urn:nasa:pds:cassini_vims_saturn:data_raw:1878580972 1.0 1.11.0.0 Product_Observational 2020-03-29 1.0 Initial PDS4 Version. Migrated from the PDS3 data product. This data file was migrated from the original PDS3 file: COVIMS_0093/data/2017193T185351_2017195T104358/v1878580972_1.qub The contents of this data file were reorganized in order to make it PDS4 compliant. Sideplanes and backplanes were removed from the cube itself and appended at the end of the file as separate arrays. The resulting data file remains compatible with ISIS2 standards. Values for instrument attributes were derived from the corresponding values in the original PDS3 label. 2017-07-12T18:53:41.171Z 2017-07-12T18:53:51.591Z Science Raw Visible Near Infrared Spectroscopy Spectral Cube Cassini-Huygens Mission urn:nasa:pds:context:investigation:mission.cassini-huygens data_to_investigation Cassini Orbiter Visual and Infrared Mapping Spectrometer Cassini Orbiter Spacecraft urn:nasa:pds:context:instrument_host:spacecraft.co is_instrument_host Cassini Orbiter Visual and Infrared Mapping Spectrometer Instrument VIMS urn:nasa:pds:context:instrument:vims.co is_instrument Saturn Rings Ring urn:nasa:pds:context:target:ring.saturn.rings data_to_target EXTENDED-EXTENDED MISSION 1 1878580983.220 1878580994.157 None known. OFF 1 SINGLE ZERO_SUB LOW VIMS_283RI_HRRADSCNL001_ISS.V1.ioi 16 1 ENABLED 59.822647 58.75959 233.43544 2017-194T20:51:02.704 2017-194T20:51:31.250 160. 10000. IR_DETECTOR_TEMP_HIGH_RES_1 IR_GRATING_TEMP IR_PRIMARY_OPTICS_TEMP IR_SPECTROMETER_BODY_TEMP_1 2 8.1 LOW LOW VIMS 10.0 05-24-2006 1878580955.13 SCIENCE OMEGA 2.932315 94.208 LINE 129.2229 128.822571 DISABLED 480. 415. NO 0 1878580972.13981 1878580983.04728 VIMS_283RI_HRRADSCNL001 OFF 132.951767 127.174942 273.93689 ON ON VIMS_283RI_HRRADSCNL001_ISS_027 2017-194T23:31:19.000 FINAL RINGS SATURN 1 ON ON HI-RES HI-RES BOTH S101 VIMS_283RI_HRRADSCNL001_ISS ENABLED ON OFF OFF 2017-193T18:53:41.171 2017-193T18:53:51.591 1 64 Information not provided 1 33 array-3d-spectrum display_settings_to_array This class specifies how two of the dimensions of the Array_3D_Spectrum object should be displayed in the vertical (line) and horizontal (sample) dimensions of a display device. Sample Left to Right Line Top to Bottom array-3d-spectrum spectral_characteristics_to_array_object 3D wavelength As described in detail by Brown et al. (2004), the size and shape of the VIMS instrument's field of view in any given product depends on a variety of parameters, including the swath_width, swath_length, instrument_mode_id, sampling_mode_id_ir, and sampling_mode_id_vis. Note that the fields of view are different for the visual and IR channels. Users of this product must consult the VIMS documentation in order to interpret the field of view of this product. urn:nasa:pds:cassini_vims_saturn:document:vims_instrument_description spectral_characteristics_to_document The binary portion of a VIMS file consists of two spatial and one spectral dimension (Sample, Line and Band in ISIS terminology). While the spatial dimensions of the cube core vary, nearly all cubes consist of 352 spectral bands (planes). A very small number of cubes contain only 256 bands, corresponding to the IR wavelengths only. If the value of the attribute cassini:spectral_summing_flag is ON, this cube was obtained using spectral summing in steps of eight spectral bins. The values you will find within each set of eight adjacent bins should be identical in this file, although in rare cases isolated NULLs and/or erroneous values may be found. urn:nasa:pds:cassini_vims_saturn:calibration:wavelength-bins-2017.5000 spectral_characteristics_to_bin_center_values This mapping from bin number (1-352) to wavelength is based on the RC19 pipeline. Note that it accounts for observed time variations in the mapping. This table updates the corresponding information contained in the original PDS3 labels. Those original values, based on ground-based calibration, are retained in the ISIS2 header of this data file. For those few files with 256 bands instead of 352, skip over the first 96 rows of this table. urn:nasa:pds:cassini_vims_saturn:calibration:wavelength-bins-2017.5000 spectral_characteristics_to_bin_width_values This mapping from bin number (1-352) to wavelength bin width is approximate, based on the assumption that each wavelength bin extends half-way to its neighboring bins. urn:nasa:pds:cassini_vims_saturn:data_raw:index data_to_resource The cumulative index table of basic parameters associated with each observation. urn:nasa:pds:cassini_vims_saturn:data_raw:body-geometry data_to_resource The cumulative index table of body surface geometry information associated with each observation. urn:nasa:pds:cassini_vims_saturn:data_raw:body-inventory data_to_resource The cummulative index listing every Saturn system body expected to fall within each field of view. urn:nasa:pds:cassini_vims_saturn:data_raw:ring-geometry data_to_resource The cumulative index table of ring geometry information associated with each observation. urn:nasa:pds:cassini_vims_saturn:document:vims-wavelength-and-radiometric-calibration-report data_to_document Nominally, this refers to the VIMS Wavelength and Radiometric Calibration 19, Final Report, Clark et. al., January 25, 2018. In the event that the 2018 report is not the final Final Calibration Report, this LID will refer to the lastest version of the report. The report provides details for wavelength and radiometric calibration of Cassini VIMS data. It Includes adjustments for shifts in the wavelength calibration of the spectrometer which occurred during various post-launch mission phases. urn:nasa:pds:cassini_vims_saturn:document:vims-ir-pixel-timing data_to_document The VIMS IR Pixel Timing document, Brown and Soderblom (2018), which provides details for calculating the time offset for each VIMS IR pixel. urn:nasa:pds:cassini_vims_saturn:document:vims_instrument_description data_to_document An overview of the instrument and its components. This information was extracted from the PDS3 instrument catalog file. urn:nasa:pds:cassini_vims_saturn:browse_raw:1878580972-full data_to_browse The browse image in PNG format that illustrates the scientific content of this product. 10.1007/s11214-004-1453-x Brown, R. H. et al., The Cassini Visual And Infrared Mapping Spectrometer (VIMS) Investigation, Space Science Reviews, Volume 115, Issue 1-4, pp. 111-168, 2004. CO-E/V/J/S-VIMS-2-QUBE-V1.0:COVIMS_0093:data/2017193T185351_2017195T104358:v1878580972_1.qub data_to_raw_source_product PDS RMS Node The original PDS3 version of this product. The form of the reference is dataset_id:volume_id:directory_path:file_name. 1878580972.qub 2020-01-12T21:50:47Z cd62068bbec34ddf1b3ccd2aaa683cf4 3D Spectral Array with suffix planes This file contains multiple objects. The Composite_Structure class provides associations between the primary data object and the supplementary objects. This refers to the primary data array. The axes are (Line, Band, Sample). array-3d-spectrum has_primary_component This refers to a sideplane visualized as an extension of the sample axis. The axes are (Line,Band). The values are background data. sideplane has_component This refers to the SLICE_TIME_SECONDS backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. backplane-SLICE_TIME_SECONDS has_component This refers to the SLICE_TIME_TICKS backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. backplane-SLICE_TIME_TICKS has_component This refers to the IR_DETECTOR_TEMP_HIGH_RES_1 backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. backplane-IR_DETECTOR_TEMP_HIGH_RES_1 has_component This refers to the IR_GRATING_TEMP backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. backplane-IR_GRATING_TEMP has_component This refers to the IR_PRIMARY_OPTICS_TEMP backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. backplane-IR_PRIMARY_OPTICS_TEMP has_component This refers to the IR_SPECTROMETER_BODY_TEMP_1 backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. backplane-IR_SPECTROMETER_BODY_TEMP_1 has_component array-3d-spectrum sideplane has_backplane array-3d-spectrum backplane-SLICE_TIME_SECONDS has_backplane array-3d-spectrum backplane-SLICE_TIME_TICKS has_backplane array-3d-spectrum backplane-IR_DETECTOR_TEMP_HIGH_RES_1 has_backplane array-3d-spectrum backplane-IR_GRATING_TEMP has_backplane array-3d-spectrum backplane-IR_PRIMARY_OPTICS_TEMP has_backplane array-3d-spectrum backplane-IR_SPECTROMETER_BODY_TEMP_1 has_backplane

