From: eugene@amelia.nas.nasa.gov (Eugene N. Miya)
Subject: [l/m 10/15/1992] Shell	(1/4) c.g.v.FAQ
Followup-To: poster
Organization: NAS Program, NASA Ames Research Center, Moffett Field, CA
Date: Tue, 15 Dec 92 12:45:16 GMT
Reply-To: eugene@amelia.nas.nasa.gov (Eugene N. Miya)

#Disabled
Archive-name: comp.viz.faq

	"Feed me."  -- Audrey II, the Plant in "The Little Shop of Horrors."

		Contents
		========

		Intro
		-----
		What is visualization?
		----------------------
		Systems
		-------
		Issue/problems
		--------------
		Netiquette
		----------
		References
		----------
================================


The FAQ is dedicated to Harold "Doc" Edgerton (MIT).


Intro
-----

The quality of this FAQ is directly proportional to the information
mailed by participants (that's you) to the maintainer (me, Amelia).
You don't like it?  Blame the rest of the posters and readers.
I don't have 100% time to maintain this.  We are starting from scratch.
If an address or phone is out of date?  Blame the group.  I'm just a dumb
computer posting as I am told.

	[It's getting better, people are emailing contributions!]

The structure of this FAQ is currently a twice monthly post, with two
weekly outriggers pointing to the Long (this) version.  We will see how well
this works (empirical science).  The header, the body, etc. have all been
specially designed and tested.  In time, mitosis will occur on this file
and it will get spread over the course of a month.

You should not have to see this file all the time.  Don't bother saving it
unless you have a flakey net connection.   Grab the most recent revision
off the net.  The Subject: line is designed to fit within the 24-char limit
of most Killfile systems.  Learn about Killfiles.  If you have something
against FAQ files, the regular expression /.*FAQ$/ will Kill All My Children
and me.  Learn how to use news and how news works before complaining.
This post is like a lighthouse or a fog horn.  Learn how to use it.



What is visualization?
======================

"Visualization is the use of computer-generated media based
on data in the service of human insight/learning."

Analytic graphics
		--Carol Hunter, LLNL

Visualization: 
	The use of computer imagery to gain 
	insight into complex phenomena.

The purpose of visualization is insight, not virtual realities or numbers.
		--enm

The Maintainer gets a chance to pontificate here: [You can, too. Just ask.]

I learned from Jack Estes (UCSB) that observation has three recursive
phases and corresponding mathematical models:
	Detection
	Identification
	Measurement and Analysis (this latter being the recursion).
Any good system will support these (reducibly).  Researchers need the latter.
Artistes only use the first (Calder was an exception, but then he trained
as an aerodynamicist 8^).  We don't teach observation very well in schools
these days.  We assume you have picked it up via osmosis or are naturally
gifted.  It requires training and some talent.  It's especially bad in
computer science depts. because of the emphasis in theory.

It is Miya's assertation that ultimately visualization will converge
of technologies like those used in cartography (>2000 years old),
surveying, photogrammetry (aerial or terrestial), certain parts of ergonomics,
etc.  Why?  Because they are quantitative.  They use stereo in some instances
(far more important than most people realize).  USGS tours are available.

Maps have better information content than any image pervading our society.
The signal to noise ratio is greater (density).  Better than photos,
better than movies (ask yourself if you can always figure out the ending 8^).
I defy the presentation of an other consistent image with better
characteristics than a map.  Maps have excellent characteristics like
an easily measurable geometry, legends, symbolization (but like all imagery
they have limitations).  Consider all this the next time you look at your AAA
maps when you go on vacation.

What kinds of quantitative, numeric support are needed?  Every basic science
measurement:
enumeration (counting, math got started because of counting), distances,
areas, volumes, angles (planar and solid), extrema,
parametric and non-parametric statistics (means, median, modes,
deviations, ANOVA), histograms, intervals and error bounds, derivatives,
partials, integrals, etc.

ONLY the trained researcher (maybe you) will make the critical insights
needed for scientific discovery.  Not your programmer,
not your Renaissance Team.
We are not talking EdVis or PresentationVis, we are talking
HackerVis/NerdVis/DeepDownAndDirtyViz.  We can't do it for you.
You the researcher have the eyes.  Only you can make the discovery:
to see differences where your artist, your programmer, your cognition expert
can't, and to see similarity where the average man can't.

Miya's Suggestion: Never view an image or film, too fast.  You should control
the rate at which you observe.  Use tools if you have to: hand lenses, filters,
etc.  If you are forced to view something too fast, jump up and say:
	"Wait, just one damn minute!"
Bob Sharp (Emeritus, Caltech Div. of Geog. and Planetary Sciences) presents
an Austin Post photo in one book and asserts that this single photo (of Denali)
is adequate for a 1 hour lecture on glaciology.  That's quite a claim (an
impressive photo).  Artificial data images have yet to assert that kind of
information density (it's not clear they should, but these are opinions).
This should be considered an implicit challenge for visualizations to get
that important for discovery.  Sometimes, some fields pour days, weeks, and
months trying to understand (interpret) an image.

Miya's Gross Generalization: Scientists like grided graph paper (and tabular 
papers) like many artists (painters) like starting with a blank canvas
(exceptions always locatable).
Frames of reference are needed badly.  Include everything a good map has:
1) A Scale, 2) a legend (both geometric and any symbology like color or
glyps or icons, whatever).  Beware of perspective.  $Billion$ are spent
yearly to remove perspective from photographic imagery.

Miya's Guess: the biologists will figure this all out before the physicists,
chemists, and others.  Others should attempt to prove this wrong.
Good luck guys. 8^)

Other inspirations: Muybridge and Edgerton.
		Add your own.
	Muybridge did his basic research at Stanford and Penn State.
	His work went on to become the motion picture industry, ergonomics,
	system analysis (time motion studies).  Edgerton is best known
	for his work on the strobe, super-fast and time lapse photography,
	and side-scanning sonar.

Hints on Design from Don Norman  -- used with permission
("Turn Signals are the Facial Expressions of Automobiles")

	A challenge to the designers of the world:
		Make signs unnecessary.
Think of the Four-Questions test and generalize to systems.
Norman originally wrote this test for kitchen appliances, but it generalizes
well to scientific computer systems
	Ouestion one: Where would we store it?
			[Consider disk space as well as foot print.]

	Ouestion two: Where would we use it?
			[Left to you.]

	Ouestion three: Where would we plug it in?
			[Consider more ways that power.]

	Ouestion four: How much work would it be to clean?
			[A question of maintenance.]

	Generalize additional important questions:

Robert Lucky notes the qualities of pictures in Silicon Dreams (pp. 292):

	describing spatial relationships
	showing the structure of data
	allowing pattern matching approaches to problem solving
	getting attention
	describing and identifying people
	invoking esthetic appreciation

This boils down largely to "geometry."

The problems:
	Hidden object elimination (obscured features)
	Optical illusions (leading to false interpretations, e.g. Necker cubes)
	Inadvertant data corruption
	Parallax and perspective in 3-D and higher D.
	Performance

Science differs from art in that we have to validate our simulations and
theory.  Right now, support for this validation is especially lacking.
Empirical/experimental techniques make simulation validation difficult,
in the works of Eduard Imhof speaking about maps:

Chap. 16 page 359.
7. On art in cartography

 The means of cartographical expression are subject to the same experiences
and visual aesthetic rules as every other type of graphic product.  *Art*
however, is the highest level attainable in graphical work.  Thus, a good map
cannot lack an artistic touch.
  There has already been much debate and writing on the question of whether
cartography has anything to do with art and if so, how much.  We must try to
remain in the clear on this topic and avoid exaggeration and cliche.  Certainly 
it is not a function of cartography to create art in the higher sense of the
word: the cartographer has scarcely the opportunity of doing so.  Art
presupposed the widest ranging freedom of form and structure, whereas
cartographers are confined to the smallest details by topographical survey,
statistical figures, by standardization of symbolism and color, and by what
is essentially a non-artistic purpose.  On the other hand, however, the
following facts are clearly established; we demand of it a balanced
expression which emphasizes the significant and subdues the insignificant;
amd we demand a well balance, harmonious interplay of all elements contained.
It is in accordance with practical experience, however, which the author has
personally observed over many decades, that in cartographic affairs, as in
all graphic work, the greatest clarity, the greatest power of expression,
balance and simplicity are concurrent with beauty.  To create beauty, a
purely technical, practical arrangement of things is not sufficient.  Beauty
is, to a large extent, irrational.  Artistic talent, aesthetic sensitivity,
sense of proportion, of harmony, of form and color, and of graphical
interplay are indispensible to the creation of a beautiful map and thus to a
clear expressive map.


Systems
=======

                StereoGraphics Corporation
                2171 East San Francisco Blvd.
                San Rafael, CA 94901
                ph: (415) 459 4500
                fax: (415) 459 3020

NCAR
----
	National Center for Atmospheric Research
		One of the original graphics packages.
	Platforms:
		Sun, RS6000, SGI, VAX, Cray Y-MP, DecStations, and more.
	Availability:

	Contact:
		scdinfo@ncar.ucar.edu
		(303)-497-1201

	Cost:	.edu
		$750 Unlimited users

		.gov
		$750 1 user
		$1500 5 user
		$3000 25 user

		.com users multiply .gov * 2.0


MOVIE.BYU
---------
See also Cquel.byu
CQUEL.BYU (pronounced "sequel") is a brand new modelling and
visualization package for the UNIX workstation.  Some of it's features
include: animation, raytracing, scientific visualization, interactive
modelling and editing, quadric primitives, Bezier and NURBS surfaces,
constructive solid geometry, texture mapping, graphical user
interface, and free-form deformation to name a few.

	Platforms: SUN, DEC, HP, SGI, IBM RS6000, others,

	Availability:
	Cquel.byu
		30-day trial period w/o obligation

	Contact:
           Engineering Computer Graphics Laboratory
           Brigham Young University
           368 Clyde Building
           Provo, UT  84602
           PHONE:  801-378-2812
           E-Mail: cquel@byu.edu

	Cost:
		$20 for 30-day trial period w/o obligation
		$1,500 for a license (exec. code, etc.)

PLOT3D
------

	Platforms:
	Availability:
	Contact:
	Cost:

apE III
---
	Platforms:
	Availability:
	Contact:

     TaraVisual Corporation
     929 Harrison Avenue
     Columbus, OH 43215
     Tel. (614) 291-2912  and  1-800-458-8731
     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.

AVS
---

	See also:
		comp.graphics.avs

	Platforms: CONVEX, CRAY, DEC, Evans & Sutherland, HP, IBM, Kubota,
		Set Technologies, SGI, Stardent, SUN, Wavetracer
	Availability: AVS4 available on all the above:
		for all UNIX workstations
	Contact:
	Advanced Visual Systems Inc.
	300 Fifth Ave.
	Waltham, MA    02154

	(617)-890-4300   Telephone
	(617)-890-8287   Fax
	avs@avs.com      Email

		 Advanced Visual Systems Inc. for: CRAY, HP, IBM, SGI,
		 Stardent, SUN
		 Advanced Visual Systems Inc. or CRAY for CRAY
		 CONVEX for CONVEX
		 DEC for DEC
		 Evans & Sutherland for Evans & Sutherland
		 Advanced Visual Systems Inc. or IBM for IBM
		 Kubota Pacfic Inc. for Kubota
		 Set Technologies for Set Technologies
		 Wavetracer for Wavetracer
		
	See also: comp.graphics.avs
	FTP Site: for modules, data sets, other info:
		avs.ncsc.org (128.109.178.23)
	Cost: 


SGI Iris Explorer
-----------------
	See also:
		comp.sys.sgi
		comp.graphics.explorer
	Platforms: SGI IRIS, Cray Y-MP, Cray 2, others in progress
	Availability: Available now on SGI, Summer '92 for Cray
	Contact: SGI for IRIS version, Cray for Cray version
	Cost: Bundled on new IRIS systems (not sure of Cray license).

