Download 2005: Past Meets Present in Astronomy And Astrophysics: by Jose Afonso, Nuno Santos, Andre Moitinho, Rui Agostinho PDF

By Jose Afonso, Nuno Santos, Andre Moitinho, Rui Agostinho

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Not. R. Astron. Soc. 315, 479 (2000); M. A. de Avillez and D. Breitschwerdt, Astron. & Astrophys. 425, 899 (2004); 436, 585 (2005). 2. A. N. R. Acad. Sci. URSS 30, 301 (1941). 3. -S. She and E. Leveque, Phys. Rev. Lett. 72, 336 (1994). 4. S. Boldyrev, Astrophys. J. 569, 841 (2002). 5. H. Politano and A. Pouquet, Phys. Rev. E 52, 636 (1995). 6. M. A. de Avillez and D. Breitschwerdt, Phys. Rev. , submitted (2005). 7. R. Benzi, S. Ciliberto, R. Tripiccione, C. Baudet, F. Massaioli, and S. Succi, Phys.

F E R R E I R A j A. AIBEO*AND J. LIMA 5 Centro de Astrofisica da Universidade do Porto, R. das Estrelas, Portugal Porto, We examine the effect of the surface magnetic flux distribution on the coronal field topology. This preliminary study is motivated by the observational evidence for high magnetic flux concentration near the stellar poles of rapidly rotating young stars, and whether this has important consequences on the magnetic braking efficiency. We find that the coronal magnetic field rapidly expands to regions of low magnetic pressure creating a relatively smooth magnetic field with no memory of the surface radial field latitudinal distribution.

J. P. F. G. Monteiro, Seismology of the Solar Convection Zone, PhD Thesis, Queen Mary and Westfield College (1996) 5. M. J. P. F. G. Monteiro and J. Cristensen-Dalsgaard and M. J. Thompson, ESA SP-485: Stellar Structure and Habitable Planet Finding, 291 (2002) 6. F. J. G. Pinheiro and M. J. P. F. G. Monteiro and D. F. M. Folha, ESA SP-538: Second Eddington Workshop: Stellar structure and habitable planet finding, 385 (2004) 7. I. W. Roxburgh and S. V. Vorontsov, A&A, 411, 215 (2003) 8. M. Tassoul, ApJS 43, 469 (1980).

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