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

Author:

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

Abstract

AbstractThe 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$^{\circ }\times 9.1^{\circ }$ × 9.1 field of view.

Funder

National Aeronautics and Space Administration

Publisher

Springer Science and Business Media LLC

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