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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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 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: 2011
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 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: -