urn:nasa:pds:ruff_pdart14_mtes:data_mtes_edc:2t189235290edcal00p3680n0a1 1.0 1.8.0.0 Product_Observational 2005-12-30T17:17:59.381Z 2005-12-30T18:01:43.387Z Mars Exploration Rover Mission urn:nasa:pds:context:investigation:mission.mars_exploration_rover data_to_investigation MER 2 Mini-TES MER2 Spacecraft urn:nasa:pds:context:instrument_host:spacecraft.mer2 is_instrument_host Mini-TES Instrument urn:nasa:pds:context:instrument:mini-tes.mer2 is_instrument Mars Planet urn:nasa:pds:context:target:planet.mars data_to_target Averaged Mirror-Dust-Corrected Emissivity Image Cube display_settings_to_array Sample Left to Right Line Top to Bottom The spectral samples are uniformly distributed in wavenumber and the full-width, half-maximum (FWHM) of each sample is determined by the optical displacement of the Michelson mirror. Averaged Mirror-Dust-Corrected Emissivity Image Cube spectral_characteristics_to_array_object urn:nasa:pds:ruff_pdart14_mtes:data_ancillary:mtes_wavenumbers data_to_ancillary_data urn:nasa:pds:ruff_pdart14_mtes:data_ancillary:mtes_wavenumbers data_to_ancillary_data urn:nasa:pds:ruff_pdart14_mtes:data_ancillary:mtes_targets data_to_ancillary_data Targets of observation in this image may be listed in the referenced document. 2T189235290EDCAL00P3680N0A1.IMG 2017-08-23T00:33:49.92Z 14028 This image cube has 167 spectral bands representing averaged and mirror-dust-corrected emissivity spectra. The number of lines and samples varies depending on the observation, but most commonly is 1 and 1, respectively. All pixels are 4-byte IEEE real numbers. Pixels are stored in band-interleaved-by-pixel order. Mini-TES Mirror-dust-corrected Emissivity Averaged Mirror-Dust-Corrected Emissivity Image Cube 0 3 Last Index Fastest This image cube has 167 spectral bands. Wavenumbers are given in the Mini-TES Wavelength file. Typically there is 1 line and 1 4-byte floating-point pixel per line. Pixels are stored in band-interleaved-by-pixel order. IEEE754LSBSingle Line 7 1 Sample 3 2 Band 167 3