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GEOPHYSICAL RESEARCH LETTERS,
VOL. 24, NO. 17,
PAGES 2163–2166,
1997
Energetic Particle Signatures at Ganymede: Implications for Ganymede’s Magnetic Field
D. J. Williams
The Johns Hopkins University Applied Physics Laboratory, Laurel, MD
B. H. Mauk
The Johns Hopkins University Applied Physics Laboratory, Laurel, MD
R. W. McEntire
The Johns Hopkins University Applied Physics Laboratory, Laurel, MD
E. C. Roelof
The Johns Hopkins University Applied Physics Laboratory, Laurel, MD
T. P. Armstrong
University of Kansas, Lawrence, KS
B. Wilken
MPAe, Katlenburg-Lindau, Germany
J. G. Roederer
University of Alaska, Fairbanks, AK
S. M. Krimigis
The Johns Hopkins University Applied Physics Laboratory, Laurel, MD
T. A. Fritz
Boston University, Boston, MA
L. J. Lanzerotti
Lucent Technologies, Murray Hill, NJ
N. Murphy
Jet Propulsion Laboratory, Pasadena, CA
Abstract
The second encounter of the Galileo satellite with the Galilean moon Ganymede provided energetic particle measurements showing
effects due to the presence of that moon. Jovian corotation signatures, present on approach to and departure from the Ganymede
system, suddenly become much smaller when Galileo enters what has been termed Ganymede’s magnetosphere. The location of these
transitions agrees with magnetopause crossings identified by the magnetometer and plasma wave instruments. In Ganymede’s magnetosphere,
energetic ion and electron distributions display loss cone signatures whenever the Energetic Particles Detector (EPD) views
along the magnetic field line. The loss cone measurements are used to estimate Ganymede’s surface magnetic field along the
satellite track. The results agree with model projections to Ganymede’s polar cap and support the existence of a Ganymede-intrinsic
magnetic field. An evolution from single to double loss cone also occurs with increasing electron energy.
Received 14
March
1997;
accepted 27
June
1997.
Read Full Article Cited by
Citation: Williams, D. J., et al.
(1997),
Energetic Particle Signatures at Ganymede: Implications for Ganymede’s Magnetic Field,
Geophys. Res. Lett.,
24(17),
2163–2166.
Copyright 1997 by the American Geophysical Union.
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