Data produced as part of the study entitled "Thermal infrared spectral characteristics of Martian dust deposits and evidence for atmosphere-regolith interactions"

These files were produced as part of the study entitled “Thermal infrared spectral characteristics of Martian dust deposits and evidence for atmosphere-regolith interactions”, published in Icarus. If you use the data, please kindly cite our paper: Rogers, A. D., S. W. Ruff, and M. D. Smith (2023), Thermal infrared spectral characteristics of Martian dust deposits and evidence for atmosphere-regolith interactions, Icarus, doi: https://doi.org/10.1016/j.icarus.2023.115687 Files contained in this archive: MAPS -- all are 4 pixels per degree, centered at 0 deg longitude and latitude (-180 to 180 E, -90 to 90N) surface_spectral_emissivity.tif -- the global surface emissivity data set (GeoTIFF), 106 bands surface_spectral_emissivity_noiserem.tif -- the global surface emissivity data set, 106 bands, noise removed (GeoTIFF) DCI.tif -- DCI map (GeoTIFF) surf_emiss_9um.tif -- the 9 micron emissivity map (GeoTIFF) surf_emiss_32um.tif -- the 32 micron emissivity map (GeoTIFF) SAM_maskedDCI96.tif -- the 1-SAM map (GeoTIFF) tes1630map.tif -- the 1630cm-1 map (GeoTIFF) tesCFmap.tif -- the CF map (GeoTIFF) tesCFmapchi.tif -- the chi-squared error map to the parabolic fit for CF (GeoTIFF) broadband_emissivity_150K.tif -- broadband emissivity at 150K broadband_emissivity_220K.tif -- broadband emissivity at 220K broadband_emissivity_300K.tif -- broadband emissivity at 300K mask_DCI_96.tif -- all pixels with DCI