Europa's Magnetic Signature: Report from Galileo's Pass on 19 December 1996

Author:

Kivelson M. G.1234,Khurana K. K.1234,Joy S.1234,Russell C. T.1234,Southwood D. J.1234,Walker R. J.1234,Polanskey C.1234

Affiliation:

1. M. G. Kivelson and C. T. Russell, Institute of Geophysics and Planetary Physics and Department of Earth and Space Sciences, University of California, Los Angeles, Los Angeles, CA 90095–1567, USA.

2. K. K. Khurana, S. Joy, R. J. Walker, Institute of Geophysics and Planetary Physics, University of California, Los Angeles, Los Angeles, CA 90095–1567, USA.

3. D. J. Southwood, Department of Physics, Imperial College of Science, Technology, and Medicine, London SW7 2BZ, UK, and Institute of Geophysics and Planetary Physics, University of California, Los Angeles, Los Angeles, CA 90095–1567, USA.

4. C. Polanskey, Jet Propulsion Laboratory, 4800 Oak Grove Avenue, Pasadena, CA 91109, USA.

Abstract

On 19 December 1996 as Galileo passed close to Jupiter’s moon, Europa, the magnetometer measured substantial departures from the slowly varying background field of Jupiter’s magnetosphere. Currents coupling Europa to Jupiter’s magnetospheric plasma could produce perturbations of the observed size. However, the trend of the field perturbations is here modeled as the signature of a Europa-centered dipole moment whose maximum surface magnitude is ∼240 nanotesla, giving a rough upper limit to the internal field. The dipole orientation is oblique to Europa’s spin axis. This orientation may not be probable for a field generated by a core dynamo, but higher order multipoles may be important as they are at Uranus and Neptune. Although the data can be modeled as contributions of an internal field of Europa, they do not confirm its existence. The dipole orientation is also oblique to the imposed field of Jupiter and thus not directly produced as a response to that field. Close to Europa, plasma currents appear to produce perturbations with scale sizes that are small compared with a Europa radius.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference15 articles.

1. Kivelson M. G., Khurana K. K., Means J. D., Russell C. T., Snare R. C., Space Sci. Rev. 60, 357 (1992).

2. Kivelson M. G., et al., Nature 384, 537 (1996).

3. A Magnetic Signature at Io: Initial Report from the Galileo Magnetometer

4. . Note that the labels on the ordinates of figure 4 are incorrect. The correct ranges on the panels from bottom to top are −2100 to −1100 nT −500 to 500 nT and −500 to 500 nT;

5. Kivelson M. G., et al., ibid. 274, 396 (1996).

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