BIOMARKERS

Molecular Biopsy of Human Tumors

- a resource for Precision Medicine *

136 related articles for article (PubMed ID: 33342385)

  • 1. 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]  

  • 2. A new method for detecting solar atmospheric gravity waves.
    Calchetti D; Jefferies SM; Fleck B; Berrilli F; Shcherbik DV
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200178. PubMed ID: 33342384
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Acoustic-gravity wave propagation characteristics in three-dimensional radiation hydrodynamic simulations of the solar atmosphere.
    Fleck B; Carlsson M; Khomenko E; Rempel M; Steiner O; Vigeesh G
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200170. PubMed ID: 33342376
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Transverse motions in sunspot super-penumbral fibrils.
    Morton RJ; Mooroogen K; Henriques VMJ
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200183. PubMed ID: 33342382
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Spectropolarimetric fluctuations in a sunspot chromosphere.
    Stangalini M; Baker D; Valori G; Jess DB; Jafarzadeh S; Murabito M; To ASH; Brooks DH; Ermolli I; Giorgi F; MacBride CD
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200216. PubMed ID: 33342387
    [TBL] [Abstract][Full Text] [Related]  

  • 6. High-resolution wave dynamics in the lower solar atmosphere.
    Jess DB; Keys PH; Stangalini M; Jafarzadeh S
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200169. PubMed ID: 33342388
    [TBL] [Abstract][Full Text] [Related]  

  • 7. On the effect of oscillatory phenomena on Stokes inversion results.
    Keys PH; Steiner O; Vigeesh G
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200182. PubMed ID: 33342373
    [TBL] [Abstract][Full Text] [Related]  

  • 8. 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]  

  • 9. Influence of ambipolar and Hall effects on vorticity in three-dimensional simulations of magneto-convection.
    Khomenko E; Collados M; Vitas N; González-Morales PA
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200176. PubMed ID: 33342386
    [TBL] [Abstract][Full Text] [Related]  

  • 10. High-frequency oscillations in small chromospheric bright features observed with Atacama Large Millimetre/Submillimetre Array.
    Guevara Gómez JC; Jafarzadeh S; Wedemeyer S; Szydlarski M; Stangalini M; Fleck B; Keys PH
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200184. PubMed ID: 33342381
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Mechanism of the effect of vertically propagating internal gravity waves on turbulence barrier and pollutant diffusion during heavy haze episodes.
    Wei Z; Zhang H; Wei W; Zhang X; Cai X; Song Y; Zhu T
    Sci Total Environ; 2022 Nov; 845():157349. PubMed ID: 35842150
    [TBL] [Abstract][Full Text] [Related]  

  • 12. 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]  

  • 13. Wave-vortex mode coupling in neutrally stable baroclinic flows.
    Salhi A; Pieri AB
    Phys Rev E Stat Nonlin Soft Matter Phys; 2014 Oct; 90(4):043003. PubMed ID: 25375590
    [TBL] [Abstract][Full Text] [Related]  

  • 14. Internal gravity waves in the energy and flux budget turbulence-closure theory for shear-free stably stratified flows.
    Kleeorin N; Rogachevskii I; Soustova IA; Troitskaya YI; Ermakova OS; Zilitinkevich S
    Phys Rev E; 2019 Jun; 99(6-1):063106. PubMed ID: 31330688
    [TBL] [Abstract][Full Text] [Related]  

  • 15. Characterization of shock wave signatures at millimetre wavelengths from Bifrost simulations.
    Eklund H; Wedemeyer S; Snow B; Jess DB; Jafarzadeh S; Grant SDT; Carlsson M; Szydlarski M
    Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200185. PubMed ID: 33342379
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Alfvén waves as a solar-interplanetary driver of the thermospheric disturbances.
    Guo J; Wei F; Feng X; Liu H; Wan W; Yang Z; Xu J; Liu C
    Sci Rep; 2016 Jan; 6():18895. PubMed ID: 26729294
    [TBL] [Abstract][Full Text] [Related]  

  • 17. 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]  

  • 18. 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]  

  • 19. 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]  

  • 20. 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]  

    [Next]    [New Search]
    of 7.