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Detailed Reference Information
Acuna et al. 1980
Acuna, M.H., Ness, N.F. and Connerney, J.E.P. (1980). The Magnetic Field of Saturn: Further Studies of the Pioneer 11 Observations. Journal of Geophysical Research 85: doi: 10.1029/JA080i011p05675. issn: 0148-0227.

Analysis of magnetic field observations by the Goddard Space Flight Center high-field flux gate magnetometer on the Pioneer 11 spacecraft during Saturn encounter yields estimates of the planetary field. The field is mainly dipolar but rather than expected, with a moment equal to 0.20 G RS3 or 4.3¿1028 G cm3, opposite in polarity to earth's. Surprisingly, the field appears to be axially symmetric but with a small (0.04 RS) offset to the north so that N (S) polar field intensities are 0.6 (0.4) G, respectively. The deduced polar offset appears to be an artifact of the limited spatial extent of the observations or the presence of fields of external origin. The average stand-off distance of the magnetopause is expected to be 20 RS, i.e., at the orbit of Titan, so that this largest of solar system satellites is immersed not only in the Saturnian magnetophere but also at times in its magnetosheath and sometimes even in the interplanetary medium.

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Abstract

Journal
Journal of Geophysical Research
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American Geophysical Union
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