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Subject: FAQ: 3-D Information for the Programmer
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O O
---+ +---- F A Q ------------------+ +------- F A Q ---------------+ +---
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---+ +--------------- F A Q -------+ +------------------ F A Q ----+ +---
Contents:
1) General references for 3-d graphics questions.
2) How do I define an object?
3) How do I define space?
4) How do I define position?
5) How do I define orientation?
6) How do I define a velocity?
7) Drawing three-dimensional objects on a two-dimensional screen.
8) Vector Math - Dot Product and Cross-Product.
9) Matrix Math
10) Collisions.
11) Perspective.
12) Z-Buffering & the Painters Algorithm & BSP-Trees.
13) Shading.
14) 3-space clipping.
15) 3-d scanning.
16) Publically available source-code.
17) Books on the topics.
18) Other forums.
19) Current Contents of Archive ftp.csh.rit.edu::/pub/3dfaq
Last update:
03Jan95
What's new?
Added a bunch of new books without net-reviews and a few more http
sites.
Added some information on velocity calculations.
1) General references for 3-d graphics questions.
Well, this FAQ is just getting off the ground. Hopefully it will
touch on most of the bases you need to get started for now, and
hopefully it will expand at least as fast as you need it too. But...
regardless, things you'll want to locate for more help are Matrix
Algebra books, Physics books talking about Eulerian motion, and some
books on the Graphics Hardware you want to program for. The code
examples included in this FAQ will most likely be in C with pseudo-code
in comments.
One of the most popular references, (and one of my favorites), is:
Computer Graphics: Principles and Practice
------------------------------------------
Foley, van Dam, Feiner, and Hughes
Addison Wesley -- Reading, Massachusetts
(c) 1990. ISBN 0-201-12110-7
But, you'll also want to definitely check out the FAQ for
comp.graphics. That FAQ touches mainly on 2-D needs, but some 3-D
aspects are reviewed there, too.
2) How do I define an object?
There are lots of ways to define objects. One of the most commonly
used is the OFF (Object File Format). The OFF toolkit and a library of
objects are available via anonymous ftp from gatekeeper.dec.com -- XXX
??? (I can't find it anymore. I found it here once about 2 years ago,
but I haven't found it since). The format provides easy methods for
extensions and a base set of things you can expect for each object. The
toolkit is a bit bulky, but the file format (in ascii) is easy enough to
parse by hand.
The OFF.aoff file contains information about the object. The most
important one there is the location of the surface specification file
(usually object name.geom). This file also contains other attributes
-
and file names relevant to this object.
The OFF surface specification begins with the number of points, the
number of polygons and the number of segments.
npts nplys nsegs
This line is followed by the floating point coordinates for the points
that make up the object.
x1 y1 z1
x2 y2 z2
x3 y3 z3
.
.
.
x(npts) y(npts) z(npts)
Then, it gets a bit more complicated. The following lines begin with a
number to indicate the number of vertices in this polygon. That number
is followed by that many numbers, one for each vertex. These are given
in an order specified in the .aoff (usually conter-clockwise). So, for
example, a triangle and a pentagon which share a side are shown below.
3 1 3 4
5 2 4 3 6 7
Here is some quick and dirty sample code to read in the .geom file:
struct polygon {
int nvert; /* Number of vertices in this polygon */
int *verts; /* Vertices in this polygon */
};
struct object {
int npts; /* The number of points */
int npolys; /* The number of polygons */
int nsegs; /* The number of segments */
double *point x,*point y,*point z;
- - -
struct polygon *polys;
};
int
read geom file( char *geom file, struct object *obj )
- - -
{
FILE *fp;
int i,j;
if (!(fp = fopen(geom file,"r"))) /* Open the .geom file */
-
return -1;
/* Get header information */
fscanf(fp,"%d %d %d",&obj.npts,&obj.npolys,&obj.nsegs);
/*
** Allocate room for the points.
*/
obj.point x = (double *)malloc(obj.npts*sizeof(double));
-
obj.point y = (double *)malloc(obj.npts*sizeof(double));
-
obj.point z = (double *)malloc(obj.npts*sizeof(double));
-
for (i=0;i triplets, it will
require a fair bit of work on reading them in to turn them into
spherical coordinates. If you're looking to this FAQ for information on
how to define the space your objects will be in, I'd strongly suggest
using rectangular coordinates and some derivative of the OFF-format.
