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Frequently Asked Questions (FAQS);faqs.320 There are 2 types of files, the image itself and the related Sequence file that holds the processing, measurements and analysis that the user defines. Automated sequences are set up in Regions Of Interest (ROI) represented by movable, sizable boxes atop the image. Inside a ROI, the program can find the distance between two edges, the area of a shape, the thickness of a wall, etc. Image Analyst finds the center, edge and other positions automatically. The application also provides tools so that the user can work interactively to find the edge of object. It also supports histograms and a color look-up table (CLUT) tool. Automatix, Inc. 775 Middlesex Turnpike Billerica, MA 01821 508-667-7900 IPLab ----- Signal Analytics Corp. 374 Maple Ave. E Vienna, VA 22180 703-281-3277 FAX 703-281-2509 "Menu-driven image processing software that supports 24-bit color or pseudocolor/grayscale image display and manipulation." MAP II ------ Among the Mac GIS systems, MAP II distributed by John Wiley has integrated image analysis. IMAGE ----- from Stanford : Try anonymous ftp from sumex-aim.stanford.edu It has pd source for image v2, and ready to run code for a mac under image v3. Windows/DOS PC-based tools ========================== CCD --- Richard Berry's CCD imaging book for Willamon-Bell contains (optional?) disks with image manipulating software. Source code is included. ERDAS ----- "ERDAS will do all of the things you want: rectification, classification, transformations (canned & user-defined), overlays, filters, contrast enhancement, etc. ... I was using it on my thesis & then changed the topic a bit & that work became secondary." ERDAS, Inc. 2801 Buford Highway Suite 300 Atlanta, GA 30329 404-248-9000 FAX 404-248-9400 RSVGA ----- "I have been getting up to speed on a program called RSVGA available from Eidetic Digital Image Ltd. in British Columbia. Its for IBM PC's or clones, cheap (about $400) and does all the stuff Erdas does but is not as fast or as powerful, though I have had only limited experience with Erdas. I have used RSVGA with 6 of 7 Landsat bands and it is a good starter program except for the obtuse manual" IMAGINE-32 ---------- It's a 32 bit package [I suppose for PCs] called "Imagine32" or "Image32" The program does a modest amount of image processing --add, subtract, multiply, divide, display, and plot an x or y cut across the image. It can also display a number of images simultaneously. The company is CompuScope, in Santa Barbara, CA. PC Vista -------- It was announced in the 1989 August edition of PASP. It is known to be available from Mike Richmond, whose email addresses have been richmond@bllac.berkeley.edu richmond@bkyast.berkeley.edu and his s-mail address is: Michael Richmond,Astronomy Department, Campbell Hall, Berkeley, CA 94720 The latest version of PC-Vista, version 1.7, includes not only the source code and help files, but also a complete set of executable programs and a number of sample FITS images. If you do wish to use the source code, you will need Microsoft C, version 5.0 or later; other compilers may work, but will require substantial modifications. To receive the documentation and nine double-density (360K) floppies (or three quad-density 3-1/2 inch floppies (1.44M) with everything on them, just send a request for PC-Vista, together with your name and a US-Mail address, to Office of Technology Licensing 2150 Shattuck Ave., Suite 510 Berkeley, Ca. 94704 Include a check (Traveller's Checks are fine) or purchase order for $150.00 in U.S. dollars, if your address is inside the continental U.S., or $165.00 otherwise, made out to Regents of the University of California to cover duplication and mailing costs. SOFTWARE TOOLS -------------- It's a set of software "tools" put out by Canyon State Systems and Software. They are not free, but rather cheap at about $30 I heard. It will handle most all of the formats used by frame grabber software. MIRAGE ------ It's image processing software written by Jim Gunn at the Astrophysics Dept at Princeton. It will run on a PC among other platforms. It is a Forth based system - i.e. a Forth language with many image processing displaying functions built in. DATA TRANSLATION SOURCE BOOK ---------------------------- The Data Translation company in Massachusetts publishes a free book containing vendors of data analysis hardware and software which is compatible with Data Translation and other frame