Magnetic Fields at Neptune

@article{Ness1989MagneticFA,
  title={Magnetic Fields at Neptune},
  author={Norman F. Ness and Mario H. Acu�a and L. F. Burlaga and John E. P. Connerney and Ronald P. Lepping and Fritz M. Neubauer},
  journal={Science},
  year={1989},
  volume={246},
  pages={1473 - 1478}
}
The National Aeronautics and Space Administration Goddard Space Flight Center-University of Delaware Bartol Research Institute magnetic field experiment on the Voyager 2 spacecraft discovered a strong and complex intrinsic magnetic field of Neptune and an associated magnetosphere and magnetic tail. The detached bow shock wave in the supersonic solar wind flow was detected upstream at 34.9 Neptune radii (RN), and the magnetopause boundary was tentatively identified at 26.5 RN near the planet-sun… 
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Field-independent source localization of Neptune's radio bursts
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The Encounter of Voyager 2 with Neptune’s Magnetosphere
The particles and fields complement of instruments on the Voyager 2 spacecraft performed a comprehensive set of measurements during the encounter with the Neptune system on August 24 through 28,
Magnetic fields of the outer planets
It is difficult to imagine a group of planetary dynamos more diverse than those visited by the Pioneer and Voyager spacecraft. The magnetic field of Jupiter is large in magnitude and has a dipole
First Plasma Wave Observations at Neptune
The Voyager 2 plasma wave instrument detected many familiar plasma waves during the encounter with Neptune, including electron plasma oscillations in the solar wind upstream of the bow shock,
Evidence for a diurnally rocking plasma mantle at Neptune
Voyager's post-encounter trajectory at Neptune allows the directions of the magnetic field in the magnetosheath produced by the draping of the typical interplanetary field and by alignment with the
ULF turbulence in the Neptunian polar cusp
One of the most fortuitous events occurring during the Voyager 2 Neptune encounter was the passage of the spacecraft through the southern magnetic cusp region prior to entry into the magnetosphere.
Tether capture of spacecraft at Neptune
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The magnetic field experiment on the Voyager 2 spacecraft revealed a strong planetary magnetic field of Uranus and an associated magnetosphere and fully developed bipolar masnetic tail. The detached
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TLDR
Results and the magnetic field geometry confirm the earlier conclusion from Voyager I studies that Jupiter has an enormous magnetic tail, approximately 300 to 400 RJ in diameter, trailing behind the planet with respect to the supersonic flow of the solar wind.
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TLDR
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The Voyager 1 spacecraft had a close encounter (miss distance = 6970 km) with Titan (diameter = 5140 km) on November 12, 1980, while this large satellite was located within the Saturnian
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If Neptune has a large magnetic moment, a weak supply of plasma for its magnetosphere, and a magnetic moment that is in near alignment with the planetary spin axis, we argue that, except for a region
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The enigmatic control of the occurrence frequency of Jupiter's decametric emissions by the satellite Io has been explained theoretically on the basis of its strong electrodynamic interaction with the
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TLDR
The plasma science experiment on Voyager 2 made observations of the plasma environment in Neptune's magnetosphere and in the surrounding solar wind, finding the maximum plasma density observed in the magnetosphere is inferred to be 1.4 per cubic centimeter, the smallest observed by Voyager in any magnetosphere.
The magnetosphere of Uranus - Plasma sources, convection, and field configuration
At the time of the Voyager 2 flyby of Uranus, the planetary rotational axis will be roughly antiparallel to the solar wind flow. If Uranus has a magnetic dipole moment that is approximately aligned
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We compare Voyager 2 magnetic field and plasma data with theoretical model calculations for the magnetosphere of Uranus in order to derive a global picture from the quite limited set of measurements.
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