[comp.graphics] 3D products for Suns: a list of responses

avr@cs.purdue.EDU (Andrew V. Royappa) (02/21/90)

Here is a list of responses I've received about 3D facilities
for Sun workstations, specifically Sun4/Sparc series. I thank
all who responded -- your suggestions were very helpful. I'm
evaluating the various options now, and will get in touch with
you when I decide on something.


Again, if anyone has information on 3D graphics products (software
hardware, or vaporware), for Sun workstations, please let me know.

		Thanks much,

				Andrew Royappa
				{ihnp4, decvax, ucbvax, pur-ee}!purdue!avr
				avr@purdue.edu

(responses are separated by lines of "=")
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X11-3D
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apE
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Facts About the apE Release:
Here are some details about the availability of the apE software:

What is It?

The apE is a software toolkit for visualizing scientific data. It is designed 
to provide the flexibility to examine data in several ways.  Release 1.1 of 
the apE is designed primarily for visualizing data in two graphical 
dimensions. (this does not mean just for visualizing two-dimensional data).  
The apE system places an emphasis on animation and the integration of the 
visualization process into the scientific process.

The apE is extendable, and will grow with the addition of more tools and 
filters. The apE is a software product resulting from leading research in 
computer graphics and scientific visualization conducted by The Ohio 
Supercomputer Graphics Project and the Advanced Computing Center for the 
Arts and Design.  The apE 2.0, available in winter 1989/90, will address 
general visualization problems in both two and three dimensions.

What Computers is it For?

The software package is designed so that there are two types of programs:  
interactive tools, and computational filters. The tools allow for interactive 
manipulation and examination of data. The filters perform all the computations.
The filters are usable without the tools, although the user may need to 
provide some programming support to create data flows and view rendered images.

The complete apE toolkit, including the tools (running under SunView), 
filters, and documentation, is available for the following workstations:

	- Sun series 4 workstations.
	- Sun series 3 workstations, running SunOS version 4.0 or greater.
	- Sun series 386i workstations.


In addition, the filters are available for the following 
computers/workstations running UNIX:

	- Silicon Graphics 4D series workstation.
	- Cray X-MP supercomputer.
	- Hewlett-Packard workstations
	- the NeXT workstation
	- the Convex C-1 superminicomputer.

How Do I Get it?

The apE is available via anonymous ftp from oscsuna.osc.edu (128.146.1.4) in 
the directory pub/apE.  Send electronic mail to michelle@rhett.osgp.osc.edu, 
for more information.


What Does the Release Include?

	- Executable versions of all the programs 
	  (tools and filters) for Sun-4, Sun-3, and Sun 386i.
	- Complete user documentation for each program.
	- Examples and tutorial.
	
Source code for the apE version 1.1 is not available; however, future 
releases will include source code at a nominal fee (<$100).


apE Version 2.0

The apE 2.0 represents a significant release of graphics software and tools 
to the research community.  Built upon the experience of staff members from 
the Ohio Supercomputer Graphics Projects and the Advanced Computing Center 
for the Arts and Design, the apE 2.0 includes software that addresses the 
full range of applications, from science to art.

The apE 2.0 is projected for release in January, 1990, and will be available 
in binary form via anonymous ftp much like the apE 1.1.  However, full 
source code and printed documentation (both user and programmer) will be 
available as well for a nominal fee.  The apE 2.0 will include libraries, 
filters, tools, and applications.

The apE 2.0 will include basis libraries, libraries for manipulating data flow 
structures, and higher level libraries for window system objects (browsers, 
etc.).  In addition to the two dimensional tools for scientific data included 
in the 1.1 release, the apE 2.0 will also include a complete polygonal system,
with data generation, animation, and rendering; several mapping systems from 
scientific data to surface data; a volumetric rendering system; full image 
manipulation and post processing software; a primitive based rendering system 
(sticks, ball, vectors, etc.), ray tracing software, and a full toolset for 
scientific and artistic image creation and manipulation.


Welcome to the apE ftp directory.


All the files needed to install a binary version of the apE software
are contained here.

The file FACTS is general information about apE.

The CONDITIONS file contains copyright information, please read.

The file install_apE.doc is documentation for the install script 'install_apE'.

The rest of the files are compressed tar files containing the apE release.
	apE.tar.Z		- documentation, examples, other files
	bin.sun3.tar.Z		- executables for sun3
	bin.sun4.tar.Z		- executables for sun4
	bin.sun386.tar.Z	- executables for sun386
	lib.sun3.tar.Z		- libraries for sun3
	lib.sun4.tar.Z		- libraries for sun4
	lib.sun386.tar.Z	- libraries for sun386


Copy the 2 install files (install_apE and install_apE.doc), apE.tar.Z,
	and the bin and lib compressed tar files for the type(s) of
	systems you have.