The explorer ftp site is :

ftp.epcc.ed.ac.uk which is housed at Edinburgh Parallel Computing Centre.
The administrator is Gordon Cameron (my office mate).

The mirror address stateside is swedishchef.lerc.nasa.gov


Visual3
-------
	Platforms:
	Availability:
	Contact:
	 contact Robert Haimes, MIT
	Cost:

FieldView
---------
	Platforms:
	Availability:
	Contact:
	 Intelligent Light Corp.
	Cost:

VIS-5D
------
   a system for visually exploring the output of weather
   models and similar data sets.

          SGI Power/VGX, Power/GTX, PI, Crimson and Indigo;
          IBM RS/6000 with GL graphics;
          Stardent GS-1000 and GS-2000
 
        Availability:
          ftp vis5d.ssec.wisc.edu  (or ftp 144.92.108.66)
 
          Login as anonymous and send your id as the password
          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.
 
        Cost: freeware (thanks to NASA for supporting the development)
 
        Contact:
        Bill Hibbard (whibbard@vms.macc.wisc.edu)
        Brian Paul (bpaul@vms.macc.wisc.edu)
 

IBM Data Explorer
-----------------

     Currently available on: IBM Risc System 6000,
                             IBM POWER Visualization Server (32 i860, 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

	Cost:

Khoros 1.0 Patch 5
------------------
	See also:	comp.soft-sys.khoros

	Platforms:	Sun, SGI, DEC, HP, IBM, NeXT, Convex and others

	Availability:	Available now on all platforms.

	Contact:	The Khoros Group
			Room 110 EECE Dept.
			University of New Mexico
			Albuquerque, NM 87131

			Email: khoros-request@chama.eece.unm.edu
		
	See also:	comp.soft-sys.khoros

	FTP Site:	The Khoros system and user contributed code available
			via anonymous ftp from pprg.eece.unm.edu [129.24.24.10]
			in /pub/khoros

			Before installing Khoros, retrieve the file
			/pub/khoros/release/install.ftp

			Precompiled binaries are available for Sun (sparc),
			SGI and DEC (mips) architectures.

			A tape and printed copies of the documentation can
			be obtained from the Contact address above, for $250

Spyglass Dicer
------------------
	3D volumetric data analysis package

	Platform: Mac

	Availability: now shipping

	Contact:
		Spyglass, Inc.
		P.O. Box 6388
		Champaign, IL  61826
		(217) 355-6000

	Cost:

Spyglass Transform
------------------
	2D data analysis package

	Platforms: Mac, SGI, Sun, DEC, HP, IBM

	Availability:
		HP and IBM: September 92
		Others: now shipping

	Contact:
		Spyglass, Inc.
		P.O. Box 6388
		Champaign, IL  61826
		(217) 355-6000
	Cost:

Data 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

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.

WIT
---

  WIT - commercial image processing package with a visual programming
  interface, a product of Logical Vision. Provided for use on the Catalyst
  CDware program as trial software; demo version on Sun CDware 4.

Platforms: Sun3, Sun4, vxWorks by Wind River Systems, and
		Datacube (MaxVideo-20 hardware) platforms.
	Special hardware:
       12 Mb. of memory and color monitor suggested Special software:
       OpenWindows or X Window system

Cost: WIT for Sparc, one yr. free upgrades, 30 days technical support $5000 US
Academic institutions: discounts available
Currently sending free 3.5" demo disks for Sun Sparcstation.

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>

VoxelBox
-------------------
	A 3D Volume renderer for Windows. Features include direct
	ray-traced volume rendering, color and alpha mapping,
	gradient lighting, animation, reflections and shadows.

	Platform: Windows 3.x on a PC(386 or higher) with at least
		  an 8 bit video card(SVGA is fine)

	Availability: now shipping

	Contact:
		Jaguar Software Inc.
		573 Main St., Suite 9B
		Winchester, MA 01890
		(617) 729-3659
		jwp@world.std.com (john w poduska)

	Cost: $495


others


Issue/problems
--------------


How to get more quantitative systems?


Employment:
Job postings (resumes or offerings) are encouraged, BUT please use your
news software appropriately.  The best way to post is cross post
comp.graphics.visualization,misc.jobs.offered (or resumes). (No spaces between
newsgroups.  Then fill the Followup-To: field with "poster."
Please read the misc.jobs.offered (or resumes) FAQ (posted twice monthly) for
stylistic considerations BEFORE POSTING.


Netiquette
----------

We assume you have read news.announce.newusers and that you understand
network informalities.  This group is not moderated, and this is one
experiment in self-moderation (education).

If you have questions, ask you system administrator.  If you are the system
administrator, use MAIL, and ask your net neighbors.

Do not post TESTS here.  Special testing groups exist to acknowledge your
posts.  Test in misc.test, or in your locale: e.g., ba.test, ca.test, na.test,
etc.

Some people believe the charter should be posted.  The name of the group
should sufficiently convey the purpose of this group.

Flame wars: 1) Flame using mail.  Failing that 2) Cut down on the number
of groups in your Newsgroups: line.  3) Use Followup-To: a line with
fewer newsgroups.  Make certain you read all posts before responding, the net
is asynchronous enough as it is: the History of Dumb posts includes such
titles as
"What time is it?"  "The Space Shuttle blew up!" and "California just had an
earthquake."  See your local broadcast news.

Attribution: (Those lines frequently beginning with ">")  MINIMIZE.
Especially: don't post "Me, too" posts after 100 lines of attribution.
Remove especially long sigatures at the bottoms of posts.
Use email.  Show that you are intelligent and net savvy in your postings.
Edit carefully.

DO NOT BOTHER TO ASK FOR PROPRIETARY or pre-release of scientific data.
Many organizations and individuals involved in scientific research are
given a lean (90 day, 1 year, several years).  This is sometimes akin
to asking for trade secrets.  Don't bother.

Posting ads: Rules do not specifically prevent posting advertising so long
as it is done is good taste.  The specific prohibitions come from specific
hosts such as those from the original Internet: machines funded by
US Government monies.  These machines are not to be used for personal gain
or profit.  Specific criminal problems won't be elaborated here for space.
If in doubt, ask someone first.

General graphics references can be found in comp.graphics.
This is the place to ask more general questions like graphics formats.
There, an FAQ will soon exist.  An electronic references
server daemon is also under work as well.
Hardware specific questions like IBM PC or SGI or SUN, etc. specific questions
are probably best answered in groups specific oriented to those machines.

Because this group is unmoderated, it is open to posts which call for
pyramid schemes, calls to send postcards to sick children, and other posts.
	1) Ignore those.
	2) Flame the poster via email.
	3) Use the Followup-To: line redirecting out of the group (net.akido)
		after one cross-post in the group.
That is the price of free speech as ruled in the United States.
The general feeling is that c.g.v. should be more oriented to that
mystical thing called visualization.


References
==========

Other useful newsgroups
-----------------------
		comp.sys.sun
		comp.graphics.avs
		comp.sys.sgi
		comp.infosystems.gis
	comp.graphics
	sci.image.processing

Books
-----

Convert to refer:
	E. Tufte, The Visual Display of Quantitative Information
Cleveland, William: "The Elements of Graphing Data" Wadsworth Advanced
Books and Software.

Tukey, John: "Exploratory Data Analysis"
Addision Weseley, pub.

"Graphics and Graphic Information Processing" - Translated by William J.
Berg and Paul Scott,
  Walter De Gruyter, Publisher.

%A Edward Huff
%T How to Lie with Statistics

%A Mark Monmonier
%T How to Lie with Maps
%I Univ. of Chicago Press
%C Chicago
%D 1991
%X	Ch. 2 Elements of the Map
	Ch. 3 Map Generalizations: Little White Lies and Lots of Them
	Ch. 4 Blunders that Mislead
	Ch. 5 Maps that Advertise
	Ch. 6 Development Maps (or, How to Seduce the Town Board)
	Ch. 7 Maps for Political Propaganda
	Ch. 8 Maps, Defense, and Disinformation: Fool Thine Enemy
	Ch. 9 Data Maps: Making Nonsense of the Census
	Ch. 10: Color: Attraction and Distraction

Jacques Bertin's "The Semiology of Graphics" ?
- it's what Tufte should have been (although it predates both books).

@book{Earnshaw:92,
	editor		= {Earnshaw, R.A. and Wiseman, N.},
	title		= {An Introductory Guide to Scientific Visualization},
	publisher	= {Springer-Verlag},
	year		= 1992,
	month		= {September},
	note		= {ISBN 3-540-54664-2, ISBN 0-387-54664-2}
}

@book{Brodlie:92,
	editor		= {Brodlie, K.W. and Carpenter, L.A. and
				Earnshaw, R.A. and Gallop, J.R. and
				Hubbold, R.J. and Mumford, A.M. and
				Osland, C.D. and Quarendon, P.},
	title		= {Scientific Visualization ---
				Techniques and Applications},
	publisher	= {Springer-Verlag},
	year		= 1992,
	month		= {January},
	note		= {ISBN 3-540-54565-4, ISBN 0-387-54565-4}
}


Better than average papers

@INPROCEEDINGS{Insel90a,
	AUTHOR = "Alfred Inselberg and Bernard Dimsdale",
	TITLE = "Parallel Coordinates: A Tool for Visualizing
		 Multi-dimensional Geometry",
	BOOKTITLE = "Proceedings of the First IEEE Conference on 
		Visualization, San Francisco, 23-26 October 1990",
	EDITOR = "Arie Kaufman",
	PUBLISHER = "IEEE Computer Society Press",
	PAGES = "361-377",
	YEAR = 1990}

Journals
--------

IEEE Computer Graphics & Applications

ACM Transactions on Graphics

The Journal of Visualization and Computer Animation
	published by John Wiley & Sons Ltd, ISSN 1049-8907

	Scientific Programming: A Wiley-Interscience Publication
Subscription:
In the US:
	Scientific Programming: A Wiley-Interscience Publication
	John Wiley and Sons
	Periodicals Division
	P.O. Box 7247-8491
	Philadelphia, PA 19170-8491
Outside the US:
	Scientific Programming: A Wiley-Interscience Publication
	John Wiley and Sons
	Journals Administration Dept.
	Baffins Lane, Chichester
	Sussex PO19 1UD
	England


Magazines
---------

	Pixel

Conferences & workshops (see also the proceedings from years passed):
---------------------------------------------------------------------

Visualization '9x - Annual visualization conference 
SIGGRAPH 	  - Annual ACM graphics conference
Eurographics '9x	- Annual European graphics conference of the
			  Eurographics association

"less than annual" Conferences
------------------------------

Symposium on Interactive 3D Graphics
Volume Visualization Workshop
Usenix Graphics Workshop


Contributions
=============

Mail it to me (amelia).  I prefer concise text which can just be concatenated
into this file.  No long winded speeches please.  I'm just a computer.

	"Take me I'm yours....."

======TAG LINE=====


From: Nick (Nikolaos) C Fotis <nfotis@theseas.ntua.gr>

Hello, here's the latest version of my SciVi and Mol. Vis. stuff
(minus + and # signs). Basically, I got your latest updates and I
incorporated them here:


17. Scientific visualization stuff
----------------------------------

a. NCSA 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).
   This site has *lot* of Visualization tools. You're advised to look at it.

b. 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 for more info....

c. 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)

d. IRIS Explorer is 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 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.

e. 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.

f. 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 Pacfic Inc. for Kubota
  Set Technologies for Set Technologies
  Wavetracer for Wavetracer


i. Wavefront products.

j. 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 :-(

k. XGRAPH : On the contrib tape of X11R5. It specialty is display of up
   to 64 data sets (2D).


