The Lunar Lander Neutron and Dosimetry (LND) Experiment on Chang’E 4. (arXiv:2001.11028v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Wimmer_Schweingruber_R/0/1/0/all/0/1">Robert F. Wimmer-Schweingruber</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yu_J/0/1/0/all/0/1">Jia Yu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bottcher_S/0/1/0/all/0/1">Stephan I. B&#xf6;ttcher</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_S/0/1/0/all/0/1">Shenyi Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Burmeister_S/0/1/0/all/0/1">S&#xf6;nke Burmeister</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lohf_H/0/1/0/all/0/1">Henning Lohf</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Guo_J/0/1/0/all/0/1">Jingnan Guo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Xu_Z/0/1/0/all/0/1">Zigong Xu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Schuster_B/0/1/0/all/0/1">Bj&#xf6;rn Schuster</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Seimetz_L/0/1/0/all/0/1">Lars Seimetz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Forstner_J/0/1/0/all/0/1">Johan L. Freiherr von Forstner</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ravanbakhsh_A/0/1/0/all/0/1">Ali Ravanbakhsh</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Knierim_V/0/1/0/all/0/1">Violetta Knierim</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kolbe_S/0/1/0/all/0/1">Stefan Kolbe</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Woyciechowsky_H/0/1/0/all/0/1">Hauke Woyciechowsky</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kulkarni_S/0/1/0/all/0/1">Shrinivasrao R. Kulkarni</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yuan_B/0/1/0/all/0/1">Bin Yuan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Shen_G/0/1/0/all/0/1">Guohong Shen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_C/0/1/0/all/0/1">Chunqing Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chang_Z/0/1/0/all/0/1">Zheng Chang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Berger_T/0/1/0/all/0/1">Thomas Berger</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hellweg_C/0/1/0/all/0/1">Christine E. Hellweg</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Matthia_D/0/1/0/all/0/1">Daniel Matthi&#xe4;</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hou_D/0/1/0/all/0/1">Donghui Hou</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Knappmann_A/0/1/0/all/0/1">Alke Knappmann</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Buschel_C/0/1/0/all/0/1">Charlotte B&#xfc;schel</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hou_X/0/1/0/all/0/1">Xufeng Hou</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ren_B/0/1/0/all/0/1">Baoguo Ren</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fu_Q/0/1/0/all/0/1">Qiang Fu</a>

Chang’E 4 is the first mission to the far side of the Moon and consists of a
lander, a rover, and a relay spacecraft. Lander and rover were launched at
18:23 UTC on December 7, 2018 and landed in the von K’arm’an crater at 02:26
UTC on January 3, 2019. Here we describe the Lunar Lander Neutron & Dosimetry
experiment (LND) which is part of the Chang’E 4 Lander scientific payload. Its
chief scientific goal is to obtain first active dosimetric measurements on the
surface of the Moon. LND also provides observations of fast neutrons which are
a result of the interaction of high-energy particle radiation with the lunar
regolith and of their thermalized counterpart, thermal neutrons, which are a
sensitive indicator of subsurface water content.

Chang’E 4 is the first mission to the far side of the Moon and consists of a
lander, a rover, and a relay spacecraft. Lander and rover were launched at
18:23 UTC on December 7, 2018 and landed in the von K’arm’an crater at 02:26
UTC on January 3, 2019. Here we describe the Lunar Lander Neutron & Dosimetry
experiment (LND) which is part of the Chang’E 4 Lander scientific payload. Its
chief scientific goal is to obtain first active dosimetric measurements on the
surface of the Moon. LND also provides observations of fast neutrons which are
a result of the interaction of high-energy particle radiation with the lunar
regolith and of their thermalized counterpart, thermal neutrons, which are a
sensitive indicator of subsurface water content.

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