STRING--A VICAR labelled file with IBIS data structure. See help file for description of file format.
The name of an ASCII text file containing a list of filenames: /home/gmy/s001245663.img /project/gll/s004455667.abc /project/gll/s987654123.img The file may be created via a text editor. A maximum of 50 images can be included, one per line. The filename cannot exceed 80 characters. The list should contain images of the same target and be listed in the order of priority for the mosaic. The FILENAME parameter overrides the SCET and CAMERA parameters.
STRING - A list of C kernel types, one for each image, indicating the preferred source of the SPICE camera pointing information. Valid values are "DAVI","NAV ","FARE","NAV2","NEAR","AMOS", and "SEDR". If CKNAME is defaulted, or if the preferred source is not available, the best available camera pointing will be substituted (in the order listed above).
INTEGER - List of camera serial numbers, one for each image.
Not required if FILENAME keyword used.
Voyager camera serial numbers:
4 = VGR-2 WA 6 = VGR-1 WA
5 = VGR-2 NA 7 = VGR-1 NA
Galileo SSI camera serial numbers:
1 = full frame
2 = summation mode
Cassini ISS camera serial numbers:
1=NAC full frame 2=WAC full frame
21=NAC 2x2 summation 22=WAC 2x2 summation
41=NAC 4x4 summation 42=WAC 4x4 summation
Integer - The spacecraft event time for each frame in the mosaic.
Not required if FILENAME keyword used.
The SCETs are entered as groups of 6 integers, representing the year, day
hour, minute, second, and millisecond:
SCET=(1998,212,18,54,32,213, 1998,212,19,2,30,214, 1998,212,19,10,28,212)
String - The project ID. Valid are: VGR-1 VGR-2 GLL
REQUIRED PARAMETER Name of target body (planet, satellite, or asteroid). Ex: TARGET=GANYMEDE specifies that GANYMEDE is the target in the input image. A complete list of valid target names is located in the ASCII file assigned the logical name (or environmental variable) BODY_IDS.
SPICEMODE=LOCAL specifies that SPICE data is to be retrieved from local SPICE kernels. SPICEMODE=REMOTE specifies that SPICE data is to be retrieved 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.
USERID is a three character string which identifies the user who created the
camera pointing.
Ex: USERID=HBM identifies Helen Mortensen as the creator of the camera
pointing.
GROUPID is a three character string which identifies the group which created the camera pointing. Ex: GROUPID=040 identifies group 040 as the creator of the camera pointing.
INSTITUTE is a four character string identifying the facility which created the camera pointing. Ex: INSTITUTE=MIPS specifies that MIPS created the 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
PROGRAM is the first six characters of the program creating the camera pointing. Ex: PROGRAM=FARENC specifies that FARENC created the camera pointing.
SPKID specifies the four character ID which uniquely identifies the SP kernel used to create the camera pointing. The SP-kernel IDs are located in the ASCII file assigned the logical name (or environmental variable) KERNELDB. Ex: SPKID=N015 specifies the SP kernel GLL_LONG_2.BSP
REQUNUM is a four character string identifying the IPL request number for which the camera pointing was created. Ex: REQNUM=3456 identifies (somewhat) request number R123456
Date and time the camera pointing was created in the form 'YEARMMDDHHMM'.
Ex: CDATE=199602291200 specifies that the pointing was created at noon
on February 29, 1996.