For starters, let me just throw in that while our universe may be
infinite in all directions, that doesn't make for good programming. We
have to limit ourselves to small enough numbers that we can multiply
them together without overflowing them, we can divide them without
crashing our systems, and we can add them without accidentally flipping
a sign bit.
Now, the fun begins. The simplest form of defining the Universe is
to flat out say that the Universe stretches over these coordinates, say
in the bounding box of <-65536, -65536, -65536> to <65536, 65536,
65536>. This is often referred to as a Universal Coordinate system or
an Absolute Coordinate system. Then, each object in the Universe will
be centered about some coordinate in that range. This includes your
viewpoint. Several strategies are available for dealing with the edge
of the Universe. One can make the Universe wrap around so that an
object leaving the cube at < X, Y, 65536> will re-appear in the Universe
at < X, Y, -65536>. Or, one can make objects bounce or stop at the edge
of the Universe. And, given any approach, one can have the edge of the
Universe be transparent or opaque.
In an Absolute Coordinate system, all objects must be shown from
the position of your viewpoint. This involves lots of interesting math
that we'll get into later. But, in general, an objects position with
respect to you is it's absolute position - your absolute position (with
all kinds of hell breaking loose if you can see past the edge of the
Universe). Then, after this position is calculated, it must be rotated
based on your orientation in the Universe.
Another possibility for defining space is a Relative Coordinate
system or a View-Centered Coordinate system. In this sort of system,
the Viewpoint is always at coordinates <0,0,0> and everything else in
the Universe is based relatively to this home position. This causes
funky math to come into play when dealing with velocities of objects,
but... it does wonders for not having to deal with the 'edge of the
Universe'. This is the Schroedinger's cat method of the 'edge of the
Universe'.... in the truest sense of out of sight is out of mind. Small
provisions have to be made if objects aren't to wrap around. But... a
Relative Coordinate system can be used to give the illusion of infinite
space on a finite machine. (Yes, even your 486/66DX is finite).
I'll leave spherical coordinates to a later version if people think
they'll be of use...
4) How do I define position?
Position in an Absolute Coordinate system is easy. Each object has
three coordinates. These are often stored in a data-type called a
vector to abstract further the notion that these numbers belong
together.
typedef struct {
long x;
long y;
long z;
} VECT;
Usually, each object in the Universe is defined about its center with
each coordinate on its surface being centered at its own <0,0,0>. This
helps tremendously in rotating the object, and I would highly recommend
this. Then, the object as a whole is given a position in space. When
it comes time to draw this object, its points' coordinates get added on
to its position.
In a Relative Coordinate system, position is also fairly straight
forward. The view-point always has position VECT={ 0, 0, 0 };. Other
objects follow the same sort of system that they would in Absolute
Coordinate systems.
5) How do I define orientation?
Orientation can be quite tricky. I interchange some of the terms
here quite often. In 3-space, orientation must be defined be two-and-
a-half angles. "Two and a half?" you say. Well, almost everyone uses
three because two just isn't enough, but if you want to be technical,
one of those angles only has to range from 0 - 180 degrees (0 - PI/2
radians).
But, taking that for granted now.... you have to pick an
orientation for your view. I personally prefer to have the X-axis run
from left to right across the center of my screen. I also like to have
the Y-axis run from the bottom of my screen; and I also like to have the
Z-axis running from me straight into my screen. With some tweaking of
plus and minus signs and a bit of re-ordering, all of the math here-in
can be modified to reflect any orientation of the coordinate system.
Some people prefer to have the Y-axis heading into the screen with the
Z-axis going vertically. It's all a matter of how you want to define
stuff.
Given that you've agreed with me that Z can go into the screen,
what 3-angles do you need? (Here's where I stand the biggest chance of
mucking up the terms.) You need roll, pitch, and yaw. (I often mix up
roll and yaw and such... so if you can follow along without getting
locked into my terminology, future FAQ's will correct it.)