==========================================================================

18. Molecular visualization stuff
---------------------------------

[ Based on a list from cristy@dupont.com < Cristy > , which asked for
 systems for displaying Molecular Dynamics, MD for short ]

a. Flex is a public domain package written by Michael Pique, at The Scripps
   Research Institute, La Jolla, CA. Flex is stored as a compressed,
   tar'ed archive (about 3.4MB) at perutz.scripps.edu [137.131.152.27], in
   pub/flex. It displays molecular models and MD trajectories.

b. MacMolecule (for Macintosh). I searched with Archie, and the most
   promising place is sumex-aim.stanford.edu (info-mac/app, and
   info-mac/art/qt for a demo)

c. If you are running on an SGI, try MD-DISPLAY, from Terry
   Lybrand (lybrand@milton.u.washington.edu).

d. Duncan McRee <dem@scripps.edu> has something called XtalView.  It is a
   crystallography package that does visualize molecules and much more.
   It uses the XView toolkit.

e. landman@hal.physics.wayne.edu:

   I am writing my own visualization code right now.  I look at MD output
   (a specific format, easy to alter for the subroutine) on PC's.  My
   program has hooks into GKS.  If your friend has access to Phigs for X
   (PEX) and fortran bindings, I would be happy to share my evolving code
   (free of charge).  Right now it can display supercells of up to 65
   atoms (easy to change), and up to 100 time steps, drawing nearest
   neighbor bonds between 2 defining nn radii.  It works acceptably fast
   on a 10Mhz 286.

f. icsg0001@caesar.cs.montana.edu:

   I did a project on Molecular Visualization for my Master's Thesis, using
   UNIX/X11/Motif which generates a simple point and space-filling model.

g. KGNGRAF by IBM.

h. ditolla@itnsg1.cineca.it:

   I'm working on molecular dynamic too.  A friend of mine and I have
   developed a program to display an MD run dynamically on Silicon
   Graphics.  We are working to improve it, but it doesn't work under X,
   we are using the graphi. lib. of the Silicon Gr. because they are much
   faster then X.  When we'll end it we'll post on the news info about
   where to get it with ftp. (Will be free software).

i. XBall V2.0: written by David Nedde. Call daven@maxine.wpi.edu.

j. XMol:  an X Window System program that uses OSF/Motif  for  the
   display and  analysis  of  molecular  model data.  Data from several
   common file formats can be read and written; current formats include:
   Alchemy, CHEMLAB-II, Gaussian, MOLSIM, MOPAC, PDB, and MSCI's XYZ
   format (which has been designed  for  simplicity  in  translating to
   and from other formats). XMol also allows for conversion between
   several of these formats.
   Xmol is available as ftp.msc.edu:pub/xmol/xmol.tar

k. INSIGHT II from BIOSYM Technologies Inc.

l. SCARECROW. The program has been published in J. Molecular Graphics 10
   (1992) 33. The program can analyze and display CHARMM, DISCOVER, YASP
   and MUMOD trajectories. The program package contains also software for
   the generation of probe surfaces, proton affinity
   surfaces and molecular orbitals from an extended Huckel program.
   It works on Silicon Graphics machines.
   Contact Leif Laaksonen <Leif.Laaksonen@csc.fi or laaksone@csc.fi>

[ I would also suggest looking at least in SGI's Applications Directory.
 It contains many more packages - nfotis ]

==========================================================================


Article 9 of comp.graphics.explorer:
From: tohanson@gonzo.lerc.nasa.gov (Jeff Hanson)
Subject: FAQ for Explorer, slightly dated

Here is the currect FAQ for Explorer.  Note that it is slightly dated
since it does not reflect the existance of this news group.  I'm sure
Gordon will soon generate a new FAQ and post it here.

          oOo Explorer Frequently Asked Question List oOo
          ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
                          Version 0.2 

               Last Altered 12th April 1992 - G.C.

           !!!!! Please Redistribute this Article !!!!!!

+ Introduction +
~~~~~~~~~~~~~~~~

This document contains answers to some Frequently Asked Questions (FAQs)
asked of the Explorer Modular Visualisation Environment (MVE). 

The latest update of this can always be obtained by FTP from :
	UK Site : ftp.epcc.ed.ac.uk (129.215.56.29)
(	US Mirror : swedishchef.lerc.nasa.gov (139.88.54.33) 	)

If you wish to be part of the Explorer mailing list, comment on this
FAQ, add/alter/CORRECT any questions, or have any suggestions, please
email:
	explorer-request@castle.ed.ac.uk, or
	gordonc@epcc.ed.ac.uk

Where relevant and possible, the sources of information are listed after
the answers - many of the questions stem from those on the mailing
list. Direct quotes are indented.

N.B. The compilers of this FAQ are independent of SGI (developers of
Explorer) - this also means that any inaccuracies are most probably our
own faults ! Thanks to the XUG and the X FAQ for ideas.
		- Gordon Cameron (Edinburgh Parallel Computing Centre)
			gordonc@epcc.ed.ac.uk
		- Chris Thornborrow, Matthew White (EPCC)

Key :
~~~~~
	+	:	New since last update
	*	:	Changed since last update
	@	:	Bug question (+ fix)

+ Topics +
~~~~~~~~~~
A) TOPIC: GENERAL INFORMATION
 A.1) What is Explorer ? 
 A.2) What platforms will Explorer run on/what are the requirements ? 
 A.3) How can I get Explorer ? 
 A.4) Modules, Maps & Ports - What are they ? 
 A.5) What is the Map Editor/Librarian ? 
 A.6) What Data Formats can Explorer handle ? 
 A.7) What is the Data Scribe ? 
 A.8) What is the Module Builder ? 
 A.9) What are the MCW and MDW ? 
 A.10) What is an MVE ? 
 A.11) What other MVEs are there ? 
 A.12) Is there any overlap between ImageVision and Explorer ? 
-
B) TOPIC: RUNNING EXPLORER
 B.1) Why does Explorer crash immediately ? +
 B.2) Can I run Explorer on one machine and display on another ? 
 B.3) Can I run modules on different machines ? 
 B.4) How can I start Explorer with a prefined map ? 
 B.5) Can I run Explorer in batch mode (i.e. without the GUI) ? 
 B.6) Will Explorer work with very large data sets ? 
 B.7) When does a module fire ? 
 B.8) Why does Explorer run slowly on my system ? 
 B.9) How can I customize the look of Explorer ? 
-
C) TOPIC: USING EXPLORER with the MAP EDITOR
 C.1) Why does Explorer ignore all my input ? @
 C.2) Why can't I start a GenerateColormap module ? 
 C.3) How can I stretch the librarian scrolling list ? 
 C.4) How can I slice into an iso-surface ? 
 C.5) How can I render translucent solids ? 
 C.6) Why can I not get LatFunction to work ? +@
-
D) TOPIC: USING THE DATASCRIBE
 D.1) Why does the help file not reflect the actual widget ? @
-
E) TOPIC: USING THE MODULE BUILDER
-
F) TOPIC: PROGRAMMING MODULES
 F.1) How can I wake Explorer on events ? 
 F.2) What has happened to the routine cxInputPortStateGet ? @
-
G) TOPIC: MODULES AVAILABLE/WANTED
 G.1) Where can I get PD modules ? +
-
H) TOPIC: FURTHER INFORMATION
 H.1) Where can I obtain documentation (e.g. Module Writers' Guide) ? *
 H.2) Is there a mailing list/FTP site ? *
 H.3) Is there a relevant newsgroup ? 
 H.4) Why are the electronic PostScript files incomplete ? *
-
I) TOPIC: MISCELLANEOUS
 I.1) How can I add/correct or comment on Q&As on the FAQ ?
 I.2) Where can I find a list of bugs ? +
-

+ Full Q&As +
~~~~~~~~~~~~~
======================================================================
A) TOPIC: GENERAL INFORMATION
======================================================================
A.1) What is Explorer ? 

	IRIS Explorer is an application creation system and user
	environment that provides visualisation and analysis
	functionality for computational scientists, engineers, and
	other investigators. It is especially useful for those whose
	needs are not met by commercial software packages. Also, IRIS
	Explorer's Graphical User Interface (GUI) allows users to build
	custom applications without having to write a single line of
	code.

			[from IRIS EXPLORER - Technical Report(SGI)]
----------------------------------------------------------------------
A.2) What platforms will Explorer run on/what are the requirements ? 

Explorer is included at no cost with each Silicon Graphics
workstation.  Explorer can be ordered for existing workstations at a
nominal media charge. It is also available from Cray Research for Cray
Research computers, and it is hinted that the package will be ported
soon(#:-} to other platforms.

On SGI platforms, requirements are that the machine have a 24 bit plane
(or virtual 24 bit plane) frame buffer i.e. All except Personal Irises
with 8 bit planes. In addition, 16MB is the minimum memory requirement,
although 24 megs is recommended, especially when the data sets to be
visualised are particularly large.

In particular, you must be running version 4.0.1 of the OS, or higher.

			[Leo Blume(SGI) and Release Notes for Explorer]
----------------------------------------------------------------------
A.3) How can I get Explorer ?

Contact your local SGI supplier for details of what Explorer is available
on, and how to obtain it.
----------------------------------------------------------------------
A.4) Modules, Maps & Ports - What are they ? 

A MODULE is a single software tool for performing a particular task.
Explorer is shipped along with a wide range of modules to perform tasks
such as data input, rendering, image processing and manipulation. Each
module has associated input and output PORTS which control the flow of
data in and out of the module.

Modules are connected together to form pipelines which perform specific
higher level tasks. The collection of such modules and the links between
them are referred to as Explorer MAPS. The function of the map is implicitly
defined by the functions of the modules and their interconnectivity.
----------------------------------------------------------------------
A.5) What is the Map Editor/Librarian ? 

The Map Editor and Librarian are the two main windows that are used
when you use Explorer.

The MAP EDITOR is a graphical tool for assembling the maps by picking
modules and joining them together in an intuitive manner. The editor
will only allow the connection of input/output port pairs of the same
data type, so Explorer is a `strongly typed system'.  The map editor is
effectively the interactive prototyping environment of Explorer.

The LIBRARIAN is the tool which allows you to browse through existing
modules and maps, to choose those which you wish to use with the map
editor.
----------------------------------------------------------------------
A.6) What Data Formats can Explorer handle ? 

Explorer works on 5 main types of data :
	Parameter : Scalar values such as integers and doubles.
	Lattice : A Generalized multi-dimensional array.
	Pyramid : Combines lattices with connectivity information in
		a hierarchical structure.
	Geometry: A general, hierarchical, geometric description.
	Unknown : An uninterpreted stream of bytes 

The first four types will be consistent between modules perhaps
executing on different machine architectures, whereas the last unknown
type does not have this feature (unless the user adds XDR-like data
conversion him/herself).
----------------------------------------------------------------------
A.7) What is the Data Scribe ? 

The DataScribe is a graphical utility to allow the user to build
templates which can convert data between formats - this is typically
used to convert a customized user data file into a lattice(say) and
vice versa.

These data conversion templates, when completed, constitute modules in
Explorer which can be used in the same fashion as any other module.
----------------------------------------------------------------------
A.8) What is the Module Builder ? 

The Module Builder is a graphical utility to aid in the creation of
Explorer modules, by helping you define which data types the module has
on its input and output ports, which widgets correspond to which
parameters, and how the module will look when placed in the Map
Editor.

The Module Builder can also automatically generate one of the extra
layers of wrapping around the core function, namely the  Module Data
Wrapper (MDW).
----------------------------------------------------------------------
A.9) What are the MCW and MDW ?

The innermost layer of an Explorer module is the computational
algorithm which provides the base functionality.  This is surrounded
first by the Module Data Wrapper (MDW) - which can be generated
automatically by the Module Builder - and this performs the conversion
of data from Explorer format at ports to the algorithm's internal
format, and vice versa.

The outermost layer is the Module Control Wrapper (MCW) which is the layer
responsible for communicating the module's input and output (Explorer)
data with other modules, and maintaining data consistency (a la XDR).
This layer also handles comms with the local controller and the firing
mechanism.

The MCW is necessary whereas the MDW may be bypassed by the programmer
if desired, allowing direct access to data at the ports.
----------------------------------------------------------------------
A.10) What is an MVE ? 

A Modular Visualisation Environment (MVE) is a package for data
visualisation consisting of a user interface allowing linking of
modules in a pipeline. Explorer is an example of an MVE.

