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<p>NASA’s Interstellar Mapping and Acceleration Probe (IMAP) mission simultaneously investigates the acceleration of particles expelled from the Sun, and how the interaction of these particles with the local interstellar medium shapes our heliospheric boundary. The IMAP observatory makes critical measurements that facilitate this ground breaking science by incorporating a spin stabilized spacecraft orbiting around the first Sun-Earth Lagrange point, L1, with a payload comprised of ten unique instruments, making comprehensive and synergistic observations of solar wind, suprathermal, energetic particles and magnetic field, energetic neutral atoms mapping the boundary of our heliosphere, as well as interstellar neutral atoms and dust. This paper provides details on the design, integration, and testing of the IMAP observatory.</p>

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The IMAP Observatory Overview

  • 期刊论文

  • 出版模式：

    开放获取

  • 发表日期：

    2026年1月29日

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  • K. P. Hegarty,
  • S. Kubota,
  • M. Cully,
  • D. J. McComas,
  • E. R. Christian,
  • N. A. Schwadron,
  • M. Gkioulidou,
  • S. Bushman,
  • C. Collura,
  • M. Dauberman,
  • C. Drabenstadt,
  • A. Driesman,
  • A. Dubill,
  • B. Duffy,
  • E. Coleman,
  • D. Eng,
  • C. J. Ercol,
  • A. Gerger,
  • R. Hall,
  • J. Hahn,
  • M. Haque,
  • S. Hefter,
  • D. Jeong,
  • D. Jones,
  • J. Kelman,
  • C. Krupiarz,
  • F. Kujawa,
  • C. Lippe,
  • D. Matlin,
  • C. Monaco,
  • D. Myers,
  • E. Rivera Sepulveda,
  • D. Rodriguez,
  • L. Roufberg,
  • J. Scherrer,
  • M. Schwinger,
  • A. Shin,
  • F. Siddique,
  • E. Smith,
  • R. Smith,
  • M. Tapley,
  • S. Vernon,
  • C. Vigil,
  • S. Weidner

摘要

NASA’s Interstellar Mapping and Acceleration Probe (IMAP) mission simultaneously investigates the acceleration of particles expelled from the Sun, and how the interaction of these particles with the local interstellar medium shapes our heliospheric boundary. The IMAP observatory makes critical measurements that facilitate this ground breaking science by incorporating a spin stabilized spacecraft orbiting around the first Sun-Earth Lagrange point, L1, with a payload comprised of ten unique instruments, making comprehensive and synergistic observations of solar wind, suprathermal, energetic particles and magnetic field, energetic neutral atoms mapping the boundary of our heliosphere, as well as interstellar neutral atoms and dust. This paper provides details on the design, integration, and testing of the IMAP observatory.