Hostname: page-component-78c5997874-fbnjt Total loading time: 0 Render date: 2024-11-18T15:14:41.497Z Has data issue: false hasContentIssue false
  • English
  • Français

Medicean Moons Sailing Through Plasma Seas: Challenges in Establishing Magnetic Properties

Published online by Cambridge University Press:  03 November 2010

Margaret G. Kivelson ,
Xianzhe Jia  and
Krishan K. Khurana
Margaret G. Kivelson
Affiliation:
Department of Earth and Space Sciences, University of California, Los Angeles, CA 90095-1567, USA email: mkivelson@igpp.ucla.edu Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109-2143
Xianzhe Jia
Affiliation:
Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109-2143
Krishan K. Khurana
Affiliation:
Department of Earth and Space Sciences, University of California, Los Angeles, CA 90095-1567, USA email: mkivelson@igpp.ucla.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Jupiter's moons, embedded in the magnetized, flowing plasma of Jupiter's magnetosphere, the plasma seas of the title, are fluids whose highly non-linear interactions imply complex behavior. In a plasma, magnetic fields couple widely separated regions; consequently plasma interactions are exceptionally sensitive to boundary conditions (often ill-specified). Perturbation fields arising from plasma currents greatly limit our ability to establish more than the dominant internal magnetic field of a moon. With a focus on Ganymede and a nod to Io, this paper discusses the complexity of plasma-moon interactions, explains how computer simulations have helped characterize the system and presents improved fits to Ganymede's internal field.

Keywords

Galilean moonsmagnetic fieldmagnetosphere
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S269: Galileo's Medicean Moons: their impact on 400 years of discovery , January 2010 , pp. 58 - 70
Copyright
Copyright © International Astronomical Union 2010

References

Anderson, J. D., Lau, E. L., Shogren, W. L., Schubert, G., & Moore, W. B. 1996, Nature, 384CrossRefGoogle Scholar
Busse, F. H. 1976, Phys. of the Earth and Plan. Int., 12, 350CrossRefGoogle Scholar
Eviatar, A., Vasyliunas, V. M., & Gurnett, D. A. 2001, Planet. Space Sci., 49, 327CrossRefGoogle Scholar
Frank, L. A., Paterson, W. R., Ackerson, K. L., & Bolton, S. J. 1997, Geophys. Res. Lett., 24, 2, 151Google Scholar
Jia, X., Walker, R. J., et al. 2008, J. Geophys. Res., 113, A06212, doi:10.1029/2007JA012748Google Scholar
Jia, X. 2009, Ph.D. Dissertation, Dept. of Earth and Space Sciences, UCLAGoogle Scholar
Jia, X., Walker, R. J., Kivelson, M. G., Khurana, K. K., & Linker, J. A. 2009a, J. Geophys. Res., 114, doi:10.1029/2009JA014375Google Scholar
Jia, X., Kivelson, M. G., Khurana, K. K., & Walker, R. J. 2009b, Space Sci Rev, doi:10.10.1007/s11214-009-9507-8Google Scholar
Jia, X., Walker, R. J., Kivelson, M. G., Khurana, K. K., & Linker, J. A. 2010, J. Geophys. Res., doi:10.1029/2010JA015771Google Scholar
Khurana, K. K., Kivelson, M. G., et al. 1998, Nature, 395, 777CrossRefGoogle Scholar
Khurana, K. K., Jia, X., & Kivelson, M. G. 2010, A magma ocean at Io?, in preparationGoogle Scholar
Kivelson, M. G. 2004, Adv. Space Res., 33, 2061CrossRefGoogle Scholar
Kivelson, M. G., Khurana, K. K., et al. 1996, Nature, 384, 537CrossRefGoogle Scholar
Kivelson, M. G., Khurana, K. K., Russell, C. T., & Walker, R. J. 1997, Geophys. Res. Lett., 24, 2127CrossRefGoogle Scholar
Kivelson, M. G., Khurana, K. K., et al. 1997, Geophys. Res. Lett., 24, 2155CrossRefGoogle Scholar
Kivelson, M. G. et al. 1998, J. Geophys. Res., 103, 19963CrossRefGoogle Scholar
Kivelson, M. G., Khurana, K. K., et al. 2001, J. Geophys. Res., 106, 26, 121Google Scholar
Kivelson, M. G., Khurana, K. K., & Volwerk, M. 2002, Icarus, 157, 507CrossRefGoogle Scholar
Kivelson, M. G., Bagenal, F., et al. 2004, Chapter 21 in Jupiter: The Planet, Satellites and Magnetosphere edited by Bagenal, F., Dowling, T. and McKinnon, W., Cambridge University PressGoogle Scholar
Neubauer, F. M. 1978, Geophys. Res. Lett., 5, 905CrossRefGoogle Scholar
Paty, C. & Winglee, R. 2006, Geophys. Res. Lett., 33, L10106, doi:10.1029/2005GL025273CrossRefGoogle Scholar
Saur, J., Strobel, D. F., & Neubauer, F. M. 1998, J. Geophys. Res., 103, 19, 947Google Scholar
Schilling, N., Neubauer, F. M., & Saur, J. 2007, Icarus, 192, 41CrossRefGoogle Scholar
Schilling, N., Neubauer, F. M., & Saur, J. 2008, J. Geophys. Res., 113, A03203. doi:10.1029/2007JA012842Google Scholar
Schubert, G., Stevenson, D. J., & Ellsworth, K. 1981, Icarus, 47, 46CrossRefGoogle Scholar
Showmann, A. P. & Malhotra, R. 1997, Icarus, 127, 93CrossRefGoogle Scholar
Walker, R. J. & Russell, C. T. 1995, in Introduction to Space Physics edited by Kivelson, M. G., & Russell, C. T., New York, Cambridge U. PressGoogle Scholar
Zimmer, C., Khurana, K. K., & Kivelson, M. G. 2000, Icarus, 147, 329CrossRefGoogle Scholar