Data Set Information
DATA_SET_NAME VG1/VG2 SATURN IMAGING SCIENCE SUBSYSTEM PROCESSED V1.1
DATA_SET_ID VG1/VG2-S-ISS-2/3/4/6-PROCESSED-V1.1
NSSDC_DATA_SET_ID
DATA_SET_TERSE_DESCRIPTION Voyager images from the Saturn encounters after various levels of processing, including cleaned, calibrated and geometrically corrected forms.
DATA_SET_DESCRIPTION
Data Set Overview
    =================
      This is a regeneration of the Voyager 1 and 2 images from Saturn,
      in multiple versions including decompressed raw, cleaned,
      calibrated and geometrically corrected forms. It has been
      derived from the earlier PDS data set VG1/VG2-S-ISS-2-EDR-V1.0,
      which appeared on volumes VG_0004, VG_0005, and VG_0026 to
      VG_0038.
 
      The information covers Voyager 1 and 2 at Saturn (1980 and
      1981), including the planet, its satellites and rings. Pointing
      information is not included in this data set.

      The data set is organized chronologically for each Voyager
      encounter. Volumes VGISS_6101-6107 contain the Voyager 1 images;
      volumes VGISS_6201-6212 contain the Voyager 2 images. For each
      Voyager image, the following files are included:

      RAW     - The decompressed raw image.
      RESLOC  - A table of reseau locations.
      GEOMA   - A table of tiepoints describing the geometric
                correction of the image.
      CLEANED - The raw image with various spikes, blemishes and
                reseau markings removed.
      CALIB   - The calibrated image, in which data numbers are
                directly proportional to reflectivity.
      GEOMED  - The geometrically corrected version of the calibrated
                image.

      All images and binary tables are provided in VICAR format, as
      defined by JPL's Multimission Image Processing Laboratory
      (MIPL). A VICAR file begins with an ASCII header describing the
      structure of the file. ASCII text versions of the binary tables
      are also included.

      Processing Level Id            : {2, 3, 4, 6}
      Software Flag                  : N
      Processing Start Time          : 2005-09-01
      Processing Stop Time           : 2012-06-01


      Overview of the Data Set from the Original DATASET.CAT
      ------------------------------------------------------
 
      NASA's Voyager Project and the Planetary Data System (PDS) have
      created an archive of planetary digital images acquired by the
      twin Voyager spacecraft (Voyager 1 and Voyager 2). This
      Voyager data set encompasses Experiment Data Record (EDR) files
      from the Saturn encounters.
 
      The information covers Voyager 1 and 2 at Saturn (1981),
      including the planet, its satellites and rings.  It is
      important to note the fact that while geometry information and
      calibration files exist for all of the Voyager data sets, they
      do not exist in the EDR data set but both are available
      separately through the PDS-JPL Imaging Node.  Neither does the
      data set include Plasma Radio Astronomy (PRA) or Plasma Wave
      Spectrometer (PWS) image-formatted information.  These too are
      available separately through the Imaging Node.
 
      This data set exists on magnetic tapes in EDR format.  This
      format is explained in the Multimission Image Processing
      Laboratory (MIPL) Real-Time Processing Subsystem Software
      Design Document (1985), an internal JPL document available from
      the JPL vellum files.  A subset of these images also exists on
      CD-ROM (reference VG1/VG2-S-ISS-2-EDR-V2.0).
 
      Detail Target Clarification:
 
      There are two targets which may prove to be confusing for the
      unfamiliar user; PLAQUE and CAL LAMPS, both are used as
      calibration targets.  PLAQUE is an image of a flat piece of
      metal illuminated by the sun.  CAL LAMPS are lamps inside the
      camera used for illumination.
 
      The target DARK is a dark current image when the camera mode is
      BODARK and the exposure is zero.  DARK SKY and SKY are
      shuttered images, non-zero exposures looking at dark sky.
 
