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  Intensification of a magnetic field in a stellar convection zone by conversion of potential energy

Rempel, M., & Schüssler, M. (2001). Intensification of a magnetic field in a stellar convection zone by conversion of potential energy. In G. Mathys, S. K. Solanki, & D. T. Wickramasinghe (Eds.), Magnetic Fields Across the Hertzsprung-Russell Diagram (pp. 165-168). San Francisco, USA: Astronomical Society of the Pacific.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-E7C3-E Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-E7C4-C
Genre: Conference Paper

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 Creators:
Rempel, Matthias1, 2, Author           
Schüssler, Manfred1, 2, 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: 2001
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: BibTex Citekey: Rempel:2001-087
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Title: Magnetic Fields Across the Hertzsprung-Russell Diagram
Source Genre: Proceedings
 Creator(s):
Mathys, G., Editor
Solanki, S. K.1, 2, Editor           
Wickramasinghe, D. T., Editor
Affiliations:
1 Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289            
2 MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291            
Publ. Info: San Francisco, USA : Astronomical Society of the Pacific
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 165 - 168 Identifier: -