PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = "2004-10-1, Initial 2014-03-25, update for ir_perf changes" RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2004-02-03 NOTE = " calinfo.txt describes the contents of this directory." END_OBJECT = TEXT END This directory contains calibration files for use with the software programs in the software directory. These files are described below. calinfo.txt = (this file) describes the content of this directory. example_kernels.def = Example kernels list for calculating geometric backplane information. ir_flatfield.lbl = Detached label for the ir_flatfield.qub. ir_flatfield.qub = Data cube used by the calibration routine to flatfield or normalize the pixels of the IR portion of a VIMS cube taken in the NORMAL mode with respect to the bore sight. ir_flatfield_ss.lbl = Same as above, but for spectrally summed cubes. ir_flatfield_ss.qub = Same as above, but for spectrally summed cubes. ir_hires_flatfield.lbl = Detached label for the ir_nyquist_flatfield.qub. ir_hires_flatfield.qub = Data cube used by the calibration routine to flatfield or normalize the pixels of the IR portion of a VIMS cube taken in the HIRES mode with respect to the bore sight. ir_hires_flatfield_ss.lbl = Same as above, but for spectrally summed cubes. ir_hires_flatfield_ss.qub = Same as above, but for spectrally summed cubes. ir_nyquist_flatfield.lbl = Detached label for the ir_nyquist_flatfield.qub. ir_nyquist_flatfield.qub = Data cube used by the calibration routine to flatfield or normalize the pixels of the IR portion of a VIMS cube taken in the NYQUIST mode with respect to the bore sight. ir_nyquist_flatfield_ss.lbl = Same as above, but for spectrally summed cubes. ir_nyquist_flatfield_ss.qub = Same as above, but for spectrally summed cubes. ir_perf_352.lbl = Detached label for the ir_perf_352.cub ir_perf_352.qub = Data cube used by the calibration routine to convert detector counts to photons at the detector for the IR portion of a VIMS cube. (RC17 version released March 2014). ir_perf.lbl-old_V1 = Detached label for the ir_perf.qub-old_V1. ir_perf.qub-old_V1 = Data cube used by the calibration routine to convert detector counts to photons at the detector for the IR portion of a VIMS cube. ir_perf_ss.lbl = Same as above, but for spectrally summed cubes. ir_perf_ss.qub = Same as above, but for spectrally summed cubes. solar.lbl = Detached label for the solar.qub solar.qub = Data cube used by the calibration routine to remove solar color the VIMS data. Contains solar spectrum. solar_ss.lbl = Same as above, but for spectrally summed cubes. solar_ss.qub = Same as above, but for spectrally summed cubes. vis_flatfield.lbl = Detached label for the vis_flatfield.qub. vis_flatfield.qub = Data cube used by the calibration routine to flatfield or normalize the pixels of the VIS portion of a VIMS cube taken in the NORMAL mode with respect to the bore sight. vis_flatfield_ss.lbl = Same as above, but for spectrally summed cubes. vis_flatfield_ss.qub = Same as above, but for spectrally summed cubes. vis_hires_dark_model.lbl = Detached label for the vis_hires_dark_model.tab. vis_hires_dark_model.tab = Data table used by the calibration routine to remove the dark background. from the VIS portion of a VIMS cube. vis_hires_flatfield.lbl = Detached label for the vis_hires_flatfield.qub. vis_hires_flatfield.qub = Data cube used by the calibration routine to flatfield or normalize the pixels of the VIS portion of a VIMS cube taken in the HIRES mode with respect to the bore sight. vis_hires_flatfield_ss.lbl = Same as above, but for spectrally summed cubes. vis_hires_flatfield_ss.qub = Same as above, but for spectrally summed cubes. vis_lowres_dark_model.lbl= Detached label for the vis_lowres_dark_model.tab. vis_lowres_dark_model.tab= Data table used by the calibration routine to remove the dark background. from the VIS portion of a VIMS cube. vis_perf.lbl = Detached label for the vis_perf.qub. vis_perf.qub = Data cube used by the calibration routine to convert detector counts to photons at the detector for the VIS portion of a VIMS cube. vis_perf_ss.lbl = Same as above, but for spectrally summed cubes. vis_perf_ss.qub = Same as above, but for spectrally summed cubes. wavecal.lbl = Detached label for the wavecal.qub. wavecal.qub = Data cube used by the calibration routine. Contains: (h*c) --------------------------- (lambda*A*omega*delta_lambda) where lambda is the wavelength in microns, A is the area of the primary mirror in square centimeters, omega is the solid angle subtended by a pixel in steradians, and delta_lambda is width of the spectel. wavecal_ss.lbl = Same as above, but for spectrally summed cubes. wavecal_ss.qub = Same as above, but for spectrally summed cubes. IR_NORMAL_uv.bin = Unit vector file used for creating geometric backplanes during data calibration. IR_HI-RES_uv.bin = Unit vector file used for creating geometric backplanes during data calibration. IR_UNDER_uv.bin = Unit vector file used for creating geometric backplanes during data calibration. VIS_NORMAL_uv.bin = Unit vector file used for creating geometric backplanes during data calibration. VIS_HI-RES_uv.bin = Unit vector file used for creating geometric backplanes during data calibration.