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Surface Roughness of the Chang’E-5 and Chang’E-6 Lunar Samples: Implications for the Microscopic Processes Shaping the Lunar Surface

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

Jun Du et al 2026 The Planetary Science Journal 7 .

Provider: AAS Journals

Caption: Figure 5.

Power spectral densities (a)–(c) and Hurst exponents (d)–(f) of all the ROIs. In panels (a) and (d), the ROIs were classified based on their morphology. In panels (b) and (e), the ROIs were classified based on their compositions. In panels (c) and (f), the ROIs were classified based on their locations. In panels (a)–(c), the powers were selected at wavelengths of 1/100, 1/50, 1/20, 1/10, 1/5, 1/2, and 1 times the ROI length of 30 μm.

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