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Text File | 1990-06-25 | 55.4 KB | 1,585 lines |
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- Draft version of
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- PC-MIPS User Manual
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- as of 04/19/90
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- PC-MIPS User Manual
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- Table of Contents
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- PC-MIPS Overview . . . . . . . . . . . . . . . . . . . 1
- Installing PC-MIPS . . . . . . . . . . . . . . . . . . 5
- User Interface . . . . . . . . . . . . . . . . . . . . 5
- Image Data Structure . . . . . . . . . . . . . . . . . . 6
- User Input . . . . . . . . . . . . . . . . . . . . . . 7
- PC-MIPS Programs
- CMBIMG . . . . . . . . . . . . . . . . . . . . . . . . 8
- DERIV . . . . . . . . . . . . . . . . . . . . . . . . 8
- EDGENH . . . . . . . . . . . . . . . . . . . . . . . . 9
- EXT_ROI . . . . . . . . . . . . . . . . . . . . . . . . 10
- FLT8B . . . . . . . . . . . . . . . . . . . . . . . . *
- IMDISP . . . . . . . . . . . . . . . . . . . . . . . . 10
- LIST . . . . . . . . . . . . . . . . . . . . . . . . 10
- MAPIMG . . . . . . . . . . . . . . . . . . . . . . . . 11
- MAPLN1 . . . . . . . . . . . . . . . . . . . . . . . . 12
- MDGRAD . . . . . . . . . . . . . . . . . . . . . . . . 13
- MEDIAN . . . . . . . . . . . . . . . . . . . . . . . . 13
- MIXBDS . . . . . . . . . . . . . . . . . . . . . . . . *
- NUVU . . . . . . . . . . . . . . . . . . . . . . . . *
- OVRLAY . . . . . . . . . . . . . . . . . . . . . . . . 14
- PCA . . . . . . . . . . . . . . . . . . . . . . . . *
- PICSTR . . . . . . . . . . . . . . . . . . . . . . . . *
- RADARS . . . . . . . . . . . . . . . . . . . . . . . . *
- RATIO . . . . . . . . . . . . . . . . . . . . . . . . 16
- ROI . . . . . . . . . . . . . . . . . . . . . . . . 17
- ROTATE . . . . . . . . . . . . . . . . . . . . . . . . 17
- SALTP . . . . . . . . . . . . . . . . . . . . . . . . 18
- SCALE . . . . . . . . . . . . . . . . . . . . . . . . *
- SHAD2 . . . . . . . . . . . . . . . . . . . . . . . . 19
- SHADRF . . . . . . . . . . . . . . . . . . . . . . . . *
- STATS . . . . . . . . . . . . . . . . . . . . . . . . *
- STEEP . . . . . . . . . . . . . . . . . . . . . . . . *
- STENCL . . . . . . . . . . . . . . . . . . . . . . . . *
- STRTCH . . . . . . . . . . . . . . . . . . . . . . . . 20
- SUBIMG . . . . . . . . . . . . . . . . . . . . . . . . 21
- SUN . . . . . . . . . . . . . . . . . . . . . . . . *
- WTCMBO . . . . . . . . . . . . . . . . . . . . . . . . 21
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- * - program write-up, as yet, not completed.
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- PC-MIPS User Manual
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- PC-MIPS Overview
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- Historically, the processing and analysis of GLORIA side-
- scan sonar data within the U.S. Geological Survey has been done
- on DEC mini-computers using the MIPS software system. Due to the
- volume of work generated by the EEZ sea-floor mapping program,
- these systems have not been readily available to a large group of
- marine scientists who would like to perform investigations that
- require image analysis capabilities. At the same time, the
- availability and use of very powerful PCs has significantly
- increased. Recently, the processed GLORIA imagery has been made
- available on Compact Disks (CDROM) which can be accessed by PCs.
- These factors make a PC-based MIPS-like system highly desirable.
- The PC-MIPS system is an attempt to satisfy this need.
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- PC-MIPS is an integrated collection of programs which have
- been adapted to a PC environment. Most of these programs have
- been selected from the MIPS software system developed at the USGS
- Image Processing Facility in Flagstaff, Arizona. While internal
- program and data structures have been extensively modified, an
- attempt has been made to preserve the basic appearance to the
- experienced MIPS user.
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- PC-MIPS was developed using MS-DOS version 3.31 for the
- Compaq Deskpro. Microsoft's Fortran version 5.0 was chosen as
- the development language since about half of the MIPS system was
- written in Fortran (the other half being in the MAC assembler
- language).
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- The selection of a display mechanism has largely been based
- on the availability of existing PC-based software. During the
- early stages of the GLORIA CD-ROM project, an image display
- program (IMDISP) developed by NASA at the Jet Propulsion Lab was
- evaluated and found to be excellent for displaying GLORIA images
- on a PC. IMDISP supports all the major graphics standards (i.e.,
- CGA, EGA, VGA, and PGA). It provides an extensive set of
- commands and utilizes a very simple but robust set of file
- structures.
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- The hardware utilized for the development of PC-MIPS is a
- Compaq 386/20 Model 130 equipped with 2Mb ram, the 80387/20 math
- coprocessor and a VGA color monitor. This configuration provides
- processing speeds which average 26Kb per second. In other words,
- if you process an input image 1Mb in size and create a resultant
- output image of the same size, the processing time will usually
- be under 1.5 minutes.
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- Standard VGA provides a display of 16 colors and/or grey
- levels with a resolution of 640 by 480 pixels. A display of 64
- grey levels can be achieved using the Orchid ProDesigner PLUS VGA
- card with 512K on-board memory.