grabbers. Surely you can find much more PC-related stuff in it. MAXEN386 -------- A couple of Canadians have written a program named MAXEN386 which does maximum entropy image deconvolution. Their company is named Digital Signal Processing Software, or something like that, and the software is mentioned in an article in Astronomy Magazine, either Jan or Feb 92 (an article on CCD's vs film). JANDEL SCIENTIFIC (JAVA) ------------------------ Another software package (JAVA) is put out by Jandel Scientific. Jandel Scientific, 65 Koch Road, Corte Madera, CA 94925, (415) 924-8640, (800) 874-1888. Microbrian ---------- Runs on an MS dos platform and uses a 32 bit graphics card (Vista), or an about to be released version will support a number of super VGA cards. Its a full blown remote sensed data processing system.. It is menu driven (character based screen), but is does not use a windowed user interface. Its is hardware protected with a dongle. Mbrian = micro Barrier reef Image Anaysis System. It was developed by CSIRO (Commonwealth Scientific & Industrial Organization) and is marketed/ supported by: MPA Australia (51 Lusher Road, Croydon, Victoria tel + 61 3 724 4488 fax +61 3 724 4455) There are educational and commercial prices, but be prepared to set aside $A10k for the first educational licence. Subsequent ones come cheaper (they need to!) It has installed sites worldwide. It is widely used at ANU. MicroImage ---------- The remote sensing lab here at Dartmouth currently uses Terra-Mar's MicroImage, on 486 PCs with some fancy display hardware. Terra-Mar Resource Information Services, Inc. 1937 Landings Drive Mountain View, CA 94043 415-964-6900 FAX 415-964-5430 Unix-based tools ---------------- IRAF (Image Reduction and Analysis Facility) -------------------------------------------- Developed in the National Optical Astronomy Observatory, Kitt Peak AZ It is free, you can ftp it from noao.edu and complement it with STSDAS from stsci.edu. Email to iraf@noao.edu for more details. Apparently this is one of the _de facto_ standards in the astronomical image community. They issue a newsletter also. They seem to support very well their users. Works with VMS also last I heard, and practically has its own shell on top of the VMS/Unix shells. It's suggested that you get a copy of saoimage for display under X windows. Very flexible/extendable -- tons (literally 3 linear feet) of documentation for the general user, skilled user, and programmer. ALV --- A Sun-specific image toolkit. Version 2.0.6 posted to comp.sources.sun on 11dec89. Also available via email to alv-users-request@cs.bris.ac.uk. AIPS ---- contact aipsmail@nrao.edu -- astronomical image processing system of the national radio astronomy observatory, Charlottesville, VA -- software distributed by 9 track tape last time I ordered it -- I did not find this package very useful -- tons of dense documentation -- very old code -- I heard in one of our astronomy laboratories the package may be rewritten completely in the near future -- major funding available. LABOimage 3.1 ------------- (version 4.0 soon for X11) It's written in C, and currently runs on Sun 3/xxx, Sun 4/xxx (OS3.5, 4.0 and 4.0.3) under SunView. The expert system for image segmentation is written in Allegro Common Lisp. It was used on the following domains: computer science (image analysis), medicine, biology, physics. It is distributed free of charge (source code). Available via anonymous FTP at ads.com (128.229.30.16), in pub/VISION-LIST-ARCHIVE/SHAREWARE/LaboImage_3.1.tar.Z Contact: Prof. Thierry Pun, Computer Vision Group Computing Science Center, U-Geneva 12, rue du Lac, CH-1207 Geneva SWITZERLAND Phone : +41(22) 787 65 82; fax: +41(22) 735 39 05 E-mail: pun@cui.unige.ch or pun@cgeuge51.bitnet Figaro ------ It was originally made for VMS, and can be obtained from Keith Shortridge in Australia (ks@aaoepp.aao.gov.au) and for Unix from Sam Southard at Caltech (sns@deimos.caltech.edu). It's about 110Mbytes on a Sun. KHOROS ------ Moved to the Scientific Visualization category below Vista ----- The "real thing" is available via anonymous ftp from lowell.edu. Email to vista@lowell.edu for more details. Total size less than 20Mbytes. DISIMP ------ (Device Independent Software for Image Processing) is a powerful system providing both user friendliness and high functionality in interactive times. Feature Description DISIMP incorporates a rich library of image processing utilities and spatial data options. All functions can be easily accessed via