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

Rempel, Matthias; Schüssler, Manfred

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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, Matthias^{1, 2}, Author
Schüssler, Manfred^{1, 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: Date issued: 2001

Publication Status: Issued

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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: -