Look at your monitor as you're reading this. Now tilt your head so
that your right ear is on your right shoulder. This change in
orientation is roll (or yaw... but I call it roll).
Ok, now sit up straight again. Now bring your chin down to meet
your chest. (Hmmm... LOOK BACK NOW!!!, whew... glad you heard me.)
That motion was pitch.
Ok, now look over your right shoulder keeping your head vertical to
see who's behind you. (LOOK BACK AGAIN!!.) Ok... that was yaw (or
roll, but I call it yaw).
That's the basics. Now, what do I do with them? Well, here's
where a nice book on Matrix Arithmetic will help you out. You have to
use these three angles to make a Transformation matrix. [See the
section on Matrix Math]. Here is a typical method of doing these
transformations: [Note, if you don't have Z going into your screen
you'll have to munge these considerably].
typedef double matrix[4][4];
double sr,sp,sy,cr,cp,cy;
matrix mr, mp, my; /* individual transformations */
matrix s; /* final matrix */
sr = sin( roll ); cr = cos( roll );
sp = sin( pitch ); cp = cos( pitch );
sy = sin( yaw ); cy = cos( yaw );
/* clear all matrixes
** [See the section on Matrix Math]
*/
identity( &mr ); identity( &mp ); identity( &my );
/* prepare roll matrix */
mr[0][0] = mr[1][1] = cr;
mr[1][0] = - (mr[0][1] = sr);
/* prepare pitch matrix */
mp[1][1] = mp[2][2] = cp;
mp[1][2] = - (mp[2][1] = sp);
/* prepare yaw matrix */
my[0][0] = my[2][2] = cy;
my[0][2] = - (my[2][0] = sy);
multiply( &mr, &my, &s );
multiply( &s, &mp, &s );
6) How do I define a velocity?
I've always been annoyed by programs that make it advantageous to run on
a slower machine. A naive view of velocity as n-units per time-
through-this-loop means that things move faster if you get through the
loop faster.
In order to by-pass this problem, you have to keep track of time in
some non-hardware-dependent way. Then, you can define your velocity in
n-units per known-time-unit. For ease of mental calculations, I always
define my velocities in units per second. (In actuality, in programming
in DOS, I define my velocity in n-units per 160/182ths of a second
because I'd rather divide by 16 than 18.2).
Here is some pseudo-code for an object moving along a line....
int x = 0; /* position */
int vx = 10; /* velocity */
int dx;
int err fact = 0;
-
int old time = gettime(); /* in milliseconds for instance */
-
int new time;
-
int elapsed;
for (;;) {
new time = gettime();
-
elapsed = new time - old time;
- -
dx = vx * elapsed + err fact;
-
x += dx/1000;
err fact = dx - (dx/1000)*1000;
-
old time = new time;
- -
}
You can ignore all of the err fact stuff if you like, but then
-
velocities that are much lower than your time frequency could end up
excessively slow or fast.
This approach can be used for each linear velocity (x, y, and z).
But, this approach isn't nearly so good for rotational velocities. I'm
still stewing on the best way to handle them.
7) Drawing three-dimensional objects on a two-dimensional screen.
Modified from comp.graphics FAQ:
"There are many ways to do this. Some approaches map the
viewing rectangle onto the scene, by shooting rays through
each pixel center and assigning color according to the object
hit by the ray. Other approaches map the scene onto the
viewing rectangle, by drawing each object into the region,
keeping track of which object is in front of which.
The mapping mentioned above is also referred to as a
'projection', and the two most popular projections are
perspective projection and parallel projection. For example,
to do a parallel projection of a scene onto a viewing
rectangle, you can just discard the Z coordinate, and 'clip'
the objects to the viewing rectangle (discard portions that
lie outside the region). To do a perspective projection,
dividing each the x and the y by some multiple or the Z-depth
is the usual approach.
For details on 3D rendering, the Foley, van Dam, Feiner and
Hughes book, reading. Chapter 6 is 'Viewing in 3D', and
chapter 15 is 'Visible-Surface Determination'. For more
information go to chapter 16 for shading, chapter 19 for
clipping, and branch out from there."