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- The hardware configuration which was used for development is
- recommended for use; however, PC-MIPS will run under MS-DOS on
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- any generic PC/AT class machine with VGA graphics, and a hard
- disk. The software itself occupies approximately 2.6Mb.
- Realistically, a hard disk of at least 40Mb should be used.
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- Following is a list of the programs currently available:
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- CMBIMG Combines from 2 - 4 input images to create a composite
- output image which can be displayed via IMDISP.
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- DERIV Generates the first differences in the horizontal,
- vertical, or diagonal direction.
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- EDGENH Uses a Laplacian transform to provide edge enhancement
- capabilities.
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- EXT_ROI Used to extract an irregularly shaped sub-image
- (defined in POLYGON.DAT) from up to 7 input images.
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- FLT8B Boxcar spatial filtering (powerful workhorse; high and
- low pass filtering; surface generation; interpolation
- for gaps; edge enhancement; etc.).
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- IMDISP JPL's image display program. Currently 18 commands
- are implemented. Among them are Profile, Stretch,
- Palette, Histogram, Browse, and Display with or
- without sub-sampling and/or zoom. Text may, also, be
- positioned on the display.
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- LIST Generates a printout (LIST.PRT) of DN values for an
- image. Sub-image areas may be specified.
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- MAPIMG Performs a user-specified mapping of 1 to 7 input
- files. An extremely robust program that generates an
- output image which is the result of a user-specified
- functional mapping applied to the input files.
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- MAPLN1 Enhances linear features using a semi-linear line
- detecting/mapping technique (useful for regular image
- data as well as Topo, Gravity, etc.).
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- MDGRAD Modified gradient method that instead of multiplying
- the constants together adds them because of the
- possibility of one of them being ZERO (linear feature
- enhancement/mapping technique; used on image and
- surface data such as TOPO).
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- MEDIAN Applies a 3 by 3 median (middle value) filter. Will
- help remove high frequency noise. MEDIAN is
- particularly suitable for data that has a skewed
- distribution. However, the value obtained for the
- median may not be representative if the individual
- items do not tend to cluster at the center of the
- distribution.
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- MIXBDS Will generate three output bands from the TM six bands
- by selecting the user-specified three optimum bands
- for each of vegetation, soils, and water. For example,
- vegetation pixels might have TM bands 2,4, and 5;
- soils pixels might have TM bands 1,4, and 5; while
- water pixels might have TM bands 1,2, and 3. This
- will allow the three output bands to be used for
- either color compositing or digital processing so that
- these three 'new' bands have the best combination for
- these three major cover types.
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- NUVU Creates oblique views of image data using a
- Topographic height file and/or image file. If only
- the image file is used, the DN value is interpreted as
- height.
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- OVRLAY Takes from 2 to 6 input files/images and generates one
- output file/image that indicates which of the input
- files have data in user specified ranges for the input
- files being used.
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- PCA Generates the linear combinations for Principal
- Component Analysis of two to seven files (the output
- of STATS may be used as input coefficients).
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- PICSTR This program allows the user to let the machine pick
- good stretch pairs for an image based on either min/
- max parameters or by giving a min/max percent of the
- image. Values outside these ranges are ignored when
- trying to pick DN values.
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- RADARS Uses digital elevation data as input (dma, dem, etc.)
- and outputs the elevation data with it's geometry
- converted to slant range mode. The user specifies the
- near range (nr) depression angle (used to determine nr
- to nadir distance) and the imaging system's height and
- pixel resolution. It assumes the radar scan direction
- is in the horizontal direction (i.e., the imaging
- system is on the left or right side of the image).
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- RATIO Generates up to three output images that are the
- result of dividing the up to four input images by each
- other.
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- ROI Used to define and extract an irregularly shaped sub-
- image from up to 7 input images. Requires VGA and
- serial MS compatible mouse.
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- ROTATE Rotates an image 90 degrees in the clockwise or
- counter-clockwise direction.
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- SALTP Does bit error or random noise removal (Salt and
- Pepper).
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- SCALE Changes the scale of an image in the line direction,
- sample direction, or both.
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- SHAD2 Does automatic shading correction on Sonar, Radar, or
- any other file.
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- SHADRF Computes reflectance for any sun elevation and one of
- four sun directions using Lommel-Seeliger Law.
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- STATS Computes the Mean, Standard Deviation, Variance,
- Covariance, and Correlation Coefficients between two
- to seven images. It will also create the eigen vector
- matrix that is required as input to PCA.
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- STEEP Uses surface data as input (dem, dma, gravity, etc.)
- and generates a thematic map (0's or 255's) of ridges
- or drainage patterns (i.e., maps linear features).
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- STENCL Uses two input files. The first file is 'stenciled'
- based on data of second file. Generates one output
- file.
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- STRTCH Performs contrast stretching on an image using up to
- 10 user-specified stretch intervals.
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- SUBIMG Allows the extraction and/or "flipping" (i.e.,
- reversing) of sub-images in the line and/or sample
- direction.
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- SUN Computes reflectance given any sun elevation and
- direction.
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- WTCMBO Generates the weighted sum of 1 to 4 input files. The
- weighting coefficients are specified by the user and
- must be real numbers. The DN values for the output
- file are computed as follows:
- OUT = C1*INPUT1 + C2*INPUT2 + C3*INPUT3 + C4*INPUT4 +
- C5
- Where C1, C2, C3, C4, and C5 are user-specified
- constants.