			[ Chris Thornborrow, EPCC ]
----------------------------------------------------------------------
A.11) What other MVEs are there ?  

Other MVEs include :
	AVS - now marketed by AVS (see comp.graphics.avs)
	apE - originally developed by Ohio Supercomputer Centre
	Khoros - developed by University of New Mexico 
		(see comp.soft-sys.khoros)

It would probably be more correct to define Khoros as a MAB (Module
Application Builder) , as it is not aimed solely at visualisation. 
----------------------------------------------------------------------
A.12) Is there any overlap between ImageVision and Explorer

ImageVision is an object oriented image processing library that
currently has about 70 image processing functions. The architecture of
ImageVision is designed to handle virtually any size and data typed
image. The ImageVision library runs on all SGI machines and on a Cray.

The image processing modules of Explorer were developed using ImageVision,
and these modules in Explorer map directly to single ImageVision objects.

				[Nancy Cam - SGI]
======================================================================
B) TOPIC: RUNNING EXPLORER
======================================================================
B.1) Why does Explorer crash immediately ? 

The main reasons that Explorer will crash on startup (on an SGI machine)
are :
	a) Wrong OS
	b) Incorrect installation

a) Explorer on an SGI requires IRIX v4.0.1 or later.

b) 

	If you use the "-r" option on "inst" when installing Explorer,
	the X11 resource default files do not get installed correctly.

	Similarly, if you NFS mount /usr/explorer from a file server,
	these default resource files are not installed on your
	machine.  If you must install Explorer somewhere other than
	/usr/explorer, first create /usr/explorer as a symbolic link to
	a directory somewhere else, then install Explorer.  If you have
	installed Explorer with "inst -r" or if you NFS mount it from
	another machine, you can set up the necessary symbolic links
	for the X11 app-default files and the shared libraries by using
	the command (as root):
	    inst -f /usr/explorer/lib/inst/explorer 

	This will establish symbolic links in /usr/lib for those files
	that must be present on every machine that runs Explorer.  This
	is explained in section 2.3.1 of the Release Notes. (from SGI)

				[SGI]
----------------------------------------------------------------------
B.2) Can I run Explorer on one machine and display on another ? 

Explorer itself can run on one machine and display on ANY other machine
running an X server. However, the modules Render and DisplayImg will
only display/function on machines with GL hardware.

The Module Builder and Datascribe can run and display on any X terminal.

Since Explorer/Module Builder/DataScribe are X Motif applications, to
get these to run externally and  display on your local workstation
running an X server, set your display variable on the external machine
before executing the program in the usual fashion. e.g.
a) On Local Machine :
	xhost +<remote_machine_name>

b) On Remote Machine :
	setenv DISPLAY <local_machine_name>:0.0
	explorer
----------------------------------------------------------------------
B.2) Can I run modules on different machines ? 

Modules within an Explorer map can execute on different machines,
provided that those machines have the execution environment of Explorer
ported to them.  For example, in a network of 5 SGI w/stations, each of
the 5 modules of an Explorer map can be running on a different
workstation.  This is achieved by pulling up a librarian for each of
the machines on which you wish to execute modules. The librarian for
these machines will show which modules are available, and these can be
placed in a map in the same manner in which local modules are placed.
Everything will `look' the same, except that the remote modules will
fire and execute on the remote machines - this could be referred to as
a form of coarse grain parallelism.

At present, the execution environment is ported to SGI and Cray platforms,
so modules can only execute on these machine types.
----------------------------------------------------------------------
B.3) How can I start Explorer with a prefined map ? 

To run explorer with a predefined map, type :
	explorer -map <mapname>

,and the map will appear in the Map Editor when it starts up.
----------------------------------------------------------------------
B.4) Can I run Explorer in batch mode (i.e. without the GUI) ? 

	Version 1.0 does not have a non-GUI capability.  There are
	designs being kicked around, but we believe that a totally
	non-GUI solution is not the full answer, since the "answer"
	produced by an Explorer map may in fact be an image that you
	want to view.  On the other hand, some Explorer maps may only
	filter data, produce geometry into a file and not incorporate
	viewing at all.  This "batch mode" would be useful for very
	long animation runs, for example.

	Khoros also lets single modules to run "standalone".  We don't
	see this as a requirement for Explorer, except that it could
	make module debugging simpler -- one of our short-term goals.
	Being able to debug a module without all of Explorer hanging
	around would be really nice, especially as debugging tools take
	more and more resources from the machine.

				[ Bob Brown - SGI ]
----------------------------------------------------------------------
B.5) Will Explorer work with very large data sets ? 

The easiest option if you have very large modules is to purchase more
memory, but this only extends so far. 

	Large data sets:
	This is a general weakness of data flow systems.  We have a few
	ideas for helping out, but it becomes very complicated when you
	want to preserve a conceptually simple programming model.  Can
	we offer an alternative execution model (that is, how things
	really compute and share data) yet maintain a simple
	programming model (that is, how the user states what is
	wanted).

				[ Bob Brown - SGI ]
----------------------------------------------------------------------
B.6) When does a module fire ?

Module inputs can be optional or required, and if the former then the module
can happily fire without any input on that port. If the port is required,
then a module won't fire until it has data on that port.

When new data arrives at a required port, then the module fires. 

Question:
	We reckon that it would be `nice to have' a template matching
	type operation at the input of each module, so that intelligent
	decisions can be made as to WHEN to fire a module. e.g. don't
	fire a module when ANY of its inputs change, but be able to
	choose how a module will fire and how many of its inputs are
	REQUIRED before a successful fire - this sort of thing would be
	useful in animations involving multiple file reads.
				[ Gordon Cameron - EPCC ]

The reply :
	We spent a lot of effort on this in the design phases, and came
	up with an overly powerful scheme that would be practically
	unusable, so it did not appear in V1.0.  The degree of
	flexibility that can be offered seems too great, particularly
	when youconsider the possibility of being able to
	programmatically add and delete ports.

	Of course, using cxInputDataChanged judiciously will let you
	essentially write your own inner firing rules.  However, this
	may break future versions of the firing algorithm.  Also, if
	you have a non-MDW module and never issue a cxInputDataGet call
	on a port with new data, cxInputDataChanged will always report
	that there is new data on the port.  You must use
	cxInputDataGet to change the port data state from "new" to
	"old".
				[ Bob Brown - SGI ]
----------------------------------------------------------------------
B.7) Why does Explorer run slowly on my system ?
				[ Jack Gallant - Caltech ]

	The overhead of X windows and Motif is not insignificant.  Two
	factors can really slow down Explorer: insufficient memory and
	NFS mounting /usr/explorer.  The first one we can help out
	with, but the second one is out of our hands for the most part
	(having local copies of the shared libraries can help,
	though).
				[ Bob Brown - SGI ]
----------------------------------------------------------------------
B.8) How can I customize the look of Explorer ? 

Explorer, and the Data Scribe and Module Builder are all X/Motif
applications, and have several resources which can be altered so that the
tools' appearance can be customised. Look at the explorer directory
[/usr/explorer]/lib/X11/app-defaults to see what's what. (The directory
enclosed in square brackets is the home of Explorer on your system).
======================================================================
C) TOPIC: USING EXPLORER with the MAP EDITOR
======================================================================
C.1) Why does Explorer ignore all my input ? 

A possibility is that you have closed the main Explorer window, and an
error has been generated - if you have closed the small gui window,
then the error diagnostic will not appear on the screen, and the entire
interface will appear to hang. However, opening the gui window again
will rectify matters.

			[ Leo Blume - SGI ]
----------------------------------------------------------------------
C.2) Why can't I start a GenerateColormap module ?

If you have applications running that have allocated colormap cells, then
the number of cells available to GenerateColormap is reduced, so that only
one (or perhaps no) GenerateColormap will be able to execute.

One way round this is to reconfigure the X server, and this is
described in Appendix B of the User Guide (also supplied electronically
with the release) - what you end up doing is in effect choosing a
different visual.
----------------------------------------------------------------------
C.3) How can I stretch the librarian scrolling list ?

You can't #:-} , at least not in Explorer 1.0
			[ Roy Hashimoto - SGI ]
----------------------------------------------------------------------
C.4) How can I slice into an iso-surface ?

Full Question :
	I've tried orthoslice, it will move the slice plane into the
	data but the full iso-surface is still there, the outside is
	not cut away.
				[ Gus Williams ]

Answers:
	The slices generated by Orthoslice won't cut away the
	isosurface.  Orthoslice and IsosurfaceLat generate completely
	independent geometry that is composited in the renderer.  It
	might be nice, though, to have this capability in the future.

	For the present, you can use SampleCrop to do that or just
	adjust the transparency on the isosurface so that you can see
	through it to the cutting plane.
				[ Leo Blume - SGI ]

	...you can use CropLattice to crop the
	lattice before taking the isosurfaces.  I'm not sure how it
	could be done any other way with the standard module set.
				[ Robert Skinner - SGI ]
----------------------------------------------------------------------
C.5) How can I render translucent solids ?

You can pass your data through the module VolumetoGeom and then on to
the Render module. VolumetoGeom makes use of a technique known as
"splatting" to visualise volumes like this - a good reference is :

	Hierarchical Splatting: A Progressive Refinement Algorithm for
	Volume Rendering by David Laur and Pat Hanrahan.

..and this paper appeared at SIGGRAPH '91.
----------------------------------------------------------------------
C.6) Why can I not get LatFunction to work ? 

Explorer has a known bug in LatFunction...The following is a long
answer, and will be condensed in time.


Problem a) - Why can I never get LatFunction to work?

	The problem is that if LatFunction's "Program File" typein does
	not refer to an existing file, then the module's interpreter
	gets confused and will never work correctly on any program file
	thereafter.  Unfortunately, the empty string (the default when
	LatFunction is brought up from the librarian) is such an
	invalid name and will confuse the module.

	Thus, the symptom you will see is that the user instantiates a
	LatFunction module, types in a file name, and gets errors. e.g.

		float f[2,3,4];
		Second_Out := First_In;

	yields the error message :
		[Unbound symbol: First_In]

	This identifies problem a) - when you instantiate LatFunction,
	it tries to read file "" and fails.

Solution a)

	All you have to do is instantiate a LatFunction module
	with the Program File name in place. You can do this by
	duplicating the brain-dead LatFunction -- the new
	LatFunction<2> will work as expected (delete the old module
	after duplicating a new one).  You can also save the
	LatFunction module with typed-in name in a map and load that
	map.

	Also, LatFunction-based modules (see the MWG, chapter 4) are
	less prone to this problem for two reasons. This makes them
	easier to work with than plain LatFunction. The first reason is
	that LatFunction-based modules typically have a filename
	specified, so these will work even when dragged from the
	librarian. The second :reason is that they typically have
	required port data, so they will not fire when instantiated,
	thus giving you time to type the right filename.

	========================================================== 

Problem b) - Why does LatFunction give me the "[Unbound
		symbol:...]" error message and refuse to work ?

	This is the same as problem a). The "[Unbound symbol: ...]"
	message is LatFunction's way of saying that it is confused.

Solution b)

	As solution for Problem a).

	========================================================== 

Problem c) - Why does LatFunction sometimes give an error
	"[Unbound symbol:...]" on some line after I edit my
	file, but then not give the error the next time I read
	in the file?

	This is related to problems 1 and 2. In this case the parsed program
	is referenced incorrectly and the interpreter exhibits the same type
	of confusion as before. However, this error is recoverable by
	reparsing the Shape program file (type <CR> in the "Program File"
	typein). 

Solution c)
	Reparse the Shape program file (type <CR> in the "Program File"
	typein).
					[SGI]

======================================================================
D) TOPIC: USING THE DATASCRIBE
======================================================================
D.1) Why does the help file not reflect the actual widget ?

In some cases, the DataScribe can get confused with consistency between
.doc and .help files, but there is a workaround. The following Q&A from
the list illustrates a specific example.