8) Vector Math - Dot Product and Cross-Product.
Adding and subtracting vectors is as easy as subtracting their
respective parts:
+ =
- =
Scaling vectors is as simple as multiplying each part by a
constant:
S * =
The Dot-Product of two vectors is simply the sum of the products of
their respective parts:
. = A*D + B*E + C*F
Note that this value is not a vector.
The Cross-Product of two vectors is a bit more complex (it is the
determinant of the matrix with the direction vector as the first row,
the first vector as the second row, and the second vector as the third
row):
X =
Note that:
X = -1 * ( X )
-and-
( X ) . = ( X ) . = 0
More later.
9) Matrix Math
The identity matrix is a square matrix (same number of rows as
columns) with all elements {i,j} given by:
{ 1.0 if i == j
m[i][j] = {
{ 0.0 otherwise
Multiplication of matrices:
if X is a matrix that is m rows and n columns (an m-by-n (or mxn) matrix)
and Y is a matrix that is n rows and r columns (nxr), then the product
X * Y ==> m[i][j] = sum{ a=0, a
Perspective is easy: realize that the viewpoint isn't on the
surface of the screen but is some distance back. Then,
[a] convert to a relative coordinate system centered around the
viewpoint, oriented so that x and y are like this:
y
|
----+----x
|
and z is the distance into the screen. Now, divide your coordinates by
z.
That's all.
Ok, sure, you don't really have to call your directions x y and z,
but that's just changing the description which fits the math. And,
sure, you have to decide what to do about things that are "the other
direction from the screen" -- but that's really something different.
And, ok, you have to decide how many game units the viewpoint is,
behind the screen [this is something you add to the z coordinate before
dividing]. And, ok, maybe you want to scale things a bit to make it
look nicer. But none of that is really all that hard to deal with.
What's annoying is that you don't want to do division for every
pixel that you draw on the screen. That means, for instance, that you
might have a line where both ends are off the screen but part of the
line [in the middle] are visible. However, that's related to the
problem of detecting collisions. Or, better yet, clipping. Yeah,
that's it take a look at the section on clipping...
Raul D. Miller n =: p*q NB. prime p, q, e
NB. public e, n, y
y =: n&|&(*&x)^:e 1
x -: n&|&(*&y)^:d 1 NB. 1 < (d*e) +.&<: (p,q)
12) Z-Buffering & the Painters Algorithm & BSP-Trees.
There are several methods available for displaying polygons in a 3-d
object so as to assure that what's behind is behind and what's in front
is in front. Each, however, has its pros and cons. With each of these
methods, it is often useful to implement backface culling. Backface
culling is simply not rendering surfaces which aren't facing you.
The Painter's Algorithm is probably the most intuitive for the
beginner, one of the easiest to implement, and the hardest to get right.
The Painter's Algorithm, quite simply, is Paint the from back to front.
Once it has been determined which polygons will be drawn, it is
necessary to sort them from furthest away to closest. Then, starting
with the furthest polygon and moving to the closest, draw them.
The tricky part of the Painter's Algorithm is determining when one
polygon is closer or farther than another. The closest to satisfactory
method I've found uses this criteria -- Surface A is further away then
surface B if:
1) The furthest point of A is further away than the furthest
point of B.
2) B faces you more directly than A.
3) The closest point of A is further than the closest point of B.
4) Surface B is more "important" than surface A.
These are to be taken in order until a decision is reached. But, I've
yet to find good enough criteria to work well on most objects that
people design. If you keep these criteria in mind when making the
objects, it can help. But, if you're using 3rd party objects, I'd
suggest a different method.
Z-Buffering is a buzzword that's finally come down to reality.
It's been replaced by 'texture-mapping' and 'bump-mapping' and 'realtime
raytracing' as the 'what's fancy' buzzword. Z-buffering is costly in
terms of memory and processing time, but gives beautiful results. If
you've got some freedom with your memory usage and a bit of processor
time to spare, and you're ok with filling your own polygons, then Z-
buffering may be for you.
