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  Toroidal vs. poloidal magnetic fields in Sun-like stars: a rotation threshold

Petit, P., Dintrans, B., Donati, J.-F., Solanki, S. K., Aurière, M., Lignières, F., et al. (2008). Toroidal vs. poloidal magnetic fields in Sun-like stars: a rotation threshold. Mon. Not. Roy. Astron. Soc., 388, 80-88. doi:10.1111/j.1365-2966.2008.13411.x.

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 Creators:
Petit, P., Author
Dintrans, B., Author
Donati, J.-F., Author
Solanki, S. K.1, 2, Author           
Aurière, M., Author
Lignières, F., Author
Morin, J., Author
Paletou, F., Author
Ramirez, J., Author
Catala, C., Author
Fares, R., Author
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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 MPIS_GROUPS: Sun and Heliosphere
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 Dates: 2008
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1111/j.1365-2966.2008.13411.x
BibTex Citekey: Petit:2008-090
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Title: Mon. Not. Roy. Astron. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 388 Sequence Number: - Start / End Page: 80 - 88 Identifier: -