the DISIMP executive. This menu is modular in design and groups image processes by their function. Such a logical structure means that complicated processes are simply a progression through a series of modules. Processes include image rectification, classification (unsupervised and supervised), intensity transformations, three dimensional display and Principal Component Analysis. DISIMP also supports the more simple and effective enhancement techniques of filtering, band subtraction and ratioing. Host Configuration Requirements Running on UNIX workstations, DISIMP is capable of processing the more computational intensive techniques in interactive processing times. DISIMP is available in both Runtime and Programmer's environments. Using the Programmers environment, utilities can be developed for specific applications programs. Graphics are governed by an icon-based Display Panel which allows quick enhancments of a displayed image. Manipulations of Look Up Tables, colour stretches, changes to histograms, zooming and panning can be interactively driven through this control. A range of geographic projections enables DISIMP to integrate data of image, graphic and textual types. Images can be rectified by a number of coordinate systems, providing the true geographic knowledge essential for ground truthing. Overlays of grids, text and vector data can be added to further enhance referenced imagery. The system is a flexible package allowing users of various skill levels to determine their own working environment, including the amount of help required. DISIMP comes fully configured with no optional extras. The purchase price includes all functionality required for professional processing of remote sensed data. For further information, please contact: The Business Manager, CLOUGH Engineering Group Systems Division, 627 Chapel Street, South Yarra, Australia 3141. Telephone: +61 3 825 5555 Fax: +61 3 826 6463 Global Imaging Software ----------------------- "We use Global Imaging Software to process AVHRR data, from the dish to the final display. Select a chunk of five band data from a pass, automatic navigation, calibrate it to Albedo and Temp, convert that to byte, register it to predesigned window, all relatively automatically and carefree. It has no classification routines to speak of, but it isn't that difficult to write your own with their programmer's module. Very small operation: one designs, one codes, one sells. Been around for a number of years, sold to Weather Service and Navy. Runs on HP9000 with HP-UX. Supports 24-bit display" HIPS ---- (Human Information Processing Laboratory's Image Processing System) Michael Landy co-wrote and sell a general-purpose package for image processing which has been used for basically all the usual image processing applications (robotics, medical, satellite, engineering, oil exploration, etc.). It is called HIPS, and deals with sequences of multiband images in the same way it deals with single images. It has been growing since we first wrote it, both by additions from us as well as a huge user-contributed library. Feature description HIPS is a set of image processing modules which together provide a powerful suite of tools for those interested in research, system development and teaching. It handles sequences of images (movies) in precisely the same manner as single frames. Programs and subroutines have been developed for simple image transformations, filtering, convolution, Fourier and other transform processing, edge detection and line drawing manipulation, digital image compression and transmission methods, noise generation, and image statistics computation. Over 150 such image transformation programs have been developed. As a result, almost any image processing task can be performed quickly and conveniently. Additionally, HIPS allows users to easily integrate their own custom routines. New users become effective using HIPS on their first day. HIPS features images that are self-documenting. Each image stored in the system contains a history of the transformations that have been applied to that image. HIPS includes a small set of subroutines which primarily deals with a standardized image sequence header, and a large library of image transformation tools in the form of UNIX ``filters''. It comes complete with source code, on-line manual pages, and on-line documentation. Host Configuration Requirements Originally developed at New York University, HIPS now represents one of the most extensive and flexible vision