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Experimental Astronomy

, Volume 33, Issue 2–3, pp 365–401 | Cite as

IMPALAS: Investigation of MagnetoPause Activity using Longitudinally-Aligned Satellites—a mission concept proposed for the ESA M3 2020/2022 launch

  • Christopher J. OwenEmail author
  • Olaf Amm
  • Roberto Bruno
  • Johan De Keyser
  • Malcolm W. Dunlop
  • Jonathan P. Eastwood
  • Andrew N. Fazakerley
  • Dominique Fontaine
  • Colin Forsyth
  • Hiroshi Hasegawa
  • Petr Hellinger
  • David Hercik
  • Christian Jacquey
  • Steven Milan
  • Joachim Raeder
  • David G. Sibeck
  • Stepan Stverak
  • Pavel Travnicek
  • Andrew P. Walsh
  • James A. Wild
Original Article
  • 131 Downloads

Abstract

The dayside magnetopause is the primary site of energy transfer from the solar wind into the magnetosphere, and modulates the activity observed within the magnetosphere itself. Specific plasma processes operating on the magnetopause include magnetic reconnection, generation of boundary waves, propagation of pressure-pulse induced deformations of the boundary, formation of boundary layers and generation of Alfvén waves and field-aligned current systems connecting the boundary to the inner magnetosphere and ionosphere. However, many of the details of these processes are not fully understood. For example, magnetic reconnection occurs sporadically, producing flux transfer events, but how and where these arise, and their importance to the global dynamics of the magnetospheric system remain unresolved. Many of these phenomena involve propagation across the magnetopause surface. Measurements at widely-spaced (Δ ∼ 5 RE) intervals along the direction of dayside terrestrial field lines at the magnetopause would be decisive in resolving these issues. We describe a mission carrying a fields and plasmas payload (including magnetometer, ion and electron spectrometer and energetic particle telescopes) on three identical spacecraft in synchronized orbits. These provide the needed separations, with each spacecraft skimming the dayside magnetopause and continuously sampling this boundary for many hours. The orbits are phased such that (i) all three spacecraft maintain common longitude and thus sample along the same magnetopause field line; (ii) the three spacecraft reach local midday when northern European ground-based facilities also lie near local midday, enabling simultaneous sampling of magnetopause field lines and their footprints.

Keywords

Magnetopause Magnetic reconnection Solar wind–magnetosphere coupling Cosmic vision 

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Copyright information

© Springer Science+Business Media B.V. 2011

Authors and Affiliations

  • Christopher J. Owen
    • 1
    Email author
  • Olaf Amm
    • 2
  • Roberto Bruno
    • 3
  • Johan De Keyser
    • 4
  • Malcolm W. Dunlop
    • 5
  • Jonathan P. Eastwood
    • 6
  • Andrew N. Fazakerley
    • 1
  • Dominique Fontaine
    • 7
  • Colin Forsyth
    • 1
  • Hiroshi Hasegawa
    • 8
  • Petr Hellinger
    • 9
  • David Hercik
    • 9
  • Christian Jacquey
    • 10
  • Steven Milan
    • 11
  • Joachim Raeder
    • 12
  • David G. Sibeck
    • 13
  • Stepan Stverak
    • 9
  • Pavel Travnicek
    • 9
    • 14
  • Andrew P. Walsh
    • 1
  • James A. Wild
    • 15
  1. 1.Mullard Space Science LaboratoryUniversity College LondonSurreyUK
  2. 2.Arctic Research UnitFinnish Meteorological InstituteHelsinkiFinland
  3. 3.INAF-IFSIRomeItaly
  4. 4.Institute for Space AeronomyBrusselsBelgium
  5. 5.Space Sciences DivisionRutherford Appleton LaboratoryOxfordshireUK
  6. 6.The Blackett LaboratoryImperial CollegeLondonUK
  7. 7.Laboratoire de Physique des PlasmasEcole PolytechniqueVélizyFrance
  8. 8.Institute of Space and Astronautical Science (ISAS)KanagawaJapan
  9. 9.Academy of Sciences of the Czech RepublicPragueCzech Republic
  10. 10.Institut de Recherche en Astrophysique et Planetologie (IRAP)ToulouseFrance
  11. 11.Radio and Space Plasmas GroupUniversity of LeicesterLeicesterUK
  12. 12.Space Science CenterUniversity of New HampshireDurhamUSA
  13. 13.NASA/Goddard Space Flight CenterGreenbeltUSA
  14. 14.University of California at BerkeleyBerkeleyUSA
  15. 15.University of LancasterLancasterUK

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