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Surface Roughness of the Chang’E-6 Lunar Samples and Landing Site from Submicrometer to Kilometer Scales: Implications for Lunar Surface Processes and Remote Sensing Data Modeling

  • Authors: Jun Du, Jianxin Tian, Yang Liu, Chenxiang Li, Yazhou Yang, Minge Liu, Huimin Shao, Mengyuan Zhang, Ding Nan, Dijun Guo, Yuchen Xu, Feng Zhang, Kaichang Di, Rui Wen, Shifeng Dai, Yongliao Zou

Jun Du et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 6.

Normalized frequency distributions of bidirectional slopes (light green) of the AFM (panel (a)), ALSCC (panel (b)), PCAM (panel (c)), LCAM (panel (d)), NAC (panel (e)), and SLDEM (panel (f)) ROIs. Hapke’s mean slope and its uncertainty are denoted by the red solid and dashed lines. In panels (a)–(d), the effective slope (22.9°–25.5°) inverted by the LROC/WAC images in the visible bands is indicated by the vertical gray shaded area.

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