Enhancements of energetic particles near the heliospheric termination shock

@article{Mcdonald2003EnhancementsOE,
  title={Enhancements of energetic particles near the heliospheric termination shock},
  author={Frank B. Mcdonald and Edward C. Stone and Alan C. Cummings and Bryant C. Heikkila and N. K. Lal and W. R. Webber},
  journal={Nature},
  year={2003},
  volume={426},
  pages={48-51}
}
The spacecraft Voyager 1 is at a distance greater than 85 au from the Sun, in the vicinity of the termination shock that marks the abrupt slowing of the supersonic solar wind and the beginning of the extended and unexplored distant heliosphere. This shock is expected to accelerate ‘anomalous cosmic rays’, as well as to re-accelerate Galactic cosmic rays and low-energy particles from the inner Solar System. Here we report a significant increase in the numbers of energetic ions and electrons that… 

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Effects of the solar wind termination shock and heliosheath on theheliospheric modulation of galactic and anomalous Helium

Abstract. The interest in the role of the solar wind termination shock and heliosheath in cosmic ray modulation studies has increased significantly as the Voyager 1 and 2 spacecraft approach the
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