Original Question :
	I created a module using the data scribe which had a file
	browser widget. When I edited the .help file produced the
	following lines were present ..

		pbmascii -- Text
		  <Describe the purpose of the widget here>

	Note that the widget is described as text, not file browser. Is
	this deliberate - I can see how it would be as the file browser
	widget is really an elaborate text widget ?
				[ Chris Thornborrow - EPCC ]

Solution :
	This looks like a bug.  dot-help files are derived from dot-doc
	files.  When you do a "Save" from the datascribe, it appears to
	not rewrite the doc file (even if you changed a widget type,
	say, from Text to File Browser) but it does regenerate the help
	file from the doc file.

	I tried your example and that is what happened.  My guess is
	that you had previously saved when "pbmascii" was really a Text
	widget, then you changed it to a browser and saved again.

	Remove your dot-doc file and do a Save again from datascribe.
	That should fix things up.  Or, if you've already edited the
	doc file, bring up the module builder on your module and select
	"Update Document" under the "Build" menu.
				[ Bob Brown - SGI ]
======================================================================
E) TOPIC: USING THE MODULE BUILDER
======================================================================
======================================================================
F) TOPIC: PROGRAMMING MODULES
======================================================================
E.1) How can I wake Explorer on events ?

	I would like wake-up Explorer on the following event:
		one descriptor is ready for reading/writing 
				[ F. Lapique ]

This has to be done using X directly. The following details how :

	In Version 1.0 Explorer the only way to do this is through X
	windows.  Make your module an X module (in the Build
	Options...  window in the module builder) and then you can use
	the XtAddInput mechanism to register a callback procedure with
	the scheduler.  The Xt manual describes how to use XtAddInput;
	it is relatively simple and straightforward.  We don't have
	code examples, but if you have trouble, let me know and I'll
	write one up.  Another user has reported success at doing
	this.

	Be aware that execution highlighting will not occur when your
	callback is called.  This is because the module isn't "really"
	firing.  In fact, you should not call cxOutputDataSet() or
	cxOutputDataFlush() from the callback.  Instead, if you want to
	send data downstream, use cxFireASAP() from the XtAddInput()
	callback to schedule the firing of your computation routine,
	and maintain some state that lets that routine know what's
	what.

	The next version generalizes this mechanism by adding a
	cxAddInput routine that works the same way, but doesn't
	(necessarily) use X windows.  (We haven't announced a release
	schedule for the next version).

				[ Bob Brown - SGI ]
----------------------------------------------------------------------
E.2) What has happened to the routine cxInputPortStateGet ?

There is no such routine, and it shouldn't appear in the documentation.
To emulate the stated effect, do :

cxInputConnectsGet()    // To tell if port is connected
cxInputDataGet()        // returns 0 for no data
cxInputDataChanged()    // to find if data there is new or old

				[ Dave Foulser - SGI ]
======================================================================
G) TOPIC: MODULES AVAILABLE/WANTED
======================================================================
G.1) Where can I get PD modules ?

There are a few modules available by anon. FTP, including one
to enable/disable geometry information. Many more modules should
appear very soon.

See the FAQ header for FTP addresses etc...
======================================================================
H) TOPIC: FURTHER INFORMATION
======================================================================
H.1) Where can I obtain documentation ? 

Compressed electronic copies of Postscript documents are supplied with
the release of Explorer. Only certain chapters and an Appendix appear
in the directory [/usr/explorer]/doc/userguide, though. You can obtain
the complete User Guide, Module Writer's Guide and Module Definitions
guide by getting in touch with SGI, who can supply bound copies.

The electronic source for the Module Writer's guide is now
available by anon. FTP !! (see header for addresses)

The contact number I have for info on SGI is (415) 960-1980.
----------------------------------------------------------------------
H.2) Is there a mailing list/FTP site ?

At present there is an Explorer mailing list for discussion on all aspects
of the package. The list was started in March of '92, and has around 250
subscribers (not including feeds) - several of the developers of Explorer
are subscribed, so the list provides a good forum for discussion which may
change the shape of future versions.

To join the list, or to get further details, send some mail to :
	explorer-request@castle.ed.ac.uk

There is also an FTP site which contains archives of postings to the
explorer mailing list, as well as many other things including a User
List and an up to date FAQ(this!), and it is hoped that this site will
develop into a store for PD modules in time. There are a few modules
here just now, but many more are expected soon.

The site can be contacted as :
	ftp.epcc.ed.ac.uk (129.215.56.29)
, and supports anonymous FTP. The explorer directory is /pub/explorer.

In addition, Jeff Hanson has kindly mirrored this site in the US as :
	swedishchef.lerc.nasa.gov (139.88.54.33))
----------------------------------------------------------------------
H.3) Is there a relevant newsgroup ?

At present (31st March 1992) there is no newsgroup specifically for
the discussion of Explorer-related issues, although this may well 
change in the near future.

However, the groups comp.sys.sgi and comp.graphics.visualization are
certainly useful, and often relevant #:-}
----------------------------------------------------------------------
H.4) Why are the electronic PostScript files incomplete ? 
The SGI Explorer is supplied with a directory /doc, which contains
the userguide in PostScript form. This is missing Chapter 1 and the
first Appendix. The explanation SGI give is as follows :

	Chapter 1 is the "Getting Started" guide that comes with the
	Explorer CD or tape. The missing appendix contains the module
	manual pages, which are accessible via the Unix "man" command.

	The release notes are on-line and can be viewed by using the
	"grelnotes" command.

	The Module Writer's Guide is not in the software distribution
	in this release because of differing production schedules for
	the software and documentation.  It may be included in future
	releases. (from SGI)

The Module Writers' Guide is now available by FTP in electronic
version.
======================================================================
I) TOPIC: MISCELLANEOUS
======================================================================
I.1) How can I add/correct or comment on Q&As on the FAQ ?

Mail explorer-request@castle.ed.ac.uk . Simple ! 

I.2) Where can I find a list of bugs ? 

A few bugs are listed in this FAQ. Others can be found by looking
at the file in the /pub/explorer/bugs directory at the FTP site.





Article 1990 of comp.graphics.visualization:
From: software@riemann.geom.umn.edu (Geometry Center Software Development Group)
Subject: Geomview is available --- 3D object viewer

The Geometry Center announces release 1.1 of geomview, a program for
looking at and interactively manipulating 3D objects.  The current
version runs on Silicon Graphics IRIS workstations.  It is available
via anonymous ftp at geom.umn.edu (128.101.25.31) in the "pub/geomview"
subdirectory.  "geomview-bin.tar.Z" contains pre-compiled binaries,
documentation, and data and takes up 3 MB of disk space.  The source
distribution is "geomview.tar.Z" and takes up 21 MB of disk space.  To
unpack, type "uncompress < [geomview|geomview-bin].tar.Z | tar xvopf -".

Please send all correspondence regarding this software via email to
"software@geom.umn.edu".

Geomview represents the current state of an ongoing effort at the
Geometry Center to provide interactive 3D graphics software which is
particularly appropriate for displaying the kinds of objects and doing
the kinds of operations of interest in mathematics research and
education.  While geomview was developed as a tool for research
mathematicians, it is a general-purpose graphics system which could be
useful in many domains. It can be used to examine a static object or
as a dynamic display for a running program. An extensive command
language allows programmers to easily extend the functionality of the
basic viewer by writing external modules. Currently hyperbolic
visualization capabilities are built-in, while four-dimensional
visualization is handled through external modules.

Geomview allows multiple independently controllable objects and
cameras.  Interactive control for motion, appearances (including
lighting, shading, and materials), picking on an object, edge or
vertex level, and adding or deleting objects is provided through
direct mouse manipulation, control panels, and keyboard shortcuts.
External programs can drive desired aspects of the viewer (such as
continually loading changing geometry or controlling the motion of
certain objects) while allowing interactive control of everything
else.

Geomview supports the following simple data types: polyhedra with
shared vertices (.off), quadrilaterals, rectangular meshes, vectors,
and Bezier surface patches of arbitrary degree including rational
patches. Object hierarchies can be constructed with lists of objects
and instances of object(s) transformed by one or many 4x4 matrices.
Arbitrary portions of changing hierarchies may be transmitted by
creating named references.

The Geometry Center is an NSF-funded independent research group based
at the University of Minnesota.  The three-fold mission of the Center
is to support and promote mathematics and computer science research;
software, animation, and tool dvelopment and production; education and
communication of mathematics at all levels.  The Geometry Center's
offical name is the "National Science and Technology Research Center
for Computation and Visualization of Geometry Structures".

The Geometry Center  
University of Minnesota  
1300 S. 2nd St.
Minneapolis, MN  55454  USA


Article 1995 of comp.graphics.visualization:
From: vachha@cisa.cis.uab.edu (Rustom (Yuppy) Vachha)
Newsgroups: comp.graphics.visualization
Subject: References on representing N Dim data

References in  represnting  N-dimensional data in  2 or 3 D.

Chambers, J. M., Cleveland, W. S., Kleiner, B., and Tukey, P. A. (1983). 
Graphical Methods for Data Analysis. Belmont, CA: Wadsworth Press.

Wang, P. (1978). Symposium on Graphical Representation of Multivariate
Data. New York: Academic Press.

While these references are very old, they will provide you with a nice
introduction to static multivariate graphics. If you are interested in
dynamic multivariate graphics, I would look at:

Cleveland, W. S., and McGill, M. E. (1988). Dynamic Graphics for Statistics.
Belmont, CA: Wadsworth Press.

Edwin A. Abbott, "Flatland. A Romance of Many Dimensions", Signet, New York,
1884 (reprint). Also from Dover Books.

H.F. Baker, "Higher Geometry; being Illustrations of the Utility of the 
Consideration of Higher Space, especially of 4 and 5 Dimensions" (Principles 
of Geometry; Vol.4), Ungar, 1963.

Dionijs Burger, "Bolland", Veen, Utrecht, 1983. In Dutch, but there are
English translations as well, probably titled "Sphereland". I don't know who
published these.

Thomas F. Banchoff, "Beyond the Third Dimension, Geometry, Computer Graphic 
and Higher Dimensions", Sci Amer. Library, 1990.

A.K. Dewdney, "Hypercubes", Scientific American, Vol. 254, Nr. 4 (april 1986),
 pp. 8 - 13.

Steve Hollasch, "Four-Space Visualisation of 4D Objects", M. Sc. Thesis, 
Arizona State Univ., 1991.

Rudy Rucker, "Geometry, Relativity and the Fourth Dimension", Dover Books, 
1977.

Rudy Rucker, "The Fourth Dimension, and How to Get There", Penguin, UK,
1986. I don't know the American publisher.
 
Jeffrey R. Weeks, "The Shape of Space, How to Visualize Surfaces and 
Three-Dimensional Manifolds", Marcel Dekker, Inc., New York, 1985.


Pielou, E.C.
The interpretation of ecological data: a primer on classification
and ordination
(Wiley,1984)


D. Asimov, ``The grand tour: a tool for viewing multidimensional data'',
SIAM Journal on Scientific and Statistical Computing, 6 (1985) 128-143.

C. Hurley and A. Buja, ``Analyzing high-dimensional data with motion
graphics'', SIAM J. Sci. Stat. Comp., 11 (1990) 1193-1211.

See the 2-volume set Multidimensional Scaling by the authors
(I think) Shepard, Kruskal, and Nerlove.


Films:

"The Hypercube: Projections and Slicing", prod. Thomas F. Banchoff & Charles 
Strauss, 1978.

"The Hypersphere: Foliation and Projections", prod. Thomas F. Banchoff, 
Huseyin Kocak, David Laidlaw & David Margolis, 1986.


Computer programs:

Steve Hollasch, "ray4-1.00" & "wire4-1.00", ftp swedishchef.lerc.nasa.gov,
directory programs/hollasch-4d

ftp site: search archie for something called xgobi (probably at Purdue)


Also:

A Topological Picturebook by George K. Francis, published by Springer Verlag.




