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 *

205 related articles for article (PubMed ID: 25562705)

  • 1. Full-Sun observations for identifying the source of the slow solar wind.
    Brooks DH; Ugarte-Urra I; Warren HP
    Nat Commun; 2015 Jan; 6():5947. PubMed ID: 25562705
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Continuous plasma outflows from the edge of a solar active region as a possible source of solar wind.
    Sakao T; Kano R; Narukage N; Kotoku J; Bando T; Deluca EE; Lundquist LL; Tsuneta S; Harra LK; Katsukawa Y; Kubo M; Hara H; Matsuzaki K; Shimojo M; Bookbinder JA; Golub L; Korreck KE; Su Y; Shibasaki K; Shimizu T; Nakatani I
    Science; 2007 Dec; 318(5856):1585-8. PubMed ID: 18063788
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Sources of solar wind over the solar activity cycle.
    Poletto G
    J Adv Res; 2013 May; 4(3):215-20. PubMed ID: 25685421
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Highly structured slow solar wind emerging from an equatorial coronal hole.
    Bale SD; Badman ST; Bonnell JW; Bowen TA; Burgess D; Case AW; Cattell CA; Chandran BDG; Chaston CC; Chen CHK; Drake JF; de Wit TD; Eastwood JP; Ergun RE; Farrell WM; Fong C; Goetz K; Goldstein M; Goodrich KA; Harvey PR; Horbury TS; Howes GG; Kasper JC; Kellogg PJ; Klimchuk JA; Korreck KE; Krasnoselskikh VV; Krucker S; Laker R; Larson DE; MacDowall RJ; Maksimovic M; Malaspina DM; Martinez-Oliveros J; McComas DJ; Meyer-Vernet N; Moncuquet M; Mozer FS; Phan TD; Pulupa M; Raouafi NE; Salem C; Stansby D; Stevens M; Szabo A; Velli M; Woolley T; Wygant JR
    Nature; 2019 Dec; 576(7786):237-242. PubMed ID: 31802007
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Interchange reconnection as the source of the fast solar wind within coronal holes.
    Bale SD; Drake JF; McManus MD; Desai MI; Badman ST; Larson DE; Swisdak M; Horbury TS; Raouafi NE; Phan T; Velli M; McComas DJ; Cohen CMS; Mitchell D; Panasenco O; Kasper JC
    Nature; 2023 Jun; 618(7964):252-256. PubMed ID: 37286648
    [TBL] [Abstract][Full Text] [Related]  

  • 6. The sun and heliosphere at solar maximum.
    Smith EJ; Marsden RG; Balogh A; Gloeckler G; Geiss J; McComas DJ; McKibben RB; MacDowall RJ; Lanzerotti LJ; Krupp N; Krueger H; Landgraf M
    Science; 2003 Nov; 302(5648):1165-9. PubMed ID: 14615526
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Magnetic Field Geometry and Composition Variation in Slow Solar Winds: The Case of Sulfur.
    Kuroda N; Laming JM
    Astrophys J; 2020 May; 895(1):. PubMed ID: 32699430
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Searching for a Solar Source of Magnetic-Field Switchbacks in Parker Solar Probe's First Encounter.
    de Pablos D; Samanta T; Badman ST; Schwanitz C; Bahauddin SM; Harra LK; Petrie G; Mac Cormack C; Mandrini CH; Raouafi NE; Martinez Pillet V; Velli M
    Sol Phys; 2022; 297(7):90. PubMed ID: 35855417
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Solar wind stream interaction regions throughout the heliosphere.
    Richardson IG
    Living Rev Sol Phys; 2018; 15(1):1. PubMed ID: 30872980
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Alfvénic velocity spikes and rotational flows in the near-Sun solar wind.
    Kasper JC; Bale SD; Belcher JW; Berthomier M; Case AW; Chandran BDG; Curtis DW; Gallagher D; Gary SP; Golub L; Halekas JS; Ho GC; Horbury TS; Hu Q; Huang J; Klein KG; Korreck KE; Larson DE; Livi R; Maruca B; Lavraud B; Louarn P; Maksimovic M; Martinovic M; McGinnis D; Pogorelov NV; Richardson JD; Skoug RM; Steinberg JT; Stevens ML; Szabo A; Velli M; Whittlesey PL; Wright KH; Zank GP; MacDowall RJ; McComas DJ; McNutt RL; Pulupa M; Raouafi NE; Schwadron NA
    Nature; 2019 Dec; 576(7786):228-231. PubMed ID: 31802006
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Probabilistic Solar Wind Forecasting Using Large Ensembles of Near-Sun Conditions With a Simple One-Dimensional "Upwind" Scheme.
    Owens MJ; Riley P
    Space Weather; 2017 Nov; 15(11):1461-1474. PubMed ID: 29398982
    [TBL] [Abstract][Full Text] [Related]  