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- Installing PC-MIPS
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- PC-MIPS can be installed on any hard disk drive (e.g., C:,
- D:, E:,,,etc.). Once a drive is selected, the installer should
- create a root-level directory named \MIPS. Next, the two sub-
- directories \MIPS\BIN and \MIPS\AUX_FILE must be created. These
- directories are created using the DOS command MKDIR or MD. The
- executable programs of PC-MIPS are stored in the \MIPS\BIN
- directory. The \MIPS\AUX_FILE directory contains various
- auxiliary files used by PC-MIPS programs.
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- Two 1.2Mb floppy disks contain three programs which are used
- to load the \MIPS sub-directories. These programs are named
- AUX_LOAD.EXE, BIN_LD1.EXE, and BIN_LD2.EXE (they were created
- using the program PKSFX from PKWARE INC., 7032 Ardara Ave.,
- Glendale, WI 53209). The installer should first load the
- AUX_FILE sub-directory by typing A:AUX_LOAD \MIPS\AUX_FILE.
- Next, the BIN sub-directory is partially loaded by typing
- A:BIN_LD1 \MIPS\BIN. The installation is completed by inserting
- the second floppy disk and typing A:BIN_LD2 \MIPS\BIN. These
- steps can be performed automatically by executing the INSTALL.BAT
- files found on each floppy disk. They assume installation on
- hard disk drive C:.
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- Once the two floppy disks have been loaded, the AUTOEXEC.BAT
- file should be changed so that the display program IMDISP knows
- what display device is being used. This is done by setting the
- environmental variable IMDISP. For instance, if the hardware has
- standard VGA capabilities, the line SET IMDISP=VGA must be added
- to the AUTOEXEC.BAT file. A complete list of devices supported
- by IMDISP can be found in the file IMDISP.DOC.
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- PC-MIPS can now be executed by typing \MIPS\BIN\PC_MIPS. If
- \MIPS\BIN is added to the DOS PATH command in the AUTOEXEC.BAT
- file, the system can be run by simply typing PC_MIPS.
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- User Interface
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- Individual PC-MIPS programs can be executed directly or via
- a menu-driven interface. A menu-driven interface presents the
- user with a list of the PC-MIPS programs available for use and
- provides a mechanism for selecting and executing individual
- entries. Individual programs in the list may be selected by name
- or number. PC_MIPS, also, provides a gateway which allows
- execution of DOS commands without exiting the system. This
- gateway is entered by typing DOS at the user prompt. After the
- gateway is entered, the user returns to the menu by typing
- PC_MIPS in response to the DOS> prompt.
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- Image Data Structure
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- The PC-MIPS image data structure is a subset of JPL's PDS
- data structure (see IMDISP.DOC). This subset has the following
- restrictions:
- 1. Only 8 bit data is supported.
- 2. The image definition must be contained in a separate
- image label file.
- 3. Image header records are not supported.
- 4. Line prefix and suffix bytes are not supported.
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- A PC-MIPS image is composed of two files. The first is an
- image label file and the second is an image data file.
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- Image label files contain information describing the image
- such as the number of lines, the number of samples, and the
- location (path name) of the image data file. Records of the
- image label file contain keywords and values. The mandatory
- keywords are FILE_TYPE, IMAGE_LINES, LINE_SAMPLES, IMAGE_POINTER,
- and END. These are described as follows:
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- FILE_TYPE - Must have the value IMAGE.
- IMAGE_LINES - Gives the number of lines (i.e., rows) in the
- image.
- LINE_SAMPLES - Gives the number of samples (i.e., columns) per
- line.
- IMAGE_POINTER - Gives the path name of the image data file.
- END - Must be the last record of a label file.
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- If the PDS keyword LINE_PREFIX_BYTES is given, its value will be
- added to the LINE_SAMPLES value. The following image label file
- named SAMPLE defines an image of 460 lines and 407 samples:
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- FILE_TYPE = IMAGE
- IMAGE_LINES = 460
- LINE_SAMPLES = 407
- IMAGE_POINTER= \images\sample.img
- END
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- The image data file is binary (i.e., non-printable) and
- contains the DN values which comprise the image. This file MUST
- be IMAGE_LINES times LINE_SAMPLES bytes in size. It is simply a
- contiguous sequence of bytes (i.e., DN values) which represent
- the image stored in row (i.e., line) major order.
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- While running PC-MIPS programs, the user refers to an image
- using the image label file name. THIS FILE NAME SHOULD NOT HAVE
- A DOS EXTENSION (i.e., not contain a period). A PC-MIPS output
- image will be composed of the user-specified image label file
- name and an image data file whose name is the same but has .IMG
- as a DOS extension.
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- User Input
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- PC-MIPS has two types of user input. The first type is file
- names (input and/or output). The second type is parameters that
- control the computation.
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- File names are entered by the user at the FILES> prompt.
- The user responds by entering a list of output names, followed by
- an equal sign, followed by a list of input names. Individual
- elements (file names) in these lists are separated by commas.
- File names may not have extensions (i.e., may not contain a
- period) and full DOS path names may be used. For example,
- FILES>OUT1,OUT2=INPUT1,INPUT2,INPUT3 represents lists of two
- output files (OUT1 and OUT2) and three input files (INPUT1,
- INPUT2, and INPUT3). For programs that generate no output files,
- the user only enters the list of input files. If an input file
- does not exist, the user is informed and requested to reenter the
- FILES> line. If an output file already exists, the user is asked
- if this file should be over-written. Prior to the FILES> prompt
- the user is informed of the expected number of file names and the
- maximum number of samples per line that is permitted. All input
- files must be of the same size (i.e., contain the same number of
- lines and samples).