Article 2002 of comp.graphics.visualization:
Newsgroups: comp.graphics.visualization
From: johne@iti.gov.sg (Dr. John S. Eickemeyer)
Subject: Re: References on representing N Dim data

And of course, no reference list about representing multidimensional data 
would be complete without Parallel Coordinates... :)  If you need a general 
method that can represent multivariate relationships in N dimensions, I 
would recommend taking a good look at Parallel Coordinates.  The papers by 
Inselberg are the best place to start...

\bibitem[Cho87]{Cho87} T. Chomut (1987), {\bf Exploratory Data
Analysis Using Parallel Coordinates}, M. Sc. Thesis, UCLA Computer
Science Dept., IBM LA Sc. Cen. Rep. 1987-2811.

\bibitem[DW91]{DW91} A. Desai, L. C. Walters (1991), {\it Graphical
Presentations of Data Envelopment Analyses: Management Implications from
Parallel Axes Representations\/}, Decision Sciences Journal,
{\bf 22-2:} 335-353. 

\bibitem[Eic91]{Eic91} J. S. Eickemeyer (1991), {\bf Visualizing \(p\)-Flats 
in \(N\)-Space Using Parallel Coordinates}, PhD. Thesis, UCLA Computer
Science Dept.

\bibitem[GDCM90]{GDCM90} C. Gennings, K. S. Dawson, W. H. Carter, R. H.
Myers (1990), {\it Interpreting Plots of a Multidimensional Dose-Response
Surface in a Parallel Coordinate System\/}, Biometrics
{\bf 46:} 719-735. 

\bibitem[ID87]{ID87} A. Inselberg, B. Dimsdale (1987), {\it
Parallel Coordinates For Visualizing Multi-Dimensional
Geometry\/}, in {\bf Proceedings of Computer Graphics International
'87} (T. L. Kunii, ed.), Springer-Verlag, Toyko.

\bibitem[ID90]{ID90} A. Inselberg, B. Dimsdale (1990), {\it
Parallel Coordinates: A Tool For Visualizing Multi-Dimensional
Geometry\/}, Proc. IEEE Conf. Visualization '90, 361-378.

\bibitem[IRC87]{IRC87} A. Inselberg, M. Reif \& T. Chomut (1987), {\it
Convexity Algorithms in Parallel Coordinates\/}, Journal of the ACM {\bf
34:} 765-801.

\bibitem[Ins85]{Ins85} A. Inselberg (1985), {\it The Plane with
Parallel Coordinates\/}, Special Issue on {\it Computational
Geometry\/}, The Visual Computer {\bf 1:} 69-91.

\bibitem[Weg90]{Weg90} E. Wegman (1990), {\bf Hyperdimensional Data
Analysis Using Parallel Coordinates}, J. Amer. Stat. Assoc. {\bf 85:}
664-675. 


From: ilana@niwot.scd.ucar.EDU (Ilana Stern)

The best thing would be if you could just ask people to ftp it from the
pit-manager.mit.edu site, because I would rather not be bothered by
people who want it.  The document at csn.org is also a good resource.

Newsgroups: sci.geo.meteorology,news.answers
Subject: Sources of Meteorological Data FAQ
Followup-To: sci.geo.meteorology
Reply-To: ilana@ncar.ucar.edu
Summary: Weather and research data available via Internet, CD-ROM, and tape.
Supersedes: <1992Sep21.155426.25740@ncar.ucar.edu>
Expires: Tue, 20 Oct 1992 07:00:00 GMT

Archive-name: weather-data
Last-modified: 24 September 1992

Recent changes:
  Addition of liasun3.epfl.ch ftp site
  Addition of IP number to cumulus.met.ed.ac.uk site
  --
  **COMPLETELY NEW FORMAT**
  Addition of Digital Chart of the World CD-ROM
  New information on marlin.jcu.edu.au ftp site
  Addition of delocn.udel.edu ftp site
  New format information for DMSP SSM/I Ice Concentration Grids CD-ROM
  Addition of WX-TALK to mailing list section
  Cleanup of cdiac.esd.ornl.gov ftp site listing

This is a guide to various sources of meteorological, oceanographic,
and geophysical data.  Some of these data types are intended for enjoyment
or hobbyist use;  other data are more research-oriented.  Much of the 
research data is not free.

More information on geological/geographical data can be found in the
FAQ for sci.geo.geology, or see the file available via FTP from csn.org.

This guide is posted every two weeks;  a copy can be obtained by 
anonymous FTP to pit-manager.mit.edu, from the file weather-data in
the directory /pub/usenet/news.answers.  A copy is also maintained in 
vmd.cso.uiuc.edu in the file SOURCES.DOC.

Corrections, additions, and comments should be sent to Ilana Stern at
ilana@ncar.ucar.edu.  **If you plan to redistribute this file to a mailing
list, in another newsgroup, or in a newsletter, PLEASE CONTACT ME FIRST!**

########################################################################

			C O N T E N T S

	  I. Data available over the Internet
	 II. CD-ROM source list
	III. Research data on tape and other media
	 IV. Weather-related mailing lists

########################################################################

Subject: Data available over the Internet

			C O N T E N T S

	1. How to use anonymous FTP 
	2. How to use telnet
	3. Index of FTP and Telnet sites by topic
	  A. Current weather images via FTP
	  B. Current weather data via telnet
	  C. Meteorological, oceanographic, and geophysical research data
	  D. Other satellite images
	  E. Map data
	  F. Other stuff
	4. Alphabetical list of FTP and Telnet sites, with information

1. How to use anonymous FTP 

FTP (File Transfer Protocol) allows transfer of files between two computers
which are on the Internet.  To access the FTP areas listed here, at your
system prompt type "ftp" followed by the name or IP number (the number
in brackets next to the system name in the listing below) of the desired
system.  For example, to access vmd.cso.uiuc.edu you'd type 

	ftp vmd.cso.uiuc.edu
or
	ftp 128.174.5.98

Use "anonymous" as your login and your email address as the password (if 
requested).  

[Note: quotes ("like this") are used to set off names of directories and
files, or commands you'd type, and are not part of these names.]

Not all FTP systems accept the same commands, but here's a list of the
most useful:

	ls	list files in the current directory.
	cd	change directory, e.g. "cd wx" changes to the wx directory.
	binary	sets binary mode; USE THIS FOR RETRIEVING IMAGES!
	ascii	sets ascii mode (the default).  Use for retrieving text.
	get	retrieves a file, e.g. "get readme" gets a file called readme.
	bye	exits FTP.


2. How to use telnet

Type "telnet" followed by the name or IP number (the number in brackets next
to the system name in the listing below) of the desired system.  These
publicly accessible systems generally allow you to log in but put you in
a restricted shell, from which only a certain menu of commands is available.


3. Index of FTP and Telnet sites by topic

This index lists the names of FTP and Telnet sites of interest, with only
a brief blurb as to their contents.  Section 4 gives more information about
each of these sites.  Some sites appear more than once under different
subject headings.

	A. Current weather images 

ats.orst.edu        		GOES vis/IR images of North, Central America
aurelie.soest.hawaii.edu        SST data from AVHRR on NOAA-11, NOAA-12
cumulus.met.ed.ac.uk		Meteosat vis/IR images of Europe
liasun3.epfl.ch			Meteosat vis/IR images of Europe
marlin.jcu.edu.au    		GMS-4 images of Australia, TOGA/COARE area
unidata.ucar.edu      		Surface maps (US, Europe, China), soundings
uriacc.uri.edu         		NOAA-11 images of the northeast US
vmd.cso.uiuc.edu        	GOES-7 vis/IR images, surface analyses over US

	B. Current weather data 
	
ats.orst.edu 			Some US city and Oregon weather forecasts
hermes.merit.edu        	US weather forecasts, global reports
madlab.sprl.umich.edu 3000 	US weather forecasts, global reports 
ncardata.ucar.edu		Colorado weather forecasts

	C. Meteorological, oceanographic, and geophysical research data

cdiac.esd.ornl.gov     		Info on climate change topics
ncardata.ucar.edu       	Info on datasets available from NCAR
nssdca.gsfc.nasa.gov		Info on datasets available from NSSDC
storm.mmm.ucar.edu		STORM-FEST data
pioneer.unm.edu       		Data and software from various CD-ROMs

	D. Other satellite images

ames.arc.nasa.gov		Various earth-from-space images
pioneer.unm.edu 		Various images taken from CD-ROMs 
sanddunes.scd.ucar.edu		AVHRR images of USA via telnet
snow.nohrsc.nws.gov		Snow cover maps of US from GOES
sseop.jsc.nasa.gov   		Pictures taken from the space shuttle

	E. Map data

csn.org                 	Mapping software and datasets
hanauma.stanford.edu   		CIA World Bank database, 0.5 deg elev dataset
ncardata.ucar.edu		Elevation data
pioneer.unm.edu 		World atlas, census data, others
spectrum.xerox.com     		Various USGS data 

	F. Other stuff

csn.org                 	Information on other Internet resources
delocn.udel.edu			Software for oceanographic computations
ncardata.ucar.edu		Script to retrieve vmd.cso.uiuc.edu GIFs
pioneer.unm.edu			Image display software
vmd.cso.uiuc.edu		Documents on weather-related topics


4. Alphabetical list of FTP and Telnet sites, with information

This section provides expanded listings of the sites in the previous
section.  Remember to set the transfer type to "binary" when retrieving
images!  

ames.arc.nasa.gov					(FTP)
  Change directory to "SPACE/CDROM".  Images from Magellan and Viking 
missions, other stuff.

ats.orst.edu  		[128.193.120.19]		(FTP)
  GOES IR and VIS images over North and Central America, plus a "floater" 
image which "could be anything."  Also Oregon and US city forecasts.

aurelie.soest.hawaii.edu	[128.171.151.121]	(FTP)
  Sea-Surface-Temperature data (near-real-time) in the directory
"pub/avhrr/images".  AVHRR images within the radius of reception of the 
university's HRPT station, approximately 5 S to 45 N and 125 W to 165 E.  
The processed images are available usually within 30 min. of NOAA-11 and 
NOAA-12 passages.  Data are compressed binary in netCDF format (get 
documentation from unidata.ucar.edu FTP site) labelled by satellite name 
(n11/n12) and time.  More info available from hrpt@hokulea.soest.hawaii.edu.

cdiac.esd.ornl.gov 	[128.219.24.36]  		(FTP)
  Contains data and information on general and technical aspects of 
carbon dioxide, methane, and other trace gas emissions; the carbon cycle; 
and other climate-change topics from CDIAC (the Carbon Dioxide Information 
Analysis Center, address in section 3).  The data for CDIAC's "Trends 91: 
A Compendium of Data on Global Change" is also available here.  (Contact 
CDIAC at cdp@stc10.ctd.ornl.gov to obtain a copy of the book.)

csn.org			[128.138.213.21]		(FTP)
  Change directory to "COGS".  A large, frequently updated file containing 
detailed information on FTP sites, Bitnet and Usenet discussion groups, 
and data sources is located in the file "internet.resources.earth.sci".
This file contains more information on mapping, GIS, remote sensing, and 
geology, subjects which are mostly outside the scope of this meteorology-
oriented FAQ.  Mapping software and datasets are also available in this 
directory.  Contact bthoen@csn.org (Bill Thoen) for more information.

cumulus.met.ed.ac.uk	[129.215.168.19]		(FTP)
  Change directory to "images".  IR and visible images of Europe from 
Meteosat, twice daily, in 1152 x 900 GIF format (size of Sun root window).  
The subdirectory "gifs" has smaller 3x daily images of the Nordic areas, 
the UK, and Europe.

delocn.udel.edu						(FTP)
  Change directory to "FORTRAN".  Programs to do various oceanographic 
computations.  Inquiries and calls for help can be addressed to 
walt@delocn.udel.edu.

hanauma.stanford.edu	[36.51.0.16]			(FTP)
  The CIA World Bank database contains coastlines, rivers and political 
boundaries.  An 0.5 degree elevation dataset is also there.  A program for 
decoding the CIA data can be found as "mfil" on pi1.arc.umn.edu 
[137.66.130.11]  (Info from ken@msc.edu)

hermes.merit.edu	[35.1.48.150]			(Telnet)
  Type um-weather at the "Which Host?" prompt and use menus. 
(Connects to madlab.sprl.umich.edu)

liasun3.epfl.ch						(FTP)
  Change directory to "pub/weather".  IR and visible images of Europe
from Meteosat, in GIF format.  It appears that this site contains
the same images as cumulus.met.ed.ac.uk.