and image processing environments currently available. It runs under the UNIX operating system. It is modular and flexible, provides automatic documentation of its actions, and is almost entirely independent of special equipment. HIPS is now in use on a variety of computers including Vax and Microvax, Sun, Apollo, Masscomp, NCR Tower, Iris, IBM AT, etc. For image display and input, drivers are supplied for the Grinnell and Adage (Ikonas) image processors, and the Sun-2, Sun-3, Sun- 4, and Sun-386i consoles. We also supply user-contributed drivers for a number of other framestores and windowing packages (Sun gfx, Sun console, Matrox VIP-1024, ITI IP-512, Lexidata, Macintosh II, X windowing system, and Iris). The Hipsaddon package includes an interface for the CRS-4000. It is a simple matter to interface HIPS with other frame- stores, and we can put interested users in touch with users who have interfaced HIPS with the Arlunya and Datacube Max- Video. HIPS can be easily adapted for other image display devices because 98% of HIPS is machine independent. Availability HIPS has proven itself a highly flexible system, both as an interactive research tool, and for more production- oriented tasks. It is both easy to use, and quickly adapted and extended to new uses. HIPS is supplied on magnetic tape in UNIX tar format (either reel- to-reel or Sun cartridge), and comes with source code, libraries, a library of convolu- tion masks, and on-line documentation and manual pages. Michael Landy SharpImage Software P.O. Box 373, Prince Street Station New York, NY 10012-0007 Voice: (212) 998-7857 Fax: (212) 995-4011 MIRA ---- Nothing known besides its name. Anyone to add here info? ========================================================================== 16. Image annotation software ----------------------------- a. Touchup runs in Sunview and is pretty good. It reads in rasterfiles, but even if your image isn't normally stored in rasterfile format you could use screendump to make it a rasterfile. b. Idraw (part of Stanford's InterViews distribution) can handle some image formats in addition to being a MacDraw like tool. I'm not sure exactly what they are. You can ftp the idraw's binary from interviews.stanford.edu. c. Tgif is another MacDraw like tool that can handle X11 bitmap (xbm) and X11 pixmap (xpm) formats. If the image you have is in formats other than xbm or xpm, you can get the pbmplus toolkit to convert things like gif or even some Macintosh formats to xpm. Tgif's sources are available in the pub directory on cs.ucla.edu (Version 2.12 of tgif at patchlevel 7 plus patch8 and patch9) d. Use the editimage facility of KHOROS (see below). This is just one utility in the overall system- you can essentially do all your image processing and macdraw-type graphics using this package. e. You might be able to get by with PBMPlus. pbmtext gives you text output bitmaps which can be overlaid on top of your image. f. 'ice' requires Sun hardware running OpenWindows 3.It's a PostScript-based graphical editor,and it's available for anonymous ftp from Internet host eo.soest.hawaii.edu (128.171.151.12). Requires Sun C++ 2.0 and two other locally developed packages, the LXT library (an Xlib-based toolkit) and a small C++ class library. All files (pub/ice.tar.Z, pub/lxt.tar.Z and pub/ldgoc++.tar.Z) are available in compressed tar format. pub/ice.tar.Z contains a README that gives installation instructions, as well as an extensive man page (ice.1). A statically-linked compressed executable pub/ice-sun4.Z for SPARC systems is also available for ftp. All software is the property of Columbia University and may not be redistributed without permission. ice means Image Composition Environment and it's an imaging tool that allows raster images to be combined with a wide variety of PostScript annotations in WYSIWYG fashion via X11 imaging routines and NeWS PostScript rasterizing. g. Use ImageMagick to annotate an image from your X server. Pick the position of your text with the cursor and choose your font and pen color from a pull-down menu. ImageMagick can read and write many of the more popular image formats. ImageMagick is available as export.lcs.mit.edu: contrib/ImageMagick.tar.Z or at your nearest X11 archive. ========================================================================== 17. Scientific visualization stuff ---------------------------------- X Data Slice (xds) ------------------- Bundled with the X11 distribution from MIT, in the contrib directory. Available at