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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 8.

Representative 1D profiles of rms slopes of the AFM (panel (a)), ALSCC (panel (b)), PCAM (panel (c)), LCAM (panel (d)), NAC (panel (e)), and SLDEM (panel (f)) ROIs with azimuth angles of 0° (green), 45° (yellow), 90° (blue), and 135° (red). In panel (b), the effective slope (20°–35°) inverted by the Diviner TIR data is indicated by the horizontal gray shaded area, and the spatial scales that satisfy the TIR-sensitive slope are denoted by the vertical solid lines.

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