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- The input of program parameters is given by the user at the
- PARAM> prompt. Prior to issuing the PARAM> prompt, the program
- displays the valid parameter names, their default values
- (enclosed in brackets), and their meaning. Parameters are
- assigned values by entering their name, followed by the equal
- sign, followed by a value. Values may be numeric constants or
- character strings. Character strings must be enclosed in
- apostrophes. Some parameters are set by simply entering their
- name (i.e., without the equal sign followed by a value). An
- example would be the specification of which type of computation
- is desired. Commas are used to separate the setting of multiple
- parameters. For example, the valid parameters for the LIST
- program are SS, SL, ES, EL, LINC, SINC, PAGE, and HEAD. If the
- user entered the line SS=200, EL=200, PAGE, HEAD='1st 200'
- he would be requesting a single page listing of the first 200
- lines and samples with the title '1st 200'.
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- PC-MIPS Programs
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- CMBIMG
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- This program is used to create an output file composed of
- multiple images which can be viewed using the IMDISP program.
- CMBIMG prompts for the input/output file specifications in normal
- PC-MIPS form (i.e., OUTPUT=INPUT1,INPUT2,INPUT3,INPUT4). There
- may be from two to four input images and the size (number of
- lines and samples) of all input images MUST be equal.
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- The composite output image (i.e., file) is structured as
- shown below:
- ------ ------
- |INPUT1|INPUT2|
- OUTPUT= |------|------|
- |INPUT3|INPUT4|
- ------ ------
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- hint:
- An output file of more than four input images can be created by
- repeated use of CMBIMG.
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- Example:
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- CMBIMG 18-MAY-88 # of files
- bit types: 8 2 - 4 input
- max samples: 3000 1 output
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- File name where the processed results will be stored.
- (e.g., OUTPUT
- File name(s) that has (have) the input data to be processed.
- =INPUT1,INPUT2,INPUT3)
- ------ ------
- |INPUT1|INPUT2|
- OUTPUT= |------|------|
- |INPUT3|INPUT4|
- ------ ------
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- FILES> comb=sample,m1,m2
- FILES>
- Do you want to display comb (y/n)? n
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- DERIV
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- Program DERIV performs a derivative (or first difference)
- function on an image. The derivative can be in the horizontal,
- vertical, or diagonal direction as specified by the user. The
- equations used are:
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- horizontal - Y(i,j) = X(i,j) - X(i+1,j) + C
- vertical - Y(i,j) = X(i,j) - X(i,j+1) + C
- diagonal - Y(i,j) = X(i,j) - X(i+1,j+1) + C
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- where X is the input image, Y is the output image, and C is a
- user-specified constant.
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- The user enters the input/output file names at the FILES>
- prompt. The program then displays the four valid parameters and
- issues a PARAM> prompt. The desired direction is selected
- entering one of the three directional parameters HORZ, VERT, or
- DIAG. The fourth parameter IADB is provided as an add-back
- constant which defaults to 127 if not specified.
-
- Example:
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- DERIVE 12-JAN-85 # of files
- bit types: 8 1 input
- max samples: 3000 1 output
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- Filename where the processed results will be stored.
- (e.g., OUTPUT
- Filename that has the input data to be processed.
- =INPUT)
- FILES> hdrev=sample
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- Valid parameters are:
- HORZ:[] - Performs a horizontal derivative
- VERT:[] - Performs a vertical derivative
- DIAG:[] - Performs a diagonal derivative
- IADB:[127] - Addback constant
- (e.g., HORZ,IADB=127)
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- PARAM> horz, iadb=100
- FILES>
- Do you want to display hderv (y/n)? n
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- EDGENH
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- EDGENH uses a Laplace transform to perform edge enhancement
- on images. The transform matrix is as follows:
- 0 -1 0
- -1 4 -1
- 0 -1 0
- The user is prompted for input/output file names via the
- FILES> prompt. Next, the user is prompted to enter a value
- representing the fraction of the Laplace transform to be added.
- Each interior pixel Y(i,j) is calculated according to the formula
- Y(i,j)=X(i,j)+f*[4*X(i,j)-X(i-1,j)-X(i,j-1)-X(i+1,j)-X(i,j+1)]
- where X is the input image, Y is the output image and f is the
- user-specified fraction. Boundary pixels are unchanged.
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- Example:
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- EDGENH 18-JUNE-88 # of files
- bit types: 8 1 input
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- max samples: 3000 1 output
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- File name where the results are to be stored
- (e.g., OUTPUT
- File name where the input data is located
- = INPUT)
- FILES> edge = sample
- Enter fraction of Laplace transform to be added: 0.4
- FILES>
- Do you want to display edge (y/n)? n
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- EXT_ROI
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- This program extracts sub-images from up to 7 input images.
- The sub-image is specified by an ascii file named POLYGON.DAT
- which contains the polygon vertices which define the sub-image.
- The first record in this file contains the number of vertices.
- Subsequent records contain the vertices themselves. They are
- given as sample/row pairs. This file must be present in the
- working directory when the program is executed. Output and input
- file names are given by the user at the FILES> prompt.
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- IMDISP
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- Refer to IMDISP.DOC file for description.
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- LIST
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- This program will generate a printout of DN values. The
- user can select a window by specifying starting/ending line and
- sample numbers. Additionally, line and sample increments may be
- given. If a single-page printout is requested, the program
- automatically determines the line and sample increments which
- will achieve this result.
