The negative ions at the lunar surface (NILS) instrument on the Chang’E-6 missionSwedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
Swedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
National Space Science Center (NSSC), Chinese Academy of Sciences (CAS), No. 1 Nanertiao, Zhongguancun, Haidian district, Beijing, China; University of Chinese Academy of Sciences, No.19(A) Yuquan Road, Shijingshan district, Beijing, China.
National Space Science Center (NSSC), Chinese Academy of Sciences (CAS), No. 1 Nanertiao, Zhongguancun, Haidian district, Beijing, China.
European Space Agency/European Space Research and Technology Centre, Keplerlaan 1, Noordwijk, Netherlands.
Lunar Exploration and Space Engineering Center (LESEC), Beijing, China.
National Space Science Center (NSSC), Chinese Academy of Sciences (CAS), No. 1 Nanertiao, Zhongguancun, Haidian district, Beijing, China.
Lunar Exploration and Space Engineering Center (LESEC), Beijing, China.
Lunar Exploration and Space Engineering Center (LESEC), Beijing, China.
Swedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
Swedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
Swedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
Swedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
Swedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
Swedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
Swedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
Swedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
Swedish Institute of Space Physics, Bengt Hultqvists väg 1, Kiruna, Sweden.
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2025 (English)In: Space Science Reviews, ISSN 0038-6308, E-ISSN 1572-9672, Vol. 221, no 3, article id 38Article in journal (Refereed) Published
Abstract [en]
The Negative Ions at the Lunar Surface (NILS) instrument is a compact mass resolving negative ion and electron analyser flown on the Chinese Chang’E-6 mission to the Moon. NILS measures negative ions and electrons in the energy range of 3 eV/q to 3 keV/q with a mass resolution m/Δm of about 2. The mass resolution is sufficient to separate charge-converted solar wind protons and sputtered negatively charged atoms form the surface. An electro-magnetic electron suppression system allows to switch between electron and ion measurements. The fan-shaped field of view is divided into 16 discrete angular pixels that are scanned sequentially. For each viewing direction, an electron and an ion energy spectrum is acquired in 4.06 s. NILS has a mass of 919 g, excluding cables and multi-layer insulation. Power consumption is on average 2.7 W during nominal operations.
Place, publisher, year, edition, pages
2025. Vol. 221, no 3, article id 38
Keywords [en]
Chang’E-6, Geometric factor determination, Lunar surface, Mass resolving negative ion analyzer, Solar wind - regolith interaction
National Category
Fusion, Plasma and Space Physics Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:umu:diva-238375DOI: 10.1007/s11214-025-01162-wISI: 001466462400001Scopus ID: 2-s2.0-105003321091OAI: oai:DiVA.org:umu-238375DiVA, id: diva2:1957228
2025-05-082025-05-082025-05-08Bibliographically approved