      SCAT_LIGHT images are used to measure how much light is
      scattered in a particular direction.
 
      The set of images on the magnetic tapes are raw; no processing
      has been performed other than organizing the original telemetry
      into raster-formatted files.
 
      Definition Clarification:
 
      Planetodetic latitude of a point on the planet surface is the
      angle between the surface normal and the equatorial plane.  For
      a spherical body, the latitude is incidental to the
      planetocentric latitude.
 
      The p5 point is one of 6 static points on all images.  It is
      the point located in the center of the image.  The p1 point is
      located in the top left corner, p2 top right corner, p3 bottom
      left corner, p4 bottom right corner, p5 center, p6 center right
      edge.  If the target is not on the p5 point then that point
      does not have latitude and longitude coordinates associated
      with it nor does the target have a p5 point.
 
      The spacecraft coordinate system is a coordinate system defined
      by the spacecraft structure.  The antenna points along the +z
      axis, the booms are along the +y and -y axes, creating a unique
      coordinate system for each spacecraft.
 
      The Canopus coordinate system is the coordinate system defined
      by the axis pointing at Canopus, one pointing at the Sun and
      one pointing somewhere else.
 
      These systems are not used for describing images or points on
      images.  Because our interest is in where the pixels lie, not
      relative to the spacecraft or stars but relative to the
      target's own system.
 
      Processing Level Id            : 2
      Software Flag                  : N
      Processing Start Time          : 1980-11-01
      Processing Stop Time           : 1982-10-01
 
    Parameters
    ==========
 
      Data Set Parameter 'DATA NUMBER'
      --------------------------------
        Data Number is an integer expressing the digital value of each
        pixel in an image.
 
        Sampling Parameter Name        : PIXEL
        Data Set Parameter Name        : DATA NUMBER
        Data Set Parameter Unit        : DIMENSIONLESS
 
      Data Set Parameter 'PIXEL COORDINATE'
      --------------------------------
        Pixel coordinate is a real value expressing the horizontal or
        vertical location in an image. Coordinates are numbered in
        units of image pixels, beginning at one.
 
        Sampling Parameter Name        : PIXEL
        Data Set Parameter Name        : PIXEL COORDINATE
        Data Set Parameter Unit        : DIMENSIONLESS
 
 
    Source Instrument Parameters
    ============================
      Instrument Host ID              : VG1
      Data Set Parameter Name         : DATA NUMBER
      Instrument Parameter Name       : RADIANCE
      Important Instrument Parameters : 1
 
 
      Instrument Host ID              : VG2
      Data Set Parameter Name         : DATA NUMBER
      Instrument Parameter Name       : RADIANCE
      Important Instrument Parameters : 1
 
 
    Processing
    ==========
 
      Processing History
      ------------------
        Source Data Set ID          : VG1/VG2-S-ISS-2-EDR-V1.0
        Software                    : VGRCDCOPY
        Product Data Set ID         : RAW IMAGE

        Source Data Set ID          : RAW IMAGE
        Software                    : VGRFILLIN
        Product Data Set ID         : VGRFILLIN IMAGE

        Source Data Set ID          : VGRFILLIN IMAGE
        Software                    : RESLOC
        Product Data Set ID         : {RESEAU TABLE, TIEPOINT TABLE}

        Source Data Set ID          : {VGRFILLIN IMAGE, RESEAU TABLE,
                                       BLEMISH TABLE}
        Software Name               : RESSAR77
        Product Data Set ID         : RESSAR77 IMAGE

        Source Data Set ID          : RESSAR77 IMAGE
        Software Name               : ADESPIKE
        Product Data Set ID         : CLEANED IMAGE

        Source Data Set ID          : {CLEANED IMAGE, DARK CURRENT
                                       IMAGE, CALIBRATION MODEL}
        Software Name               : FICOR77
        Product Data Set ID         : CALIBRATED IMAGE

        Source Data Set ID          : {CALIBRATED IMAGE, TIEPOINT
                                       TABLE}
        Software Name               : GEOMA
        Product Data Set ID         : GEOMETRICALLY CORRECTED IMAGE
 
      Software 'VGRCDCOPY'
      --------------------
        VICAR routine VGRCDCOPY decompresses a raw, EDR image as
        archived in PDS data set VG1/VG2-S-ISS-2-EDR-V1.0. It creates
        the RAW version of the image with a VICAR header.

