Saturn's very axisymmetric magnetic field: No detectable secular variation or 
tilt

Cao, Hao; Russell, Christopher T.; Christensen, Ulrich R.; Dougherty, Michele K.; Burton, Marcia E.

doi:10.1016/j.epsl.2011.02.035

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Saturn's very axisymmetric magnetic field: No detectable secular variation or tilt

Cao, H., Russell, C. T., Christensen, U. R., Dougherty, M. K., & Burton, M. E. (2011). Saturn's very axisymmetric magnetic field: No detectable secular variation or tilt. Earth and Planetary Science Letters, 304(1-2), 22-28. doi:10.1016/j.epsl.2011.02.035.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0015-078B-0 Version Permalink: https://hdl.handle.net/21.11116/0000-0007-2367-E

Genre: Journal Article

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Creators:
Cao, Hao, Author
Russell, Christopher T., Author
Christensen, Ulrich R.^{1, 2}, Author
Dougherty, Michele K., Author
Burton, Marcia E., 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: 2011

Publication Status: Issued

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Rev. Type: Peer

Identifiers: DOI: 10.1016/j.epsl.2011.02.035
BibTex Citekey: Cao:2011-200

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Title: Earth and Planetary Science Letters

Source Genre: Journal

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Pages: - Volume / Issue: 304 (1-2) Sequence Number: - Start / End Page: 22 - 28 Identifier: -