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- The name of the image to be listed is specified on the
- FILES> prompt line. The desired listing parameters are specified
- on the PARAM> prompt line. The parameters which may be specified
- are as follows:
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- SS:[1] - Starting sample number
- SL:[1] - Starting line number
- ES:[NS] - Ending sample number
- EL:[NL] - Ending line number
- SINC:[1] - Sample increment
- LINC:[1] - Line increment
- PAGE:[] - List total area on one page
- HEAD:[] - Label to be put on top of printout
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- Note that default values are indicated within the square
- brackets. As an example, SS=10, LINC=5, HEAD='SAMPLE LISTING'
-
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- would generate a listing of every fifth line and all samples
- after the first nine. The listing would be titled 'SAMPLE
- LISTING'.
-
- The output file which contains the listed DN values is
- named LIST.PRT. Sample numbers are given along the top of pages
- and line numbers are given down the first column of pages. Each
- page contains 50 lines and 25 samples. Multiple pages are
- generated until the entire specified area is represented.
-
- Example:
-
- LIST 9-AUG-84 # of files
- bit types: 8 1 input
- max samples: 8000 0 output
-
- File name that has the input data to be processed.
- FILES> sample
- Valid parameters are:
- SS:[1] -Starting sample
- SL:[1] -Starting line
- ES:[NS] -Ending sample (defaults to the number of samples in the
- input file)
- EL:[NL] -Ending line (defaults to the number of lines in the
- input file)
- LINC:[1] -Line increment
- SINC:[1] -Sample increment
- PAGE:[] -List total area on one page.
- HEAD:[] -Label to be put on top of listing.
-
- (e.g., LINC=1,SINC=1,PAGE, HEAD='LABEL')
-
- PARAM> ss=151, es=200, sl=201, el=300, sinc=2
- FILES>
-
-
- MAPIMG
-
- MAPIMG provides the ability to create an output image which
- is computed by a user-specified mapping of from 1 to 7 input
- images. The mapping is done on a pixel-by-pixel basis.
-
- The user first specifies the output and input image file
- names in the normal PC-MIPS format (e.g. out=in1,in2,in3).
- Next, the user specifies the mapping by entering a mathematical
- expression which defines the desired mapping.
- This expression may contain numeric constants, arithmetic
- operators (+, -, /, *, and **), input image identifiers F1 to
- F7 which refer to the corresponding input images, and intrinsic
- functions. Parenthesis may be used to control the order of
- evaluation.
-
- The intrinsic functions supported are as follows:
-
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- Function Returns
- -------- -------
- abs() Absolute value
- sqrt() Square root
- log() Base 10 logarithm
- ten() Power of 10
- int() Integer truncation
- sin() Trigonometric sine
- cos() '' cosine
- max() Maximum pixel value
- min() Minimum pixel value
- rand() Pseudo-random value in the range 0.0 to 1.0
-
- All functions take a mathematical expression as an argument.
- This argument is evaluated prior to evaluating the function. For
- the max(), min(), and mean() functions, the evaluated argument is
- considered an integer which represents the number of input images
- to be considered. The sin() and cos() functions assume their
- argument to represent degrees. The rand() function assumes its
- argument to be a non-zero seed (or starting value) to be used in
- generating the random numbers.
-
- Example:
-
- MAPIMG 10-MAY-88 # of files
- bit types: 8 1 - 7 input
- max samples: 3000 1 output
-
- File name where the processed results will be stored.
- (e.g., OUTPUT
- File name(s) that has (have) the input data to be processed.
- =INPUT1,INPUT2,INPUT3)
- FILES> map1 = sample, m1, m2
- Enter mapping as a function of the input files F1 - F7
- (i.e. 0.33*(F1+F2+F3) or (F1+F2)/F3+127 )
- MAPPING> (f1 + 0.5*(max(3) - min(3)) + f2 + f3)/3
- FILES>
- Do you want to display map1 (y/n)? n
-
-
- MAPLN1
-
- MAPLN1 enhances linear features using a semi-linear line
- detecting/mapping technique. The semi-linear technique is one
- proposed by G. J. Vanderbrug (1975) and is a compromise between
- linear and nonlinear detectors. It makes separate comparisons to
- the left and to the right so it does not respond to edges but
- will respond to isolated noise. For more information see Bureau
- of Mines report on automatic linear feature mapping by Chavez
- (1983).
-
- The only user input is the input/output file names at the
- FILES> prompt.
-
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- Example:
-
- MAPLN1 24-JAN-85 # of files
- bit types: 8 1 input
- max samples: 3000 1 output
-
- File name where the processed results will be stored.
- (e.g., OUTPUT
- File name that has the input data to be processed.
- =INPUT)
- FILES> linout = sample
- FILES>
- Do you want to display linout (y/n)? n
-
-
- MDGRAD
-
- This program uses a modified gradient method for linear
- feature enhancement/mapping, but instead of multiplying the
- constants A, B, C, and D together they are added. The reason for
- this is that if only one of them is zero, no information is seen
- and the computation is faster.
-
- The formulas used are:
-
- A = |X(i+2,j+1)-X(i+3,j+2)| + |X(i+2,j+2)-X(i+3,j+1)|
- B = |X(i+1, j )-X(i+4,j+3)| + |X(i+1,j+3)-X(i+4, j )|
- C = |X(i+2, j )-X(i+3,j+3)| + |X(i+1,j+2)-X(i+4,j+1)|
- D = |X(i+3, j )-X(i+2,j+3)| + |X(i+1,j+1)-X(i+4,j+2)|
- Y(i,j) = A + B + C + D
- where X is the input image and Y is the output image.
-
- The only user input is the input/output file names at the
- FILES> prompt.
-
- Example:
-
- MDGRAD 21-AUG-84 # of files
- bit types: 8 1 input
- max samples: 3000 1 output
- File name where the processed results will be stored.
