This program must be run in a LOCATION_NAME with a x,y coordinate system (i.e., a coordinate system with projection 0). For further information regarding this LOCATION_NAME refer to the manual entry for imagery.
The first prompt in i.tape.mss asks the user for the tape device name. This is sometimes /dev/rmt0 (for a half-inch tape with a tape density of 1600), but this varies with each machine.
The next prompt is:
Please mount and load tape, then hit RETURN -->
please enter the following information
Tape Identification: __
Image Description: __
Title for the Extracted Raster (Cell) Files: __
AFTER COMPLETING ALL ANSWERS, HIT TO CONTINUE
(OR TO CANCEL)
This program automatically enters the scene ID number and
the date of the image into the field for Tape
Identification. The sun angles are automatically entered
into the field for Image Description.
The second menu is:
MSS TAPE EXTRACTION
please select the desired tape window (geographic
region definition) to extract
first row: _______(1-2984)
last row: _______(1-2984)
first col: _______(1-3548)
last col: _______(1-3548)
AFTER COMPLETING ALL ANSWERS, HIT TO CONTINUE
(OR TO CANCEL)
The numbers in parentheses are the total number of rows and
columns on the tape including filler (zeros). This
information and additional information can also be obtained
by running the GRASS program
i.tape.mss.h which
reads the header information on an MSS tape. Any subset of
the image on tape may be extracted. For a discussion of
row and column extraction see the subheading titled
ROW AND
COLUMN EXTRACTION below.
The next menu is:
please make an x by the bands you want extracted
_____ 1
_____ 2
_____ 3
_____ 4
AFTER COMPLETING ALL ANSWERS, HIT TO CONTINUE
(OR TO CANCEL)
MSS imagery has 4 bands, but the user may want to extract
only a subset of these bands. See the subheading in this entry
titled
ROW AND COLUMN EXTRACTION.
The user then is asked to enter the prefix/group for the band files to be created. This name will precede each band file extracted into GRASS. For example, if three bands are extracted the following three (raster) band files will result:
prefixname.1
prefixname.2
prefixname.3
Whatever prefixname is specified will also automatically become the name for the imagery group file being created. Each image (i.e., each run of i.tape.mss) should be given a unique prefix/group name.
The extraction process will begin by first skipping the number of specified files, advancing to the starting row, and then reading the tape. The percent completion of the extraction is displayed on the screen. If more than one tape is required to store the image, the program will pause and inform the user to mount the next tape.
The extracted (raster) band files will be listed as raster map layers available in the current MAPSET and may be displayed using the GRASS commands d.display, d.rast or i.points.
This program is interactive and requires no command line arguments.
ROW AND COLUMN EXTRACTION
The display options in GRASS allow the user to locate rows and
columns on the digital image. If enough disk space is available, one
band of an entire image, or one band of a portion of an image known to
contain the area of interest, can be extracted and displayed. The
measurements
option in d.display, or
d.where (following the use of
d.rast) will echo
x and y coordinates to the screen. (These coordinates will display
negative numbers in the north-south direction, but ignoring the negative
sign will yield the row number.) See the
imagery manual entry
for further explanation.
If a photograph of the digital image is available, the rows and columns to be extracted can be determined from it by associating inches with the total number of known rows and columns in the scene. For example, if the total length of the photograph is 12 inches, the total number of rows on the tape is 2000, and the northwest corner of the area of interest begins 2 inches from the top of the photo, then:
12" / 2000 rows = 2" / x rows x = 333.333The northwest corner of the area of interest starts at row 333. The starting row, ending row, starting column, and ending column can be calculated in this manner.
d.display, d.rast, d.where, i.group, i.points, i.tape.mss.h, i.tape.other, i.tape.tm, imagery