Terrestrial analogues for lunar impact melt flows
Lunar impact melt deposits have unique physical properties. They have among the highest observed radar returns at S-Band (12.6 cm wavelength), implying that they are rough at the decimeter scale. However, they are also observed in high-resolution optical imagery to be quite smooth at the meter scale...
Published in: | Icarus |
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Main Authors: | , , , , , , , , , , , , |
Format: | Text |
Language: | unknown |
Published: |
LSU Scholarly Repository
2017
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Subjects: | |
Online Access: | https://repository.lsu.edu/geo_pubs/1853 https://doi.org/10.1016/j.icarus.2016.08.008 |