String Name of the input IBIS SEDR file.
The project ID.
Specifies whether the data is in OBJECT space (geometricaly corrected) or IMAGE space (uncorrected). IMAGE (uncorrected) is only valid for GLL project.
The spacescraft event time for each image. Required only for GLL project. If omitted the scet times will be extracted from columns 32-37 in the input ibis file. Groups of 6 integers for each image in the order: Year, day, hour, minute, second, milisecond.
Keyword
Indicator of whether to update or not update the Voyager SEDR file.
Valid: UPDATE and NOUPDATE. Default: NOUPDATE.
Array of Integers The serial number of the camera which took all images. By default the program will obtain the cameras from the input IBIS file. This parameter is used to override the camera s/n specified in the IBIS table. If the override is desired on the n-th record, all cameras from the first record up to the n-th are to be specified. For GLL's case, which actually has only one camera, this parameter specifies if an image was taken in Full Frame Mode (CAMERA = 1) or Summation Mode (CAMERA = 2).
Ex: TARGET=GANYMEDE specifies that GANYMEDE is the target in the input image. The TARGET may be a planet, satellite, or asteroid. A complete list of valid target names is located in the ASCII file assigned the logical name (or environmental variable) BODY_IDS. If defaulted, the target is retrieved from the VICAR label or other TBD means.
SPICEMODE=LOCAL specifies that SPICE data is to be accessed from local SPICE kernels. SPICEMODE=REMOTE specifies that SPICE data is to be accessed via the SPICE server. If SPICEMODE is defaulted, the logical name (or environmental variable) DEFAULTSPICE is used to determine whether LOCAL or REMOTE is used. Note that if SPICE data is not found in LOCAL or REMOTE mode, the other mode is attempted in order to retrieve SPICE data. However, when improved camera pointing data is stored, only the specified or default mode is used.
INSTITUTE is a four character string identifying the facility which creates
the improved (C-Smithed) camera pointing. If defaulted, the value of the
logical name (or environmental variable) VICAR_SITE is used.
Ex: INSTITUTE=ASU identifies ASU as the creator of the improved camera
pointing.
PURPOSE is a four character string identifying the purpose of the observation or the purpose of processing. For example, PURPOSE=MOSA identifies the image as part of a mosaic sequence PURPOSE=COLO identifies the image as part of a color sequence
REQUNUM is a four character string identifying the IPL request number for which the camera pointing was created. REQNUM must contain exactly 4 digits. Ex: REQNUM=0123 identifies (somewhat) request number R000123
Date and time the camera pointing was created in the form 'YEARMMDDHHMM'.
The date string must contain exactly 12 digits.
Ex: CDATE=199602291200 specifies that the pointing was created at noon
on February 29, 1996.
If defaulted, the current date and time is used.
GROUPID is a three character string which identifies the group of the user running this program to store improved camera pointing. (The user ID is automatically determined by the program). Ex: GROUPID=040 identifies group 040 as the creator of the camera pointing. On VMS, this parameter is ignored since the program automatically determines the group ID of the current user. If GROUPID is defaulted on Unix, the program uses the value of the environmental variable GROUPID. Note that GROUPID is not a system-defined variable, and should be defined in your .cshrc as in the following example: Ex: setenv GROUPID 040