madlab.sprl.umich.edu 3000	[141.212.196.79]	(Telnet)
  Include the "3000" when connecting to the machine.  This is a menu driven
system which has a large variety of information, including US and Canadian
weather forecasts, ski conditions, earthquake reports, severe weather
reports, and current weather conditions for some international cities.

marlin.jcu.edu.au 	[137.219.16.14]			(FTP)
  Change directory to "JCUMetSat". GMS-4 images updated regularly for 
various Australian states, Australia as a whole, the globe, the TOGA/COARE 
area, and events of interest such as cyclones. The images are in a format 
designed for the package JCUMetSat on Amiga computers, but can be converted 
to GIF format using the ALCHEMY software (shareware) available at this site.  
(More information on the format and images can be obtained from Professor 
C.J. Kikkert, eecjk@marlin.jcu.edu.au.)

ncardata.ucar.edu	[128.117.8.111]			(FTP)
  Information on datasets available from NCAR (the National Center for 
Atmospheric Research), and a few small datasets.  If you would like to 
order data after browsing this information, email to datahelp@ncar.ucar.edu.  
Small datasets can be provided by FTP;  we also write various kinds of tapes.  
See the README file.
  A shell archive containing scripts to retrieve GIFs from vmd.cso.uiuc.edu,
get_gifs, is located in the "weather" subdirectory.  This subdirectory also
contains Colorado weather and ski reports.
  A few special datasets are located in the FTP area, and are free.  They
are described in the file "pricing".  These include a 1 deg resolution
elevation dataset, a continental outline dataset, and a list of all WMO
stations with latitude, longitude, and elevation.

nssdca.gsfc.nasa.gov					(FTP or Telnet)
  Telnet:  The National Space Science Data Center (NSSDC) On-Line Data and 
Information Service (NODIS) is a menu-driven interactive system which provides
information on services and data supported by NSSDC.  Login as NSSDC.  Some
topics:  Nimbus-7 GRID TOMS Data, Geophysical Models, Standards and 
Technology Information System.
  FTP: some information and actual data is also available via anonymous FTP.

pioneer.unm.edu		[129.24.9.217]			(FTP)
  Change directory to "pub/info" and retrieve beginner-info, cd-list,
newcd-list, and cd-schedule to get started.  This machine is part of the
Space and Planetary Image Facility (SPIF), sponsored by the Computer and 
Information Resource Technology group at UNM;  it currently has 3 CD readers
and expects to add more.  You can use this machine to FTP data and software
from a variety of CD-ROMs, including both research data and images.  There
is no charge for this service.  Contact help@pioneer.unm.edu for more 
information.  

sanddunes.scd.ucar.edu					(Telnet)
  AVHRR (Advanced Very High Resolution Radiometer) images from 1989 through
7 Jan 1992 cover CO, WY, KS, NE, and NM, as well as parts of AZ, UT, OK,
and TX.  Since 7 Jan 1992, coverage includes these plus CA, OR, NV, WA,
and MT, to 1000 km off Pacific coast.  Total coverage of US for 1989-present
will be available soon.  West coast data from 1980-1985 will be available
some time this year.
  Images are 1024 lines x 1024 elements before 7 Jan 1992, 2560 lines x
1024 elements after.  Images are 1 km resolution and 8-bit format.
  Contact Tim Kelley by email kelley@sanddunes.scd.ucar.edu or telephone 
303/497-1221 for login, password, and manual.  Service is free to Internet 
users and is funded by NASA.

snow.nohrsc.nws.gov 	[192.46.108.1]  		(FTP)
  Change directory to "snow". Various snow-related images in GIF form.  
US snow cover map updated weekly.  JPEG of current AVHRR images.  Contact 
tim@snow.nohrsc.nws.gov (Tim Szeliga) for more info.

spectrum.xerox.com	[192.70.225.78]			(FTP)
  Various USGS data in subdirectories under the directory "pub/map".

sseop.jsc.nasa.gov	[146.154.11.34]			(FTP)
  Many pictures taken from the space shuttle.  Files are in a 512x512 
format as red, green, and blue bitmaps. Image files are binary format, 
and have .DAT as an extension. 

storm.mmm.ucar.edu	[128.117.88.53]			(FTP)
  Hourly and 5-minute composite surface observations, and composite 
rawinsonde soundings, from STORM-FEST, in the directories "/fest/hrly_sfc", 
"fest/5min_sfc", and "/fest/sounding", respectively.  There is one file per 
day. The data are in ASCII.  This data is a preliminary release. 
  This FTP system will eventually be replaced by a different data access
system, although the data will still be available via the new system.
(Info from Mark Bradford, bradfrd2@ncar.ucar.edu)

unidata.ucar.edu	[128.117.140.3]			(FTP)
  Change directory to "images". Weather radar summary map GIFS, surface maps 
for various places, a few soundings on skew-t log-p diagrams, GOES Hugo images 
(in subdirectory "images/hugo").  Surface maps include Europe and China.

uriacc.uri.edu		[131.128.1.1]			(FTP)
  Change directory to "davet.195".  Images of the northeast US in GIF format 
from the afternoon passes of NOAA-11.  (Provided by Dave Tetreault, 
DAVET@uriacc.uri.edu.)

vmd.cso.uiuc.edu 	[128.174.5.98]			(FTP)
  Change directory to "wx".  GOES-7 visible and IR images over the US and 
Mexico, and surface analyses over the US, are available in GIF format.  A 
script to retrieve GIFs automatically is available from the ncardata.ucar.edu 
FTP area.
  Also available in this directory are many useful documents, including
SPOTFREQ.DOC and CHASE-TV.DOC, lists of ham radio frequencies and TV 
stations which carry useful info for storm chasers, WX-PUBS.DOC, which is
a list of weather-related publications, WX-TALK.DOC, which gives information
on the WX-**** mailing lists, and many others. 

########################################################################

Subject: CD-ROM source list

			C O N T E N T S

	1. Basic information
	2. List of CD-ROMs by topic, with summaries
	  A. Weather data
	  B. Research data
	  C. Miscellaneous 

1. Basic information

CD-ROMs tend to be relatively expensive, but can hold as much as 600 megabytes
of data.  Prices are current as of October 1991;  prices for some discs 
are not known.  Some discs are provided with driving software.  Most of
the software is for IBM-PC or compatible systems, but some is available
for the Macintosh, and, increasingly, for Unix systems.

Some of these listings are not for CD-ROMs, but are for floppies or
tapes.  These are listed here, rather than in the section on data available
on other media, because they have been prepared as a package.  The 
research data available on tape is generally copied from a computer
archive as requests come in.  

Commercial sources are flagged as such.  Inclusion of a commercial
source in this listing does not imply endorsement.  

2. List of CD-ROMs by topic, with summaries

	  A. Weather data

Climate Change Data ($950, or 595 pounds sterling from UK source):
  Monthly 5-degree surface temperature anomaly grids 1854-1990, pressure 
grids 1873-1990.  Monthly world temperature data at about 3500 stations and
precipitation data at about 6500 stations, for period of record (long).
Retrieval and mapping software included, available for various systems.
  Contact:  Dr. Phil Jones, Climatic Research Unit, University of East
Anglia, Norwich NR4 7TJ United Kingdom.  Distributed in North America by
Chadwyck-Healey Inc.,1101 King St, Alexandria, VA 22314.  800/752-0515.

World Weather Disc ($295):
  Monthly temp, precip, pressure, sunshine data for about 2000 world stations 
for period of record.  Daily weather data at hundreds of US stations.  Data 
for some stations on temp, precip, freeze, drought, soil moisture, wind,
storms.  Frequency and movement of tropical cyclones.
  Contact:  Cliff Mass, Dept. of Atmos. Sci. (AK40), University of Washington,
Seattle, WA  98195.  206/685-0910.

National Climate Info System ($50):
  Monthly temperature, precipitation, Palmer drought index data for 344
climate divisions of US.  Data can be viewed in tabular or graphical format.
  Contact:  National Climatic Data Center, Federal Building, Asheville, NC
28801.  704/259-0682.

High Resolution Climatology ($199/variable):  *COMMERCIAL*  (Floppy disk)
  Average monthly climatological values [don't have info as to which
variables] for every 1 square km of the conterminous US for the 30-year
period 1951-1980.  The data are stored as a rectangular matrix for each
state.  Digitized state and county political boundaries are included and
referenced to the climate data sets.  The data are in raster form as ASCII 
or 16-bit binary integers.  This dataset is distributed on 5.25" or 3.5" 
floppy disks. 
  Contact:  ZedX, Inc., P.O. Box 404, Boalsburg, PA  16827-0404.

	  B. Research data

NMC gridpoint dataset ($150):
  Twice daily grids for the Northern Hemisphere at a resolution of about 
381 km.  
  Contact: National Center for Atmospheric Research, PO Box 3000, Boulder, 
CO  80307.  303/497-1219, email datahelp@ncar.ucar.edu.

National Geophysical Data Center (NGDC) discs:
  Various discs available, including:  ice and snow coverage, ocean sediment
drilling data, ionospheric vertical soundings ($100), solar variability 
(sunspots, magnetic field data, flares, tree-ring data -- $100), geophysics
of North America (earthquake data, magnetic fields, topography, gravity,
geopolitical info -- $600), and more.
  Contact:  NGDC, 325 Broadway, Boulder, CO  80303.  303/497-6958.

Global Ocean Temperature and Salinity (2 discs, $80 each or $124/both)
  Temperature and salinity in the world ocean for about 1900-1990, based
on all available XBTs, MBTs, BTs, etc.
  Contact:  National Oceanographic Data Center, NOAA/NESDIS E/OC21, 
Washington, DC  20235.  202/673-5549.

GALE and ERICA datasets (2 discs, price not known):
  GALE (Genesis of Atlantic Lows), 1/15/86-4/15/86:  ship data, raobs,
aircraft, radar, etc off N Carolina coast.  ERICA (Experiment on Rapidly
Intensifying Cyclones over the Atlantic), 12/1/88-2/26/89:  rawinsondes,
aircraft, radar, buoys, satellite data, etc. 
  Contact:  C. Kreitzberg, Dept. of Physics and Atmospheric Science, 
Drexel University, Philadelphia, PA  19104.

GEDEX (Greenhouse Effect Detection Experiment)(price not known):
  Two discs containing surface, upper air, and/or satellite-derived 
measurements of temperature, solar irradiance, clouds, greenhouse
gases, fluxes, albedo, aerosols, ozone, and water vapor, along with
Southern Oscillation Indices and Quasi-Biennial Oscillation statistics.
Many of the data sets provide global coverage.  The spatial resolutions
vary from zonal to 2.5 degree grids.  Some surface station data sets 
span more than 100 years;  most satellite-derived sets cover only the
past 12 years.  Temporal coverage is monthly for most sets.  An update
will be available by June 1992.
  Contact:  NCDS/Goddard Distributed Active Archive Center, Code 935,
Goddard Space Flight Center, Greenbelt, MD  20771.  301/286-3209, email 
NCDSUSO@NSSDCA.GSFC.NASA.GOV.
  A more complete description of these discs may be obtained from 
the ncardata.ucar.edu FTP site, in the file "catalogs/nondss/gedex".

