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Reconciling solar and stellar magnetic cycles with nonlinear dynamo simulations

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Science  14 Jul 2017:
Vol. 357, Issue 6347, pp. 185-187
DOI: 10.1126/science.aal3999

Article Information

vol. 357 no. 6347 185-187

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History: 
  • Received for publication November 14, 2016
  • Accepted for publication June 5, 2017

Author Information

  1. A. Strugarek1,2,*,
  2. P. Beaudoin1,
  3. P. Charbonneau1,
  4. A. S. Brun2,
  5. J.-D. do Nascimento Jr.3,4
  1. 1Département de Physique, Université de Montréal, C.P. 6128 Succursale Centre-Ville, Montréal, Quebec H3C-3J7, Canada.
  2. 2Laboratoire Astrophysique, Instrumentation, Modélisation Paris-Saclay, Commissariat à l'Energie Atomique et aux Energies Alternatives/Irfu Université Paris-Diderot CNRS/Institut National des Sciences de l’Univers, F-91191 Gif-sur-Yvette, Paris, France.
  3. 3Departamento de Física Teórica e Experimental, Universidade Federal do Rio Grande do Norte, CP 1641, 59072-970 Natal, Rio Grande do Norte, Brazil.
  4. 4Harvard–Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA.
  1. *Corresponding author. Email: antoine.strugarek{at}cea.fr

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