):. PubMed ID: 25897091
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Nonlinear waves in the solar atmosphere.
    Ruderman MS
    Philos Trans A Math Phys Eng Sci; 2006 Feb; 364(1839):485-504. PubMed ID: 16414893
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Is magnetic topology important for heating the solar atmosphere?
    Parnell CE; Stevenson JE; Threlfall J; Edwards SJ
    Philos Trans A Math Phys Eng Sci; 2015 May; 373(2042):. PubMed ID: 25897085
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Evidence for wave heating in the solar corona.
    Hahn M
    Ann N Y Acad Sci; 2013 Jul; 1293():45-53. PubMed ID: 23676178
    [TBL] [Abstract][Full Text] [Related]  

  • 5. 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]  

  • 6. 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]  

  • 7. 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]  

  • 8. 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]  

  • 9. 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]  

  • 10. 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]  

  • 11. Investigating Alfvénic wave propagation in coronal open-field regions.
    Morton RJ; Tomczyk S; Pinto R
    Nat Commun; 2015 Jul; 6():7813. PubMed ID: 26213234
    [TBL] [Abstract][Full Text] [Related]  

  • 12. On the influence of magnetic topology on the propagation of internal gravity waves in the solar atmosphere.
    Vigeesh G; Roth M; Steiner O; Fleck B
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200177. PubMed ID: 33342385
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Wave Modeling of the Solar Wind.
    Ofman L
    Living Rev Sol Phys; 2010; 7():4. PubMed ID: 27194962
    [TBL] [Abstract][Full Text] [Related]  

  • 14. Solar Coronal Jets: Observations, Theory, and Modeling.
    Raouafi NE; Patsourakos S; Pariat E; Young PR; Sterling A; Savcheva A; Shimojo M; Moreno-Insertis F; DeVore CR; Archontis V; Török T; Mason H; Curdt W; Meyer K; Dalmasse K; Matsui Y
    Space Sci Rev; 2016 Jul; 201():1-53. PubMed ID: 32908324
    [TBL] [Abstract][Full Text] [Related]  

  • 15. A Solar cycle correlation of coronal element abundances in Sun-as-a-star observations.
    Brooks DH; Baker D; van Driel-Gesztelyi L; Warren HP
    Nat Commun; 2017 Aug; 8(1):183. PubMed ID: 28775304
    [TBL] [Abstract][Full Text] [Related]  

  • 16. 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]  

  • 17. Magnetoacoustic wave energy dissipation in the atmosphere of solar pores.
    Gilchrist-Millar CA; Jess DB; Grant SDT; Keys PH; Beck C; Jafarzadeh S; Riedl JM; Van Doorsselaere T; Ruiz Cobo B
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200172. PubMed ID: 33342383
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Reflection of Fast Magnetosonic Waves near a Magnetic Reconnection Region.
    Provornikova E; Laming JM; Lukin VS
    Astrophys J; 2018 Jun; 860(2):. PubMed ID: 32690976
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Stellar activity and coronal heating: an overview of recent results.
    Testa P; Saar SH; Drake JJ
    Philos Trans A Math Phys Eng Sci; 2015 May; 373(2042):. PubMed ID: 25897087
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Observations of ubiquitous compressive waves in the Sun's chromosphere.
    Morton RJ; Verth G; Jess DB; Kuridze D; Ruderman MS; Mathioudakis M; Erdélyi R
    Nat Commun; 2012; 3():1315. PubMed ID: 23271649
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 9.