作者: R. E. Arvidson , E. A. Guinness , J. F. Bell , P. R. Christensen , M. K. Shepard
DOI:
关键词: Near infrared radiation 、 Geology 、 Remote sensing 、 Martian 、 Visible near infrared 、 Radiative transfer 、 Photometry (optics) 、 Spectral line 、 Radiative transfer modeling 、 Mars surface
摘要: We present a comprehensive visible/near-infrared two-layer radiative transfer modeling study using laboratory spectra of variable dust thicknesses deposited on substrates with known photometric parameters. The masking effects Martian airfall deposition rocks, soils, and lander/rover components provides the incentive to improve models [1-3]. It is believed that model presented will facilitate understanding spectral compositional properties both layer substrate material, allow for better compensation deposition.