        Source Data Set ID          : COMPRESSED RAW IMAGE
        Software Name               : VGRCDCOPY
        Product Data Set ID         : RAW IMAGE
        Software Type               : N/A
        Software Release Date       : UNK
        Node ID                     : IMAGING
        Cognizant Engineer          : SUSAN K. LAVOIE
        Software Access Description : MIPL
 
      Software 'VGRFILLIN'
      --------------------
        VICAR routine VGRCDCOPY fills in incomplete lines with the
        average of the adjacent lines.
 
        Source Data Set ID          : RAW IMAGE
        Software Name               : VGRFILLIN
        Product Data Set ID         : VGRFILLIN IMAGE
        Software Type               : N/A
        Software Release Date       : UNK
        Node ID                     : IMAGING
        Cognizant Engineer          : SUSAN K. LAVOIE
        Software Access Description : MIPL
 
      Software 'RESLOC'
      -----------------
        VICAR routine RESLOC locates the reseau markings within the
        Voyager image.
 
        Source Data Set ID          : VGRFILLIN IMAGE
        Software Name               : RESLOC
        Product Data Set ID         : {RESEAU TABLE, TIEPOINT TABLE}
        Software Type               : N/A
        Software Release Date       : UNK
        Node ID                     : IMAGING
        Cognizant Engineer          : SUSAN K. LAVOIE
        Software Access Description : MIPL
 
      Software 'RESSAR77'
      -------------------
        VICAR routine RESSAR77 erases reseau markings and blemishes by
        replacing them with an average of the adjacent images.
 
        Source Data Set ID          : {VGRFILLIN IMAGE, RESEAU TABLE,
                                       BLEMISH TABLE}
        Software Name               : RESSAR77
        Product Data Set ID         : RESSAR77 IMAGE
        Software Type               : N/A
        Software Release Date       : UNK
        Node ID                     : IMAGING
        Cognizant Engineer          : SUSAN K. LAVOIE
        Software Access Description : MIPL
 
      Software 'ADESPIKE'
      -------------------
        VICAR routine ADESPIKE erases spikes in the images by
        replacing them with an average of the adjacent images.
 
        Source Data Set ID          : RESSAR77 IMAGE
        Software Name               : ADESPIKE
        Product Data Set ID         : CLEANED IMAGE
        Software Type               : N/A
        Software Release Date       : UNK
        Node ID                     : IMAGING
        Cognizant Engineer          : SUSAN K. LAVOIE
        Software Access Description : MIPL
 
      Software 'FICOR77'
      ------------------
        VICAR routine FICOR77 subtracts a dark current and rescales
        the image into calibrated values.
 
        Source Data Set ID          : {CLEANED IMAGE, DARK CURRENT
                                       IMAGE, CALIBRATION MODEL}
        Software Name               : FICOR77
        Product Data Set ID         : CALIBRATED IMAGE
        Software Type               : N/A
        Software Release Date       : UNK
        Node ID                     : IMAGING
        Cognizant Engineer          : SUSAN K. LAVOIE
        Software Access Description : MIPL
 
      Software 'GEOMA'
      ------------------
        VICAR routine GEOMA resamples a Voyager image to remove its
        intrinsic geometric distortion.
 
        Source Data Set ID          : {CALIBRATED IMAGE, TIEPOINT
                                       TABLE}
        Software Name               : GEOMA
        Product Data Set ID         : GEOMETRICALLY CORRECTED IMAGE
        Software Type               : N/A
        Software Release Date       : UNK
        Node ID                     : IMAGING
        Cognizant Engineer          : SUSAN K. LAVOIE
        Software Access Description : MIPL


    Change History
    ==============
        Version 1.0 of this data set was released on May 31, 2012.

