Models of magnetic field generation in partly stable planetary cores: 
Applications to Mercury and Saturn

Christensen, U. R.; Wicht, J.

doi:10.1016/j.icarus.2008.02.013

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Models of magnetic field generation in partly stable planetary cores: Applications to Mercury and Saturn

Christensen, U. R., & Wicht, J. (2008). Models of magnetic field generation in partly stable planetary cores: Applications to Mercury and Saturn. Icarus, 196, 16-34. doi:10.1016/j.icarus.2008.02.013.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-FF26-D Version Permalink: https://hdl.handle.net/21.11116/0000-0007-2357-0

Genre: Journal Article

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Creators:
Christensen, U. R.^{1, 2}, Author
Wicht, J.¹, Author

Affiliations:
1Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291

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MPIS_GROUPS: Planets and Comets

MPIS_PROJECTS: Planetary Dynamics

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Dates: Date issued: 2008

Publication Status: Issued

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Rev. Type: Peer

Identifiers: DOI: 10.1016/j.icarus.2008.02.013
BibTex Citekey: Christensen:2008-075

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Title: Icarus

Source Genre: Journal

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Pages: - Volume / Issue: 196 Sequence Number: - Start / End Page: 16 - 34 Identifier: -