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The Lunar Environment Heliophysics X-ray Imager (LEXI) Mission

  • B. M. Walsh,
  • K. D. Kuntz,
  • S. Busk,
  • T. Cameron,
  • D. Chornay,
  • A. Chuchra,
  • M. R. Collier,
  • C. Connor,
  • H. K. Connor,
  • T. E. Cravens,
  • N. Dobson,
  • M. Galeazzi,
  • H. Kim,
  • J. Kujawski,
  • C. K. Paw U,
  • F. S. Porter,
  • V. Naldoza,
  • R. Nutter,
  • R. Qudsi,
  • D. G. Sibeck,
  • S. Sembay,
  • M. Shoemaker,
  • K. Simms,
  • N. E. Thomas,
  • E. Atz,
  • G. Winkert

摘要

The Lunar Environment heliospheric X-ray Imager (LEXI) is a wide field-of-view soft X-ray telescope developed to study solar wind-magnetosphere coupling. LEXI is part of the Blue Ghost 1 mission comprised of 10 payloads to be deployed on the lunar surface. LEXI monitors the dayside magnetopause position and shape as a function of time by observing soft X-rays (0.1–2 keV) emitted from solar wind charge-exchange between exospheric neutrals and high charge-state solar wind plasma in the dayside magnetosheath. Measurements of the shape and position of the magnetopause are used to test temporal models of meso- and macro-scale magnetic reconnection. To image the boundary, LEXI employs lobster-eye optics to focus X-rays to a microchannel plate detector with a 9.1 × 9.1 $^{\circ }\times 9.1^{\circ }$ field of view.