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 *

223 related articles for article (PubMed ID: 35479733)

  • 1. Data-driven modeling of solar coronal magnetic field evolution and eruptions.
    Jiang C; Feng X; Guo Y; Hu Q
    Innovation (Camb); 2022 May; 3(3):100236. PubMed ID: 35479733
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Introduction to the physics of solar eruptions and their space weather impact.
    Archontis V; Vlahos L
    Philos Trans A Math Phys Eng Sci; 2019 Jul; 377(2148):20190152. PubMed ID: 31079579
    [TBL] [Abstract][Full Text] [Related]  

  • 3. EVIDENCE FOR THE MAGNETIC BREAKOUT MODEL IN AN EQUATORIAL CORONAL-HOLE JET.
    Kumar P; Karpen JT; Antiochos SK; Wyper PF; Devore CR; Deforest CE
    Astrophys J; 2018 Feb; 854(2):. PubMed ID: 33867543
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Earth-affecting solar transients: a review of progresses in solar cycle 24.
    Zhang J; Temmer M; Gopalswamy N; Malandraki O; Nitta NV; Patsourakos S; Shen F; Vršnak B; Wang Y; Webb D; Desai MI; Dissauer K; Dresing N; Dumbović M; Feng X; Heinemann SG; Laurenza M; Lugaz N; Zhuang B
    Prog Earth Planet Sci; 2021; 8(1):56. PubMed ID: 34722120
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Understanding the Origins of Problem Geomagnetic Storms Associated with "Stealth" Coronal Mass Ejections.
    Nitta NV; Mulligan T; Kilpua EKJ; Lynch BJ; Mierla M; O'Kane J; Pagano P; Palmerio E; Pomoell J; Richardson IR; Rodriguez L; Rouillard AP; Sinha S; Srivastava N; Talpeanu DC; Yardley SL; Zhukov AN
    Space Sci Rev; 2021; 217(8):82. PubMed ID: 34789949
    [TBL] [Abstract][Full Text] [Related]  

  • 6. Modeling a Carrington-scale Stellar Superflare and Coronal Mass Ejection from
    Lynch BJ; Airapetian VS; DeVore CR; Kazachenko MD; Lüftinger T; Kochukhov O; Rosén L; Abbett WP
    Astrophys J; 2019 Aug; 880(2):. PubMed ID: 32214410
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Sources of solar energetic particles.
    Vlahos L; Anastasiadis A; Papaioannou A; Kouloumvakos A; Isliker H
    Philos Trans A Math Phys Eng Sci; 2019 Jul; 377(2148):20180095. PubMed ID: 31079581
    [TBL] [Abstract][Full Text] [Related]  

  • 8. 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]  

  • 9. Time-dependent Data-driven Modeling of Active Region Evolution Using Energy-optimized Photospheric Electric Fields.
    Pomoell J; Lumme E; Kilpua E
    Sol Phys; 2019; 294(4):41. PubMed ID: 31057187
    [TBL] [Abstract][Full Text] [Related]  

  • 10. SUN-TO-EARTH MHD SIMULATION OF THE 14 JULY 2000 "BASTILLE DAY" ERUPTION.
    Török T; Downs C; Linker JA; Lionello R; Titov VS; Mikić Z; Riley P; Caplan RM; Wijaya J
    Astrophys J; 2018 Mar; 856(1):. PubMed ID: 29628520
    [TBL] [Abstract][Full Text] [Related]  

  • 11. A universal model for solar eruptions.
    Wyper PF; Antiochos SK; DeVore CR
    Nature; 2017 Apr; 544(7651):452-455. PubMed ID: 28447632
    [TBL] [Abstract][Full Text] [Related]  

  • 12. The emergence of magnetic flux and its role on the onset of solar dynamic events.
    Archontis V; Syntelis P
    Philos Trans A Math Phys Eng Sci; 2019 Jul; 377(2148):20180387. PubMed ID: 31079584
    [TBL] [Abstract][Full Text] [Related]  

  • 13. A dynamic magnetic tension force as the cause of failed solar eruptions.
    Myers CE; Yamada M; Ji H; Yoo J; Fox W; Jara-Almonte J; Savcheva A; DeLuca EE
    Nature; 2015 Dec; 528(7583):526-9. PubMed ID: 26701052
    [TBL] [Abstract][Full Text] [Related]  

  • 14. The source and engine of coronal mass ejections.
    Georgoulis MK; Nindos A; Zhang H
    Philos Trans A Math Phys Eng Sci; 2019 Jul; 377(2148):20180094. PubMed ID: 31079580
    [TBL] [Abstract][Full Text] [Related]  

  • 15. 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]  

  • 16. Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption.
    Jiang C; Wu ST; Feng X; Hu Q
    Nat Commun; 2016 May; 7():11522. PubMed ID: 27181846
    [TBL] [Abstract][Full Text] [Related]  

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

  • 18. Coronal mass ejections are not coherent magnetohydrodynamic structures.
    Owens MJ; Lockwood M; Barnard LA
    Sci Rep; 2017 Jun; 7(1):4152. PubMed ID: 28646228
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Coronal Holes.
    Cranmer SR
    Living Rev Sol Phys; 2009; 6():3. PubMed ID: 27194961
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Forward Modeling of Coronal Mass Ejection Flux Ropes in the Inner Heliosphere with 3DCORE.
    Möstl C; Amerstorfer T; Palmerio E; Isavnin A; Farrugia CJ; Lowder C; Winslow RM; Donnerer JM; Kilpua EKJ; Boakes PD
    Space Weather; 2018 Mar; 16(3):216-229. PubMed ID: 29780287
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 12.