ftp.ncsa.uiuc.edu [141.142.20.50] (either as a source or binaries for various platforms). National Center for Supercomputing Applications (NCSA) Tool Suite ----------------------------------------------------------------- Platforms: Unix Workstations (DEC, IBM, SGI, Sun) Apple MacIntosh Cray supercomputers Availability: Now available. Source code in the public domain. FTP from ftp.ncsa.uiuc.edu. Contact: National Center for Supercomputing Applications Computing Applications Building 605 E. Springfield Ave. Champaign, IL 61820 Cost: Free (zero dollars). The suite includes tools for 2D image and 3D scene analysis and visualization. The code is actively maintained and updated. KHOROS ------ Available via anonymous ftp at pprg.eece.unm.edu (129.24.24.10). cd to /pub/khoros to see what is available. It is HUGE (> 100 MB), but good. Needs Unix and X11R4. Freely copied (NOT PD), complete with sources and docs. Very extensive and at its heart is visual programming. Khoros components include a visual programming language, code generators for extending the visual language and adding new application packages to the system, an interactive user interface editor, an interactive image display package, an extensive library of image and signal processing routines, and 2D/3D plotting packages. See comp.soft-sys.khoros on Usenet and the relative FAQ for more info.... Contact: The Khoros Group Room 110 EECE Dept. University of New Mexico Albuquerque, NM 87131 Email: khoros-request@chama.eece.unm.edu MacPhase -------- Analysis & Visualization Application for the Macintosh. Operates on 1D and 2D data arrays. Import/Export several different file formats. Several different plotting options such as gray scale, color raster, 3D Wire frame, 3D surface, contour, vector, line, and combinations. FFTs, filtering, and other math functions, color look up editor, array calculator, etc. Shareware, available via anonymous ftp from sumex-aim.stanford.edu in the info-mac/app directory. For other information contact Doug Norton (e-mail: 74017.461@@compuserve.com) IRIS Explorer ------------- It's an application creation system developed by Silicon Graphics that provides visualisation and analysis functionality for computational scientists, engineers and other scientists. The Explorer GUI allows users to build custom applications without having to write any, or a minimal amount of, traditonal code. Also, existing code can be easily integrated into the Explorer environment. Explorer currently is available now on SGI and Cray machines, but will become available on other platforms in time. [ Bundled with every new SGI machine, as far as I know] See comp.graphics.explorer for discussion of the package. There are also two FTP servers for related stuff, modules etc.: ftp.epcc.ed.ac.uk [129.215.56.29] swedishchef.lerc.nasa.gov [139.88.54.33] - mirror of the UK site apE --- Back in the 'old good days', you could get apE for nearly free. Now has gone commercial and the following vendor supplies it: TaraVisual Corporation 929 Harrison Avenue Columbus, Ohio 43215 Tel: 1-800-458-8731 and (614) 291-2912 Fax: (614) 291-2867 Cost: $895 (plus tax); runtime version with a site-license for a single user (at a time), no limit on the number of machines in a cluster. $895 includes support/maintenance and upgrades. Source code more. Additional user licenses $360. The name of the package has become apE III (TM). Khoros is very similar to apE on philosophy, as are AVS and Explorer. AVS --- See also: comp.graphics.avs Platforms: CONVEX, CRAY, DEC, Evans & Sutherland, HP, IBM, Kubota, Set Technologies, SGI, Stardent, SUN, Wavetracer Availability: AVS3 available on all the above: AVS4 currently available on SGI, SUN AVS4 will be available on: HP, IBM, Kubota, SGI, Stardent, SUN 6/1/92 Contact: Advanced Visual Systems Inc. for: CRAY, HP, IBM, SGI, Stardent, SUN CONVEX for CONVEX Advanced Visual Systems Inc. or CRAY for CRAY DEC for DEC Evans & Sutherland for Evans & Sutherland Advanced Visual Systems Inc. or IBM for IBM Kubota Pacific Inc. for Kubota Set Technologies for Set Technologies Wavetracer for Wavetracer WIT --- In a nutshell it's a package of the same genre as AVS,Explorer,etc. It seems more a image processing system than a generic SciVi system (IMHO) Major elements are: - a visual programming language, which automatically exploits the inherent parallelism - a ode generator which converts the graph to a standalone program Iconified libraries present a rich set of point, filter, io, transform, morphological, segmentation, and