Image Details
Caption: Figure A1.
All of the 11 soil targets observed by Chang’e-6 (CE-6) LMS in FBO hyperspectral mode, which collected a total of 16 spectra. The x-axis is the wavelength in nm, and the y-axis is the apparent reflectance RADF (I/F), which is contaminated with thermal emission of the high-temperature (∼350 K) lunar soil.
© 2026. The Author(s). Published by the American Astronomical Society.