- (e.g., OUTPUT
- File name that has the input data to be processed.
- =INPUT)
- FILES> mdout = sample
- FILES>
- Do you want to display mdout (y/n)? n
-
-
- MEDIAN
-
- This program applies a 3 x 3 median filter to an image. It
- will smooth the data in a slightly different manner than that
- done by a simple average. The median is equal to the middle item
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- in a distribution which has been arranged by increasing value.
- Therefore the median location is equal to the pixel in the exact
- center and its DN value is assigned to the output pixel.
-
- Output and input file names are specified on the FILES>
- prompt line. There are no other program parameters to be
- entered.
-
- Example:
-
- MEDIAN 31-MAY-85 # of files
- bit types: 8 1 input
- max samples: 3000 1 output
-
- File name where the results are to be stored
- (e.g., OUTPUT
- File name where the input data is located
- = INPUT)
- FILES> m1=sample
- FILES>
- Do you want to display m1 (y/n)? n
-
-
- OVRLAY
-
- OVRLAY takes from 2 to 6 input images and generates one
- output image that indicates which of the input images have data
- in user specified ranges for the input images being used.
-
- This program can be used as part of an IMAGE or GIS
- processing system. In the GIS mode it can be used to overlay and
- merge various data sets together and in the IMAGE processing mode
- as a quick parallelepiped classifier. Currently there is a limit
- of six input files, but more can be processed by executing the
- program twice on two different groups of input files and then
- executing it a third time using the results of the first two
- groups as input. But this will be good ONLY to map where the
- data is in given ranges for ALL the input files used. The range
- of the third image results will be 0 to 3, where 3 indicates
- where the data is in the given ranges for all the files used.
- The program uses the MIN and MAX values for each input file
- supplied by the user to create a look-up table (ITBLA) indexed by
- the DN values of the input data. The values assigned to ITBLA
- are either 1 or 2 (1 implies DN value outside range and 2 implies
- DN value inside MIN-MAX range). This is like stretching all data
- outside the given range to 1 and inside the range to 2.
-
- The values (1 or 2) in this table (ITBLA) are then used to
- index into a second table (ITBLB) which has the correct sum or DN
- value for the given input file ranges. The values in the second
- table (ITBLB) are computed as if the input files were summed
- after they were given the values of 0 and 1,2,4,8,16, or 32
- according to the data being outside (0) or inside (FILE1=1,
- FILE2=2, FILE3=4, FILE4=8, FILE5=16, and FILE6=32) the specified
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- ranges. The data range of the output image will be from zero to
- (2**NFILES-1) where NFILES = number of input files used (2 to 6).
-
- In the case of four input files, the following table (where
- YES indicates value of given input file is in specified range)
- gives the value of the output file for possible combinations of
- input values:
-
- INPUT INPUT INPUT INPUT OUTPUT
- FILE1 FILE2 FILE3 FILE4 DN
- ----- ----- ----- ----- ------
- NO NO NO NO 0
- YES NO NO NO 1
- NO YES NO NO 2
- YES YES NO NO 3
- NO NO YES NO 4
- YES NO YES NO 5
- NO YES YES NO 6
- YES YES YES NO 7
- NO NO NO YES 8
- YES NO NO YES 9
- NO YES NO YES 10
- YES YES NO YES 11
- NO NO YES YES 12
- YES NO YES YES 13
- NO YES YES YES 14
- YES YES YES YES 15
-
- These values may be summarized as follows:
- 0 = All 4 files NO
- 1,2,4,8 = Only 1 file YES
- 3,5,6,9,10,12 = 2 files YES
- 7,11,13,14 = 3 files YES
- 15 = All 4 files YES
-
- Example:
-
- OVRLAY 3-MAY-84 # of files
- bit types: 8 2 - 6 input
- max samples: 3000 1 output
-
- File name where the processed results will be stored.
- (e.g., OUTPUT
- File names that have the input data to be processed.
- =INPUT1,INPUT2,INPUT3)
- FILES> overlay = sample, bathy, dpth
-
- Valid parameters are:
- MIN* = Minimum value for FILE(1-6)
- MAX* = Maximum value for FILE(1-6)
- * .. Replace with the file number.
- There are no default values.
- Values for MIN* and MAX* must be between 0 and 255.
- (e.g., MIN1=5,MAX1=70,MIN2=22,MAX2=33,MIN3=0,MAX3=96)
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- PARAM> min1=3,max1=240, min2=5,max2=170, min3=10,max3=210
- FILES>
- Do you want to display overlay (y/n)? n
-
-
- RATIO
-
- This program is used to generate output images which are
- ratios of input images. Up to four input images and three output
- images may be specified.
-
- The names of the output and input images are specified on
- the FILES> prompt line. The program then requests ratio
- parameters on the PARAMS> prompt line. The parameters which may
- be specified are as follows:
-
- R1 - A two digit number specifying how the first output
- image is to be calculated. The first digit gives the
- number of the input file which is to be used as the
- numerator. The second digit gives the number of the
- input file which is to be used as the denominator. For
- example R1=13, specifies that the first output image is
- the ratio of the first and third input images.
- R2 - Same as R1, but for the second output image.
- R3 - Same as R1, but for the third output image.
- FACT - A value which is to be used as a multiplication factor.
- The default value is 1.
-
- Example:
-
- RATIO 28-SEP-83 # of files
- bit types: 8 2 - 4 input
- max samples: 3000 1 - 3 output
- File names where the processed results will be stored (1-3
- images).
- (e.g., OUTPUT
- File names that have the input data to be processed (2-4 images).