DMSP SSM/I Brightness Temperature Grids for the Polar Regions, volume 1-12, 
9 July 1987 - 30 June 1990 (Price on request):
  Each volume contains 3 months of daily brightness temperature grids.
Sensor is currently flying; one additional CD-ROM volume is produced
approximately every 8 weeks.  Passive microwave brightness temperatures
(7 dual-polarized frequencies ranging from 19.3 to 85.5 GHz.), used
primarily to derive sea ice concentration; Northern and Southern
Hemispheres.  
  Data format: 16-bit raster images (2-byte integers), in "SSM/I grid 
format".  
  Associated software:  Extraction and ice concentration software, IMDISP 
image display program for IBM PC, IMAGIC image display program for the 
Macintosh II.  Software distributed on diskettes.  
  Contact:  World Data Center A for Glaciology [Snow and Ice], National Snow 
and Ice Data Center, University of Colorado, CIRES - Campus Box 449, Boulder, 
CO  80309.   303/492-5171, FAX 303/492-2468, email hanson@kryos.colorado.edu 
(Claire Hanson).

DMSP SSM/I Ice Concentration Grids for the Polar Regions, Volume 1, 
9 July 1987 - 31 December 1989 (Price on request):
  Contains sea ice concentration derived from SSM/I brightness
temperatures, using NASA Team algorithm and J. Comiso algorithm,
for Northern and Southern Hemispheres.  
  Data format:  8-bit raster images (1-byte integers) in "HDF format" 
(software available via anonymous ftp from ftp.ncsa.uiuc.edu).  Grid files 
have NASA PDS (Planetary Data System) header labels.  Additional volumes 
will be produced, for the entire time series.  
  Associated software: Source code used to derive ice concentration from 
brightness temperatures.  IMDISP image display software. Software distributed 
on diskettes.  
  Contact: World Data Center A for Glaciology, information above.

Nimbus-7 SMMR Polar Radiances, Volumes 1-12, 25 October 1978 - 20 August 
1987 (life of SMMR sensor) (Price on request):
  Contains passive microwave brightness temperatures (5 dual-polarized
frequencies ranging from 6.6 to 37 GHz) and derived sea ice concentration
for the Northern and Southern Hemispheres.  
  Data format:  2-byte integers, in single-frequency grids.
  Associated software:  IMDISP image display program (C code) for IBM PC; 
landmask and latitude/longitude overlay (Fortran).  Software distributed on 
IBM PC diskettes.  
  Contact: World Data Center A for Glaciology, information above.

Eastern Arctic Ice, Ocean and Atmosphere Data, Volume 1, CEAREX-1 ($50):
  Contains sea ice acceleration, deformation and stress; hydrography
(CTDs); meteorology; bathymetry; acoustics and ambient noise (sample
data) from Coordinated Eastern Arctic Experiment (CEAREX).  Includes
meteorology from Marginal Ice Zone Experiment (MIZEX), 1983, 1984, 1987.
Experiment location: Arctic Ocean north of Svalbard; Fram Strait, September 
1988 - May 1989.  Amount of data: 460 mbytes.  
  Data format: ASCII files.  Associated software: none.  Additional volumes 
are planned; content not yet determined. 
  Contact: World Data Center A for Glaciology, information above.

NWS/NOHRSC Snow cover data (1990 and 1991, $200 each):
  Airborne snow water equivalent and satellite areal extent of snow cover 
data for 1990 and 1991 are now available on CD-ROM for major portions of the 
U.S.  and southern Canada. The CD-ROMs include: (1) airborne snow water 
equivalent data and the digitized flight line network, (2) calibrated AVHRR 
and GOES satellite data used to map snow cover, (3) the classified snow cover 
images (4) national and regional snow cover image products, and (5) ancillary 
data sets including digital elevation data, digitized NWS basin boundaries, 
and the alphanumeric results of the satellite snow cover mapping by basin and 
by elevation zone.
  Contact:  CD-ROM Snow Cover Data, National Operational Hydrologic Remote
Sensing Center (NOHRSC), Office of Hydrology, National Weather Service,
6301 34th Avenue South: Room 112, Minneapolis, MN 55450-2985.
612/725-3258, FAX 612/725-3338, email tim@snow.nohrsc.nws.gov (Tim Szeliga)

	  C. Miscellaneous 

NASA discs:
  Various discs available, including:  Voyager spacecraft images (12 discs,
under $20 each!), Viking images of Mars, Magellan Venus data, Halley's
comet data (25 discs), excerpts from astronomical catalogs, and more.
  Contact:  NSSDC (NASA Space Science Data Center), Code 933.4, NASA
Goddard Space Flight Center, Greenbelt, MD  20771.  301/286-6695.  They
also publish a free newsletter.

CD-ROM, INC:		*COMMERCIAL*
  Several hundred discs available, including:  "GRIPS 2" high resolution
images of topography, Landsat, vegetation maps, plus software ($49), 
"JEDI" 3 discs full of earth, space, and sea science data intended for
school use ($31), 13 business/economic discs, >50 literature and
entertainment discs, >40 health-related discs, many science discs.
Prices range from $29-$895.  Free catalog available from them.
  Contact:  CD-ROM, Inc, 1667 Cole Blvd. Suite 400, Golden, CO  80401.
303/231-9373, FAX 303/231-9581.

Digital Chart of the World ($200):
  The Digital Chart of the World (DCW) is a comprehensive 1:1,000,000-scale 
vector basemap of the world containing cartographic, attribute, and 
textual data.  It is provided with software that permits the database to 
be accessed, queried, and displayed on PC-class computers.  The primary 
source for the database is the U.S. Defense Mapping Agency (DMA) Operational 
Navigation Chart (ONC) series.  
  There are 4 discs:   (1)North America, (2)Europe/Northern Asia, (3)South 
American/Africa/Antarctica, and (4)Southern Asia/Australia.  The data are 
organized into 17 thematic coverages, including political boundaries and 
ocean coast lines, cities, transportation networks, drainage, land cover, 
and elevation contours.  
  Contact:  USGS Open File Section, Box 25286, Denver, CO  80225. 
303/236-7476.

########################################################################

Subject: Research data on tape and other media

Carbon Dioxide Information Analysis Center (CDIAC):  
  Research and distribution center for data related to carbon dioxide, 
methane, and other trace gas emissions; the carbon cycle; and other 
climate-change topics.  You can access catalog information by FTP (see 
section I).  Datasets are available on various media including CD-ROM and 
magnetic tape.  They also publish a free newsletter.
  Contact: CDIAC, Oak Ridge National Laboratory, P. O. Box 2008, Oak Ridge, 
TN 37831-6335. 615/574-0390, FAX 615/574-2232, email cdp@stc10.ctd.ornl.gov.  

NASA Space Science Data Center (NSSDC):  
  Astronomical and atmospheric data.  You can access catalog information by
FTP or telnet (see section I).  
  Contact: NSSDC, Code 933.4, NASA Goddard Space Flight Center, Greenbelt, 
MD  20771.  301/286-6695. 

National Center for Atmospheric Research (NCAR):
  Over 400 datasets available to the research community on various media.  
You can access catalog information by FTP (see section I).
  Contact: NCAR Data Support Section, PO Box 3000, Boulder, CO  80307.  
303/497-1219, FAX 303/497-1137, email datahelp@ncar.ucar.edu.
  (DISCLAIMER:  NCAR is a non-profit government organization operated by 
UCAR under a grant from the NSF.  Our charges reflect the actual cost of 
data retrieval and magnetic media.  I receive no benefit from you ordering
data.  Please, research-related inquiries only.)

National Climatic Data Center (NCDC):  NCDC, Federal Building, Asheville, 
NC 28801.  704/259-0682.

National Geophysical Data Center (NGDC):  NGDC, 325 Broadway, Boulder, 
CO  80303.  303/497-6958.

########################################################################

Subject: Weather-related mailing lists

1. CLIMLIST (moderated by John Arnfield)

  CLIMLIST is a moderated electronic mail distribution list for climat-
ologists and those working in closely-related fields.  It is used to
disseminate notices regarding conferences and workshops, data avail-
ability, calls for papers, positions available etc, as well as requests
for information.  An updated directory of email addresses for the 
subscribers to the list is distributed every month (usually on the 15th).
  To subscribe, mail to whichever of these addresses works for you:
  AJA+@OHSTMAIL.BITNET / aja+@osu.edu / johna@magnus.acs.ohio-state.edu
with the following information:
  Your name (for directory listing), email address, institutional affiliation;
  Indicate if your email address is shared, so your name will be in header
    of messages.
  If your 'climatological credentials' are not apparent from your
  affiliation, please explain.

2. Weather-users (administered by scott@zorch.sf-bay.org)

  This list is for discussions of weather servers; sharing of code to 
automatically query weather servers; and announcements of availability 
(or lack thereof) and changes to weather servers.  Initially, Jeff Masters 
(sdm@madlab.sprl.umich.edu) has agreed to send Weather Underground status 
notices to this list.
To join or quit the list, email to weather-users-request@zorch.sf-bay.org;
the list mail address is weather-users@zorch.sf-bay.org.

3. WX-TALK and other WX-lists

  WX-TALK, formerly STORM-L, is a mailing list for weather-related topics, 
special event notifications, job announcements, and administrative
messages.  This list, and other specialized weather-related lists, are
run from the vmd.cso.uiuc.edu (UIUCVMD) machine at Urbana-Champaign, 
Illinois. WX-TALK is for discussions and questions; the others are intended
to distribute information on particular topics, but you should not 
post mail to them.
  To join the list, send a message consisting of the single line
SUB WX-TALK Your Name
to whichever of these addresses works for you:
  LISTSERV@UIUCVMD / LISTSERV@UIUCVMD.BITNET / LISTSERV@VMD.CSO.UIUC.EDU
or uiucuxc!vmd!listserv from uucp.
Contributions should then go to WX-TALK@[working address]
  For more information, and a list of the other WX-lists on vmd.cso.uiuc.edu, 
use anonymous FTP to retrieve the file WX-TALK.DOC from vmd.cso.uiuc.edu 
in the directory "wx".

4. Wxsat (administered by Richard B. Emerson)

  Wxsat resends all NOAA/NESDIS bulletins on polar and geostationary weather 
satellites as well as occasional material on Meteosat.  Bulletins with 
orbital predictions, spacecraft operation schedules, and related messages 
are copied from NOAA.SAT on SCIENCEnet and forwarded to all addresses on 
the list.  The list is configured to accept and broadcast mail from
subscribers to the list at large.  Wxsat does not store or distribute imagery
and is not primarily a "chat" list.  Wxsat is oriented towards users with a
daily operational need for TBUS and related bulletins.
  An archive of roughly 60 days' messages are available for retrieval via
email messages to wxsat-archive@ssg.com.  Send the message "help" in the
text to the archive server for details on how to retrieve the current index
and other files.
  Subscription requests go to wxsat-request@ssg.com.  The service is free 
to all Internet users but donations are accepted as this is a volunteer 
operation.

########################################################################

From rlb@lavalite.asd.sgi.com  Mon Nov 16 16:45:41 1992
Received: from sgi.sgi.com (SGI.COM) by amelia.nas.nasa.gov (5.61/1.34)
	id AA11463; Mon, 16 Nov 92 16:45:41 -0800
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	for @giraffe.asd.sgi.com:eugene@amelia.nas.nasa.gov id AA12827; Mon, 16 Nov 92 16:45:25 -0800
Date: Mon, 16 Nov 92 16:45:25 -0800
From: rlb@lavalite.asd.sgi.com (Bob Brown)
Message-Id: <9211170045.AA12827@lavalite.asd.sgi.com>
To: eugene@amelia.nas.nasa.gov (Eugene N. Miya)
Subject: Re: [l/m 10/15/1992] Shell (1/4) c.g.v.FAQ
Status: R

Gene,
  You list "other platforms" for IBM Explorer.  You might list for
my Explorer that we have contracted with NAG, Ltd., to do DEC, IBM,
HP, and SPARC ports, that the SPARC port was demo'd at Siggraph'92,
and that we have announced agreements with Intel (Paragon) and
Kendal Square Research.  Also, DuPont Pixel will be offering it soon 
on their systems, which are GL accellerators for SPARC machines.

Never did get over to see the ruskie transport; Friday was our
wrap-up day for 2.0 beta.

Bob
---------------
Robert L. Brown
Silicon Graphics, Inc.




Article 973 of comp.graphics.avs:
Newsgroups: comp.graphics.visualization,comp.graphics.avs