Plasma Observations Near Uranus: Initial Results from Voyager 2

@article{Bridge1986PlasmaON,
  title={Plasma Observations Near Uranus: Initial Results from Voyager 2},
  author={H. Bridge and J. Belcher and B. Coppi and A. Lazarus and R. McNutt and S. Olbert and J. Richardson and M. Sands and R. Selesnick and J. D. Sullivan and R. Hartle and K. Ogilvie and E. Sittler and F. Bagenal and R. S. Wolff and V. Vasyliūnas and G. Siscoe and C. Goertz and A. Eviatar},
  journal={Science},
  year={1986},
  volume={233},
  pages={89 - 93}
}
Extensive measurements of low-energy positive ions and electrons in the vicinity of Uranus have revealed a fully developed magnetosphere. The magnetospheric plasma has a warm component with a temperature of 4 to 50 electron volts and a peak density of roughly 2 protons per cubic centimeter, and a hot component, with a temperature of a few kiloelectron volts and a peak density of roughly 0.1 proton per cubic centimeter. The warm component is observed both inside and outside of L = 5, whereas the… Expand
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