  • 12. The Dependence of the Peak Velocity of High-Speed Solar Wind Streams as Measured in the Ecliptic by ACE and the STEREO satellites on the Area and Co-latitude of Their Solar Source Coronal Holes.
    Hofmeister SJ; Veronig A; Temmer M; Vennerstrom S; Heber B; Vršnak B
    J Geophys Res Space Phys; 2018 Mar; 123(3):1738-1753. PubMed ID: 29882534
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Helios Observations of Quasiperiodic Density Structures in the Slow Solar Wind at 0.3, 0.4, and 0.6 AU.
    Di Matteo S; Viall NM; Kepko L; Wallace S; Arge CN; MacNeice P
    J Geophys Res Space Phys; 2019 Feb; 124(2):837-860. PubMed ID: 32908809
    [TBL] [Abstract][Full Text] [Related]  

  • 14. The heliospheric magnetic field over the South polar region of the sun.
    Balogh A; Southwood DJ; Forsyth RJ; Horbury TS; Smith EJ; Tsurutani BT
    Science; 1995 May; 268(5213):1007-10. PubMed ID: 17774226
    [TBL] [Abstract][Full Text] [Related]  

  • 15. Picoflare jets power the solar wind emerging from a coronal hole on the Sun.
    Chitta LP; Zhukov AN; Berghmans D; Peter H; Parenti S; Mandal S; Aznar Cuadrado R; Schühle U; Teriaca L; Auchère F; Barczynski K; Buchlin É; Harra L; Kraaikamp E; Long DM; Rodriguez L; Schwanitz C; Smith PJ; Verbeeck C; Seaton DB
    Science; 2023 Aug; 381(6660):867-872. PubMed ID: 37616348
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Solar origins of solar wind properties during the cycle 23 solar minimum and rising phase of cycle 24.
    Luhmann JG; Petrie G; Riley P
    J Adv Res; 2013 May; 4(3):221-8. PubMed ID: 25685422
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Probing Upflowing Regions in the Quiet Sun and Coronal Holes.
    Schwanitz C; Harra L; Raouafi NE; Sterling AC; Moreno Vacas A; Del Toro Iniesta JC; Orozco Suárez D; Hara H
    Sol Phys; 2021; 296(12):175. PubMed ID: 34866662
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock.
    Richardson JD; Kasper JC; Wang C; Belcher JW; Lazarus AJ
    Nature; 2008 Jul; 454(7200):63-6. PubMed ID: 18596800
    [TBL] [Abstract][Full Text] [Related]  

  • 19. 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]  

  • 20. In Situ Observations of Interstellar Pickup Ions from 1 au to the Outer Heliosphere.
    Zirnstein EJ; Möbius E; Zhang M; Bower J; Elliott HA; McComas DJ; Pogorelov NV; Swaczyna P
    Space Sci Rev; 2022; 218(4):28. PubMed ID: 35574273
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 11.