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Space Science Reviews

, Volume 140, Issue 1–4, pp 261–313 | Cite as

The Solar Wind Around Pluto (SWAP) Instrument Aboard New Horizons

  • D. McComas
  • F. Allegrini
  • F. Bagenal
  • P. Casey
  • P. Delamere
  • D. Demkee
  • G. Dunn
  • H. Elliott
  • J. Hanley
  • K. Johnson
  • J. Langle
  • G. Miller
  • S. Pope
  • M. Reno
  • B. Rodriguez
  • N. Schwadron
  • P. Valek
  • S. Weidner
Article

Abstract

The Solar Wind Around Pluto (SWAP) instrument on New Horizons will measure the interaction between the solar wind and ions created by atmospheric loss from Pluto. These measurements provide a characterization of the total loss rate and allow us to examine the complex plasma interactions at Pluto for the first time. Constrained to fit within minimal resources, SWAP is optimized to make plasma-ion measurements at all rotation angles as the New Horizons spacecraft scans to image Pluto and Charon during the flyby. To meet these unique requirements, we combined a cylindrically symmetric retarding potential analyzer with small deflectors, a top-hat analyzer, and a redundant/coincidence detection scheme. This configuration allows for highly sensitive measurements and a controllable energy passband at all scan angles of the spacecraft.

Keywords

Solar wind Pluto plasma interaction Pickup ions 

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Copyright information

© Springer Science+Business Media B.V. 2007

Authors and Affiliations

  • D. McComas
    • 1
  • F. Allegrini
    • 1
  • F. Bagenal
    • 2
  • P. Casey
    • 1
  • P. Delamere
    • 2
  • D. Demkee
    • 1
  • G. Dunn
    • 1
  • H. Elliott
    • 1
  • J. Hanley
    • 1
  • K. Johnson
    • 1
  • J. Langle
    • 1
    • 3
  • G. Miller
    • 1
  • S. Pope
    • 1
  • M. Reno
    • 1
  • B. Rodriguez
    • 1
  • N. Schwadron
    • 1
    • 4
  • P. Valek
    • 1
  • S. Weidner
    • 1
  1. 1.Southwest Research InstituteSan AntonioUSA
  2. 2.University of ColoradoBoulderUSA
  3. 3.Midwest Research InstituteKansas CityUSA
  4. 4.Boston UniversityBostonUSA

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