measurement operations. A flow library allows graphs to employ broadcast, merge, synchronization, conditional, and sequencing control strategies. Users can easily extend WIT by defining new C functions, data types, and servers to access specialized hardware. They are currently sending out free 3.5" demo disks suitable for Sun Sparcstation floppy drives to anyone interested in trying out the software (and they are thinking about putting a copy of the demo for FTP). Or you can try the Catalyst CDware program as trial software; Demo version on Sun CDware 4. WIT supports Sun3, Sun4, vxWorks by Wind River Systems, and Datacube (MaxVideo-20 hardware) platforms. Pricing: WIT for Sparc, one yr. free upgrades, 30 days technical support....................$5000 US Academic institutions: discounts available Contact: Logical Vision, Ltd. 6882 Rupert St. Vancouver, B.C., Canada V5S 2Z6 Tel: 604-435-2587, Fax: 604-299-8263 Terry Arden <poon@ee.ubc.ca> VIS-5D ------ A system for visually exploring the output of weather models and similar data sets. Platforms: SGI Power/VGX, Power/GTX and PI, Crimson and Indigo; IBM RS/6000 with GL graphics; Stardent GS-1000 and GS-2000 You can get it freely (thanks to NASA support) via anonymous ftp: ftp vis5d.ssec.wisc.edu (or ftp 144.92.108.66), then ftp> cd pub/vis5d ftp> ascii ftp> get README ftp> bye Read section 2 of the README file for full instructions on how to get and install VIS-5D. Contact: Bill Hibbard (whibbard@vms.macc.wisc.edu) Brian Paul (bpaul@vms.macc.wisc.edu) DATAexplorer (IBM) ------------------ Platforms : IBM Risc System 6000, IBM POWER Visualization Server (SIMD mesh 32 i860s, 40 MHz) Working on (announced) : SGI, HP, Sun Contact: Your local IBM Rep. For a trial package ask your rep to contact : David Kilgore Data Explorer Product Marketing YKTVMH(KILCORE), (708) 981-4510 Wavefront --------- Data Visualizer, Personal Visualizer, Advanced Visualizer. Platforms: SGI, SUN, IBM RS6000, HP, DEC Availability: Available on all the above platforms from Wavefront Technologies. Educational programs and site licenses are available. Contacts: Mike Wilson (mike@wti.com) Wavefront Technologies, Inc. 530 East Montecito Street Santa Barbara, CA 93103 805-962-8117 FAX: 805-963-0410 Wavefront Europe Guldenspoorstraat 21-23 B-9000 Gent, Belgium 32-91-25-45-55 FAX: 32-91-23-44-56 Wavefront Technologies Japan 17F Shinjuku-sumitomo Bldg 2-6-1 Nishi-shinjuku, Shunjuku-Ku Tokyo 168 Japan 81-3-3342-7330 FAX 81-3-3342-7353 PLOT3D and FAST from NASA Ames ------------------------------ These packages are distributed from COSMIC at least (for FAST ask Pat Elson <pelson@nas.nasa.gov> for distribution information). In general, these codes are for US citizens only :-( XGRAPH ------ On the contrib tape of X11R5. Its specialty is display of up to 64 data sets (2D). NCAR ---- National Center for Atmospheric Research [ Anyone to add more info? ] IDL/PV-WAVE ----------- "The IDL/PV-WAVE software package is what I currently use . I/O is very simple (a major plus!!) & most of my programming is very short & sweet. Numerous output formats are available. there are certainly some minuses & it does require "programming". I use the command line version, though the "point & click" version is available...I have some acquaintances who use it on the Mac (I think via Mac-X). Basically, there are a lot of built-in functions, though some manipulation is required. IDL/PV-WAVE is able to work with any type of imagery. IDL runs on a unix system" IDL/SIPS -------- A lot of people are using IDL with a package called SIPS. This was developed at the University of Colorado (Boulder) by some people working for Alex Goetz. You might try contacting them if you already have IDL or would be willing to buy it. It's a few thousand dollars (American) I expect for IDL and the other should be free. Those are the general purpose packages I've heard of, besides what TerraMar has. SIPS _was_ written for AVIRIS imagery. I'm not sure how general purpose it is. You would have to contact Goetz or one of his people and ask. I have another piece of software (PCW) that does PC and Walsh transformations with pseudocoloring and clustering and limited image modification (you can compute an image using selected components). I've used it on 70 megabyte AVIRIS images without problems, but for the best speed you need an external DSP card. It will work without it, but large images take quite a while (50-70 times as long) to process. That's a freebie if you want it.