To install apE, go to the directory containing the apE files, and
	follow the instructions in install_apE.doc

When the release is correctly installed, remove the compressed tar files (.Z)


Hints:

(1)  Use binary mode in FTP

(2)  Do the installation for each type of system.


Please send questions to michelle@osgp.osc.edu


	

	                         apE (tm)
                   the animation production Environment
	       Copyright (c) 1989 The Ohio State University

Release 1.1
Conditions of Release

The Ohio State University holds copyright in this software, including 
documentation and screen designs.  Any person may download a copy of 
apE Software Release 1.1 which will be deemed acknowledged by the act of 
downloading all or any portion of such software:

1.  The downloaded software, and any copies or derivatives thereof, will 
    be used solely for research and evaluation, but will not be decompiled, 
    commercialized,or made available to anyone not acknowledging acceptance 
    of these conditions.

2.  Acknowledgment of the source of this software will be included on 
    all copies of it and of any derivatives, including produced works such as 
    still images and films.  The original copyright notice(s) will be retained 
    on all copies, including partial  copies, and appropriate copyright 
    notice(s) will be  placed on all copies of any derivatives.

3.  This apE software and any subsequently released corrections, 
    improvements, or other modifications, is made available as is, without 
    warranty of any kind. WARRANTIES OF MERCHANTABILITY AND 
    OF FITNESS FOR A PARTICULAR PURPOSE ARE EXPRESSLY 
    DISCLAIMED.  Neither the Ohio State University nor anyone in privity 
    with it shall be liable for any loss or damages, including without 
    limitation special, indirect or consequential damages, arising from any 
    use, defect, omission, failure or the like of said software, nor shall 
    they have any obligation to make available any corrections, improvements,
    or other modifications or to provide any assistance or service of any kind.

For terms under which source code, licenses for commercialization and/or 
assistance in developing particular applications can be obtained, please 
contact:

			Michelle Messenger
			The Ohio Supercomputer Graphics Project
			1224 Kinnear Road
			Columbus, Ohio  43212
			(614) 292-3274
			email:  michelle@rhett.osgp.osc.edu
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PV-Wave	
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You will probably want to consider PV-Wave.  Call 303-530-9000 for
more info.
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Sun frame-buffer/bus possibilities
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	4/110, 3/60, 3/80, 3/110 have the P4 bus
	4/260, 3/260, 4/280, 3/280 have the VME bus
	4/330, 3/430 have both P4 and VME buses
	4/60, sparcstation 1, has the S4 bus
	
	CG6, 8 bit accellerated color fb, is P4 and S4 available
	CG2/3/5, 8 bit unaccellerated color fb, is VME
	CG4, 10 bit unaccellerated color and mono fb is P4
	CG3, 8 bit unaccellerated color fb is sun386i and S4
	CG8, 24 bit + overlay unaccellerated is P4
	CG9, 24 bit + GP2 accellerator is VME
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SunPhigs
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SunPhigs works really well on the sparc -- talk to your local Sun rep.
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RenderMan/RasterOps
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Pixar offers it's PhotoRealistic RenderMan product for Sun4/SparcStation.
The emphasis is on image quality, not on speed.

A company call RasterOps Has recently announced a 24-bit framebuffer
for the SparcStation 1.  I have tried Pixar's software on it and it worked
without problems.  The framebuffer is software compatible with Sun's
own CG8 and CG9 24-bit framebuffers.   
This is a quality improvement, it will not improve speed.
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Alliant GX4000
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From: rutgers!market.alliant.com!dud (W.A."Dudley" Gaman)

Alliant makes a PHIGS-based parallel-processor add-on graphics board set
for the Sun3 and Sun4.  We are currently modifying the board set for the
SparcStation.  The board set is known as the GX4000.  The GX4000 provides
the ability to render 1,000,000 vectors and 225,000 shaded polygons per
second with dedicated graphics processors and memory, thus freeing the Sun
CPU for other computational tasks.  The GX4000 uses the ISO/ANSI standard 
PHIGS+ 3-D graphics library as its native instruction set (all PHIGS commands
are processed using Alliant's parallel hardware and firmware).

If you would like more information, please send your address and phone number
and I'll pass along some product brochures.

dud@alliant.com
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And Finally, from a pessimist...
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The bottom line is "don't bother". If you spend the money to put graphics 
hardware (VME-style) into a Sun you could probably have bought an SGI.
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