ISIS2 Header isis-header 0 16384 ISIS2

Processing History isis-history 16384 12800 ISIS2 History Label

Raw Data Number array-3d-spectrum 29184 3 Last Index Fastest SignedMSB2 Line 1 1 Band wavelength-axis 352 2 Sample 64 3 -8192 -32765 -32764 -4095 -32766 -32767 Sample Suffix Backgrounds sideplane 74240 2 Last Index Fastest This sideplane is visualized as an extension of the sample axis. The axes are (Line,Band). The values are background data; however the visual and IR channels populate this array differently; See the documentation referenced in the Reference_Area above. SignedMSB4 Line 1 1 Band 352 2 -8192 -32765 -32764 -4095 -32766 -32767 Backplane SLICE_TIME_SECONDS backplane-SLICE_TIME_SECONDS 75776 2 Last Index Fastest This is the SLICE_TIME_SECONDS backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. SignedMSB4 sec Line 1 1 Sample 64 2 -8192 Backplane SLICE_TIME_TICKS backplane-SLICE_TIME_TICKS 76032 2 Last Index Fastest This is the SLICE_TIME_TICKS backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. SignedMSB4 sec Line 1 1 Sample 64 2 -8192 Backplane IR_DETECTOR_TEMP_HIGH_RES_1 backplane-IR_DETECTOR_TEMP_HIGH_RES_1 76288 2 Last Index Fastest This is the IR_DETECTOR_TEMP_HIGH_RES_1 backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. SignedMSB4 sec Line 1 1 Sample 64 2 -8192 Backplane IR_GRATING_TEMP backplane-IR_GRATING_TEMP 76544 2 Last Index Fastest This is the IR_GRATING_TEMP backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. SignedMSB4 sec Line 1 1 Sample 64 2 -8192 Backplane IR_PRIMARY_OPTICS_TEMP backplane-IR_PRIMARY_OPTICS_TEMP 76800 2 Last Index Fastest This is the IR_PRIMARY_OPTICS_TEMP backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. SignedMSB4 sec Line 1 1 Sample 64 2 -8192 Backplane IR_SPECTROMETER_BODY_TEMP_1 backplane-IR_SPECTROMETER_BODY_TEMP_1 77056 2 Last Index Fastest This is the IR_SPECTROMETER_BODY_TEMP_1 backplane, which can be visualized as an extension of the Band (wavelength) axis. The axes are (Line,Sample). Values are four-byte integers. SignedMSB4 sec Line 1 1 Sample 64 2 -8192 Corner Array corner 77312 2 Last Index Fastest SignedMSB4 Backplane 6 1 Line 1 2 Padding Bytes from PDS3 File padding 77824 1 Last Index Fastest UnsignedByte padding 104 1