Axial vs. equatorial dipolar dynamo models with implications for planetary 
magnetic fields

Aubert, Julien; Wicht, Johannes

doi:10.1016/S0012-821X(04)00102-5

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Axial vs. equatorial dipolar dynamo models with implications for planetary magnetic fields

Aubert, J., & Wicht, J. (2004). Axial vs. equatorial dipolar dynamo models with implications for planetary magnetic fields. Earth and Planetary Science Letters, 221, 409-419. doi:10.1016/S0012-821X(04)00102-5.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-F08F-E Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-F090-8

Genre: Journal Article

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Creators:
Aubert, Julien, Author
Wicht, Johannes¹, Author

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

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MPIS_GROUPS: Planets and Comets

MPIS_PROJECTS: Planetary Dynamics

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Dates: Date issued: 2004

Publication Status: Issued

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Rev. Type: Peer

Identifiers: DOI: 10.1016/S0012-821X(04)00102-5
BibTex Citekey: Aubert:2004-122

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Title: Earth and Planetary Science Letters

Source Genre: Journal

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Pages: - Volume / Issue: 221 Sequence Number: - Start / End Page: 409 - 419 Identifier: -