        Version 1.1 was released on January 31, 2014. This revision
        corrects a number of errors noted in the PDS labels of the data
        files. No data files have been modified. Indices and
        documentation are also unchanged.
DATA_SET_RELEASE_DATE 2014-01-31T00:00:00.000Z
START_TIME 1980-09-24T12:00:00.000Z
STOP_TIME 1981-10-05T12:00:00.000Z
MISSION_NAME VOYAGER
MISSION_START_DATE 1972-07-01T12:00:00.000Z
MISSION_STOP_DATE N/A (ongoing)
TARGET_NAME SKY
SYSTEM
DIONE
HELENE
CALYPSO
JANUS
DARK
HYPERION
PHOEBE
TITAN
S RINGS
RHEA
STAR
TETHYS
SATURN
ENCELADUS
EPIMETHEUS
IAPETUS
MIMAS
TELESTO
PANDORA
TARGET_TYPE CALIBRATION
UNKNOWN
SATELLITE
SATELLITE
SATELLITE
SATELLITE
CALIBRATION
SATELLITE
SATELLITE
SATELLITE
RING
SATELLITE
STAR
SATELLITE
PLANET
SATELLITE
SATELLITE
SATELLITE
SATELLITE
SATELLITE
SATELLITE
INSTRUMENT_HOST_ID VG2
VG1
INSTRUMENT_NAME IMAGING SCIENCE SUBSYSTEM - NARROW ANGLE
IMAGING SCIENCE SUBSYSTEM - NARROW ANGLE
IMAGING SCIENCE SUBSYSTEM - WIDE ANGLE
IMAGING SCIENCE SUBSYSTEM - WIDE ANGLE
INSTRUMENT_ID ISSN
ISSN
ISSW
ISSW
INSTRUMENT_TYPE CAMERA
CAMERA
VIDICON CAMERA
VIDICON CAMERA
NODE_NAME Planetary Rings
ARCHIVE_STATUS LOCALLY ARCHIVED
CONFIDENCE_LEVEL_NOTE
Overview
    ========
      This data set represents a complete collection of images from
      Voyager 1 & 2 Saturn encounters beginning with the Observatory
      Phase.

      The image processing history represents our best understanding
      of the cameras circa the early 1990's. The programs used to
      process the images have not been updated in any significant way
      since the Voyager 2 Neptune encounter in 1989. Absolute
      calibration is probably accurate to the level of 5-10%; relative
      calibration of images through the same camera and filter is
      better. Absolute calibration of the Voyager 2 data set is
      probably somewhat more accurate due to results from the
      subsequent Uranus and Neptune encounters.

      NOTE: No calibration model is available for filters NAD (sodium)
      and CH4_JS on the Voyager 1 wide angle camera. For these images,
      the Voyager 2 models are substituted. However, the cameras have
      different gains so these images are not photometrically
      accurate in absolute terms.

      Zero values in the images are based on a dark current
      subtraction; these values are probably accurate to the level of
      a few data numbers. Comparison of reference dark current images
      taken close in time can be used to estimate the systematic
      variations.
CITATION_DESCRIPTION Showalter, M.R., Gordon, M.K., and D. Olson, VG1/VG2 SATURN IMAGING SCIENCE SUBSYSTEM PROCESSED V1.1, VG1/VG2-S-ISS-2/3/4/6-PROCESSED-V1.1, 2014.
ABSTRACT_TEXT This data set contains all of the Voyager images from Saturn in cleaned, calibrated and geometrically corrected forms. It is derived from data set VG1/VG2-S-ISS-2-EDR-V1.0.
PRODUCER_FULL_NAME MARK R. SHOWALTER
SEARCH/ACCESS DATA
  • Rings Online Archives