Articles | Volume 22, issue 5
https://doi.org/10.5194/angeo-22-1829-2004
© Author(s) 2004. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-22-1829-2004
© Author(s) 2004. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
08 Apr 2004
Surface conductivity of Mercury provides current closure and may affect magnetospheric symmetry
P. Janhunen
Finnish Meteorological Institute, Geophysical Research, Helsinki, Finland
E. Kallio
Finnish Meteorological Institute, Geophysical Research, Helsinki, Finland
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Cited
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- Ultra‐Low Frequency Waves in the Hermean Magnetosphere: On the Role of the Morphology of the Magnetic Field and the Foreshock E. Kallio et al. 10.1029/2022GL101850
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- MESSENGER Observations of Flow Braking and Flux Pileup of Dipolarizations in Mercury's Magnetotail: Evidence for Current Wedge Formation R. Dewey et al. 10.1029/2020JA028112
- A 3D hybrid simulation study of the electromagnetic field distributions in the lunar wake Y. Wang et al. 10.1016/j.icarus.2011.09.021
- Global Structure and Sodium Ion Dynamics in Mercury's Magnetosphere With the Offset Dipole M. Yagi et al. 10.1002/2017JA024082
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- Review of Mercury’s dynamic magnetosphere: Post-MESSENGER era and comparative magnetospheres W. Sun et al. 10.1007/s11430-021-9828-0
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- A time-averaged regional model of the Hermean magnetic field E. Thébault et al. 10.1016/j.pepi.2017.07.001
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