- = INPUT1,INPUT2)
- FILES> band17,band24=band1,band2,band4,band7
-
- Valid parameters are:
- R1:[] -First ratio
- R2:[] -Second ratio
- R3:[] -Third ratio
- FACT:[1.0]-Ratio multiplying factor
- (e.g.,R1=12,R2=13,FACT=1.2)
- R1=12 means that the 1'st ratio will be input file 1 divided by
- file 2
- R2=13 means that the 2'nd ratio will be input file 1 divided by
- file 3
- R3=23 means that the 3'rd ratio will be input file 2 divided by
- file 3
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- PARAM> r1=14, r2=23
- FILES>
- Do you want to display band17 (y/n)? n
-
-
- ROI
-
- This program requires VGA graphics capability and a serial
- MS-compatible mouse. It allows the user to delineate a sub-image
- which is extracted from up to 7 input images. The sub-image is
- determined by entering polygon vertices using a mouse.
-
- At the FILES> prompt the user enters output and input file
- names. The first input file is displayed up to a maximum of 480
- lines and 640 samples. Next, the user positions the graphics
- cursor (an arrow) to an initial vertex and "clicks" on that point
- by pressing the leftmost mouse button. That point is illuminated
- and the user moves to the second vertex and "clicks" on it using
- the same button. A line is drawn connecting the two points. The
- remaining vertices, up to the last, are specified in the same
- manner. When the cursor has been positioned on the last vertex,
- the polygon is closed by "clicking" with the second mouse button.
-
- After the polygon has been entered, the program creates the
- specified sub-image from each of the input files and creates an
- ascii file named POLYGON.DAT which contains the polygon vertices
- in a format acceptable to EXT_ROI which can be executed if sub-
- images from additional files are desired.
-
-
- ROTATE
-
- This program rotates an image 90 degrees (i.e., interchanges
- lines and samples) in the clockwise or counter-clockwise
- direction. The user specifies output and input file names on the
- FILES> prompt line. The program, then, requests the direction of
- rotation. Entering 0 (zero) indicates clockwise and 1 (one)
- indicates counter-clockwise.
-
- If the input image is small enough to reside in the
- available computer memory, the execution is very fast. For
- larger images, each pixel must be accessed individually and the
- execution time is quite slow. If this situation exists, a
- warning is given.
-
- Example:
-
- ROTATE 18-OCT-88 # of files
- bit types: 8 1 input
- max samples: 3000 1 output
-
- File name where the results are to be stored
- (e.g., OUTPUT
- File name where the input data is located
-
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- = INPUT)
- FILES> r1=m1
- Enter 0 for clockwise or 1 for counter-clockwise: 0
- FILES>
- Do you want to display r1 (y/n)? n
-
-
- SALTP
-
- This program is used to remove bit errors from images. The
- removal is based on a DN tolerance value which may be specified
- by the user or determined automatically based on the image
- histogram.
-
- A 3-line by 5-sample box is moved from left to right and
- from top to bottom through the input image to remove bad pixels
- from the image. This box is illustrated below:
- ---- ---- ---- ---- ----
- | U1 | U2 | U3 | U4 | U5 |
- ---- ---- ---- ---- ----
- | M1 | M2 | M3 | M4 | M5 |
- ---- ---- ---- ---- ----
- | L1 | L2 | L3 | L4 | L5 |
- ---- ---- ---- ---- ----
- Each time the box is moved, the pixel element in the middle (M3)
- of the box is compared with averages of other pixels inside the
- box to determine if the pixel needs to be replaced. This is done
- in two steps. Step 1 finds the average of the two points at the
- upper left corner of the box (U1 and U2) and the average of the
- two points at the lower right hand corner of the box (L4 and L5).
- If the difference of the two averages is greater than four times
- the tolerance limit then the box is currently over an edge in the
- image. If the edge test succeeds (box is over an edge) then the
- pixel in the middle cannot be corrected. If the edge test fails
- then step 2 is performed. Step 2 finds the average of the line
- above (U1-U5) and the line below (L1-L5) the line containing the
- pixel to be corrected. If the difference of the point in the
- middle and the average is greater than the acceptable tolerance
- then the point is considered bad data and is replaced with the
- average of the box.
-
- Example:
-
- SALTP 21-DEC-84 # of files
- bit types: 8 1 input
- max samples: 3000 1 output
-
- File name where the processed results will be stored.
- (e.g., OUTPUT
- File name that has the input data to be processed.
- =INPUT)
- FILES> cleaned = sample
-
- Valid parameters are:
-
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- TOL:[] - Integer DN tolerance value to be used to identify
- pixels that have a bit error. If not specified,
- TOL is calculated based on the histogram.
- PARAM> tol = 11
- TOLERANCE= 11 Percentage of pixels changed = 25.8
- FILES>
- Do you want to display cleaned (y/n)? n
-
-
- SHAD2
-
- SHAD2 computes the average of each sample position using
- every other line. The computed averages are then normalized by
- either the average value of all the averages or by a user
- supplied DN value (e.g., NORM). It can be used to correct for
- shading problems that exist in the horizontal direction (e.g., on
- sonar or radar data).
-
- SHAD2 uses the normalized average values as shading
- coefficients for image shading corrections. The user specifies
- values of TOL1 and TOL2 which are used to compute the average
- values using only data greater than or equal to TOL1 and less
- than or equal to TOL2. It passes through the input data twice,
- once to compute the correction coefficients and the second time
- to apply them. The user may specify a beginning sample number
- (e.g., ISS) for the computation.
-
- The user-specified keywords are as follows:
-
- TOL1:[0] - Lower DN limit tolerance to be used to compute
- averages.
