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.
215 related articles for article (PubMed ID: 12040189)
1. Explaining the latitudinal distribution of sunspots with deep meridional flow. Nandy D; Choudhuri AR Science; 2002 May; 296(5573):1671-3. PubMed ID: 12040189 [TBL] [Abstract][Full Text] [Related]
2. Meridional flow in the Sun's convection zone is a single cell in each hemisphere. Gizon L; Cameron RH; Pourabdian M; Liang ZC; Fournier D; Birch AC; Hanson CS Science; 2020 Jun; 368(6498):1469-1472. PubMed ID: 32587017 [TBL] [Abstract][Full Text] [Related]
3. Variations in the Sun's meridional flow over a solar cycle. Hathaway DH; Rightmire L Science; 2010 Mar; 327(5971):1350-2. PubMed ID: 20223980 [TBL] [Abstract][Full Text] [Related]
4. The unusual minimum of sunspot cycle 23 caused by meridional plasma flow variations. Nandy D; Muñoz-Jaramillo A; Martens PC Nature; 2011 Mar; 471(7336):80-2. PubMed ID: 21368827 [TBL] [Abstract][Full Text] [Related]
5. Evolution of the Sun's large-scale magnetic field since the Maunder minimum. Solanki SK; Schüssler M; Fligge M Nature; 2000 Nov; 408(6811):445-7. PubMed ID: 11100720 [TBL] [Abstract][Full Text] [Related]
6. Observations of Time Variation in the Sun's Rotation. Woodard MF; Libbrecht KG Science; 1993 Jun; 260(5115):1778-81. PubMed ID: 17793654 [TBL] [Abstract][Full Text] [Related]
7. Solar physics. The crucial role of surface magnetic fields for the solar dynamo. Cameron R; Schüssler M Science; 2015 Mar; 347(6228):1333-5. PubMed ID: 25792324 [TBL] [Abstract][Full Text] [Related]
8. Influence of gravity waves on the internal rotation and Li abundance of solar-type stars. Charbonnel C; Talon S Science; 2005 Sep; 309(5744):2189-91. PubMed ID: 16195453 [TBL] [Abstract][Full Text] [Related]
9. The magnetic activity sunlike stars. Vaughan AH Science; 1984 Aug; 225(4664):793-800. PubMed ID: 17801135 [TBL] [Abstract][Full Text] [Related]
10. Reconciling solar and stellar magnetic cycles with nonlinear dynamo simulations. Strugarek A; Beaudoin P; Charbonneau P; Brun AS; do Nascimento JD Science; 2017 Jul; 357(6347):185-187. PubMed ID: 28706068 [TBL] [Abstract][Full Text] [Related]
11. Why does the sun's torsional oscillation begin before the sunspot cycle? Chakraborty S; Choudhuri AR; Chatterjee P Phys Rev Lett; 2009 Jan; 102(4):041102. PubMed ID: 19257410 [TBL] [Abstract][Full Text] [Related]
12. 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]
13. The solar dynamo. Miesch MS Philos Trans A Math Phys Eng Sci; 2012 Jul; 370(1970):3049-69. PubMed ID: 22665892 [TBL] [Abstract][Full Text] [Related]
14. Turbulent dynamics in the solar convection zone. Brummell N; Toomre J; Cattaneo F Science; 1995 Sep; 269(5229):1370-9. PubMed ID: 17731146 [TBL] [Abstract][Full Text] [Related]
15. Dynamic variations at the base of the solar convection zone. Howe R; Christensen-Dalsgaard J; Hill F; Komm RW; Larsen RM; Schou J; Thompson MJ; Toomre J Science; 2000 Mar; 287(5462):2456-60. PubMed ID: 10741959 [TBL] [Abstract][Full Text] [Related]
16. Solar-type dynamo behaviour in fully convective stars without a tachocline. Wright NJ; Drake JJ Nature; 2016 Jul; 535(7613):526-8. PubMed ID: 27466124 [TBL] [Abstract][Full Text] [Related]
17. 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]
18. A deep dynamo generating Mercury's magnetic field. Christensen UR Nature; 2006 Dec; 444(7122):1056-8. PubMed ID: 17183319 [TBL] [Abstract][Full Text] [Related]
19. No Sun-like dynamo on the active star ζ Andromedae from starspot asymmetry. Roettenbacher RM; Monnier JD; Korhonen H; Aarnio AN; Baron F; Che X; Harmon RO; Kővári Z; Kraus S; Schaefer GH; Torres G; Zhao M; ten Brummelaar TA; Sturmann J; Sturmann L Nature; 2016 May; 533(7602):217-20. PubMed ID: 27144357 [TBL] [Abstract][Full Text] [Related]
20. Magneto-convection. Stein RF Philos Trans A Math Phys Eng Sci; 2012 Jul; 370(1970):3070-87. PubMed ID: 22665893 [TBL] [Abstract][Full Text] [Related] [Next] [New Search]