- TOL2:[maxdn] - High DN limit tolerance to be to compute averages.
- ISS:[1] - Starting sample user wants to start processing the
- input data. Output lines will still contain all
- samples.
- NORM:[ave] - DN values to be used to normalize all the
- averages. Default is the average of all the
- averages.
-
- Example:
-
- SHAD2 27-APR-84 # of files
- bit types: 8 1 input
- max samples: 3000 1 output
-
- File name where the processed results will be stored.
- (e.g., OUTPUT
- File name that has input data to be processed.
- =INPUT)
- FILES> shaded = sample
-
- Valid parameters are:
- TOL1:[0] - Lower DN tolerance to be used to compute averages.
- TOL2:[maxdn] - High DN tolerance to use to compute averages.
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- ISS:[1] - Starting sample to start processing.
- Output lines will still contain all samples.
- NORM:[ave] - DN value to be used to normalize all the averages.
- Default is average of averages.
- (e.g., TOL1=1,TOL2=250,ISS=17,NORM=100)
-
- PARAM> tol1=5, tol2=250, norm=100
- FILES>
- Do you want to display shaded (y/n)? n
-
-
- STRTCH
-
- The STRTCH program performs contrast stretching on images.
- The user can specify up to ten stretch intervals. A stretch
- interval is specified by four values. These four values are
- given in terms of DN values. They are IN_LOW, IN_HIGH, OUT_1,
- and OUT_2. IN_LOW and IN_HIGH represent an input interval.
- OUT_1 and OUT_2 represent the corresponding output interval.
-
- Input DN values are assigned to values in the output
- interval based on their position within the input interval. If
- IN_LOW is equal to IN_HIGH, input DN values of IN_LOW are
- assigned the value of OUT_1. IN_HIGH cannot be less than IN_LOW.
- Input DN values not within any of the specified input intervals
- are unchanged.
-
- If OUT_1 is equal to OUT_2, all DN values in the input
- interval are reassigned a value of OUT_1. If OUT_2 is less
- than OUT_1, an 'inverse' stretch is performed (i.e., increasing
- input DN values are reassigned to decreasing output DN values).
- Note:
- STRTCH differs from the MIPS STRETC program which uses
- stretch 'pairs' instead of stretch 'intervals' to specify the
- stretch operation.
-
- Example:
-
- STRETC 09-NOV-88 # of files
- bit types: 8 1 input
- max samples: 3000 1 output
-
- File name where the processed results will be stored.
- (e.g., OUTPUT.EXT
- File name that has the input data to be processed.
- =INPUT.EXT)
- FILES> result = image
- Enter number of stretch intervals: 4
- Enter IN_LOW, IN_HIGH, OUT_1, OUT_2 for interval 1:
- 0, 15, 0, 0
- Enter IN_LOW, IN_HIGH, OUT_1, OUT_2 for interval 2:
- 16, 71, 0, 127
- Enter IN_LOW, IN_HIGH, OUT_1, OUT_2 for interval 3:
- 72, 127, 128, 255
-
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- Enter IN_LOW, IN_HIGH, OUT_1, OUT_2 for interval 4:
- 128, 255, 255, 255
- FILES>
- Do you want to display result (y/n)? n
-
-
- SUBIMG
-
- The sub-image program is used to extract a user-specified
- sub-image. This program is similar to the MIPS DK2DK program.
- Additionally, the output image may be 'flipped' (or 'reversed')
- in the line and/or sample directions.
-
- The user is prompted for an input file name. After the
- input file name is specified, the number of lines and samples in
- the input file are displayed and the user is prompted for
- starting/ending line and sample numbers. The output file is
- 'flipped' by specifying an ending value less than the starting
- value. Finally, the user is prompted for an output file name.
-
- Example:
-
- SUBIMG (10/88) allows the extraction and/or "flipping" of sub-
- images. The dimensions of the sub-image are entered by the user.
- "flipping" is accomplished by indicating starting values greater
- than ending values.
-
- Enter input file name: study
- study contains 1112 lines and 984 samples
- Enter starting and ending line numbers: 1, 420
- Enter starting and ending sample numbers: 981, 400
- Enter output file name: sub_stdy
-
- Enter input file name:
-
-
- WTCMBO
-
- This program is used to generate an output image which is
- the weighted sum (i.e., a linear combination) of up to four input
- images. The output is calculated using the following formula:
- Y = C1*X1 + C2*X2 + C3*X3 + C4*X4 +C5
- where
- Y is the output image,
- C1-C5 are user-specified constants, and
- X1-X4 are user-specified input images.
- The computation is done using 16-bit arithmetic.
-
- Example:
-
- WTCMBO 04-JUN-84 # of files
- bit types: 8 1 - 4 input
- max samples: 3000 1 output
-
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- File name where the processed results will be stored.
- (e.g., OUTPUT
- File name(s) that has (have) the input data to be processed.
- =INPUT1,INPUT2,INPUT3)
- FILES> sum = sample, shade
- Valid parameters are:
- CON1:[.25] - Weighting coefficient for input file 1.
- CON2:[.25] - Weighting coefficient for input file 2.
- CON3:[.25] - Weighting coefficient for input file 3.
- CON4:[.25] - Weighting coefficient for input file 4.
- CON5:[0] - Add-back constant for output file. Used to center
- the results in 8-bit positive range.
- (e.g., CON1=1.0,CON2=-1.0,CON3=.5,CON5=100)
-
- PARAM> con1=0.75, con2=1.25, con5 = -127
- FILES>
- Do you want to display sum (y/n)? n
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