To Z-buffer, one keeps a 2d-array of numbers (shorts or ints
usually) the same dimensions as the viewport. As each point is
prepared for display, the final value is compared to the Z value already
in the position in the Z-buffer array. If the new Z is less than
the one already in the buffer, the pixel-color is placed in the Screen-
Buffer at position and the new Z is copied into position of
the Z-Buffer.
The expense of Z-Buffering is having to set each element to the
MAX Z VALUE after each frame and keeping track of the Z-value for every
- -
pixel in the Screen Buffer and every pixel in the polygon you're
drawing. In most applications, it is unnecessary to keep track of the
Z-values of any more than the vertices of a polygon.
And, my favorite of the bunch (but the nastiest to store in an
object file, is BSP-trees. BSP-tree stands for Binary Space Partition
tree. They are based the idea that surfaces of most objects don't
change positions relative to each other. Objects whose surfaces change
relative positions cannot be (to my knowledge) easily used with BSP-
trees.
The first step in using BSP-trees is to break up your object into a
'good' object. But, I can't think of a way to describe a 'good' object
without just telling you how to make one. So, here's a general
algorithm for making a BSP-tree object from ye average object:
1) Pick a surface to call the root node.
2) Compare every other surface in the set of surfaces to the
root node.
3) If a surface is In-Front-Of the root node, then put it in
the 'Front Heap'.
If a surface is Behind the root node, then put it in the
'Back Heap'.
If neither of the above is true, chop up the surface into
smaller surfaces that are all either In-Front-Of or Behind
the root node. (This is the tricky bit).
4) Repeat these steps with the 'Front Heap' and the 'Back Heap'.
As an interesting note, I can see no advantage at all to trying to keep
a relatively balanced tree.
Now comes the interesting bit. Now that the object is a 'good'
BSP-tree object, it is time for the drawing algorithm. This is fairly
straight- forward.
1) Compare the root node with you.
2) If you are In-Front-Of the root node,
draw 'Root->Back', then the Root surface, then 'Root->Front'.
If you are Behind the root node,
draw 'Root->Front', then the Root surface (unless you're
backface culling), then 'Root->Back'.
I fully admit that I didn't believe BSP-trees would work when I
first read about them in Foley-van Dam, nor did I believe they would
work after seeing them work for me. Now, three months later, I fully
believe they work, and I can even say I understand why. I may soon
attempt an explanation here, but suffice it for now to say, 'they can be
grokked'.
13) Shading.
Sorry... This is a FAQ in-progress. Will do more later. Please
feel free to send me a paragraph for this section.
14) 3-space clipping.
Sorry... This is a FAQ in-progress. Will do more later. Please
feel free to send me a paragraph for this section.
15) 3-d scanning.
Three dimensional scanning is a verifiable pain. I've only really heard
of three basic techniques. Two of them require the scanned item to be
entirely still, and one of them even destroys the object being scanned.
The first technique I ever saw was in 'The Making of T-2'. An
actor was dressed in tight, dark clothing and a mesh of masking tape was
placed over his body. This mesh was filmed simultaneously from several
different camera positions as the actor walked. The films were then
digitally processed to provide a close model of a person walking. The
amount of work and expense involved in creating the images, registration
of the multiple images, and conversion into 3-space data makes this a
big time investment.
The second technique I saw set the item to be scanned on a
turntable. A laser sensing system or simple armature-stylus were used
to obtain a bump-map along a vertical slice of the item. Then, the item
was rotated 5 degrees and the process repeated. The gives a very
detailed cylindrical bump-map of an item.
The third technique is by far the most interesting I've seen. But,
it is useful mostly only for height-field generation. This method
employs a CAT-scan like approach. First, the object is painted solid
black (or white). Then, the item is dipped in milk (or chocolate syrup)
to a certain depth. A still photo is taken. Then, the item is dipped
further into the liquid. Another still is taken. This is done to
obtain slice view of the item. The photos are then digitally scanned to
locate the boundaries of the items.
16) Publically available source-code.
Well, I've started a collection at ftp.csh.rit.edu::/pub/3dfaq/src.
Feel free to upload relevant stuff (that I can't find on archie in under
twenty minutes). Some other sites of interest:
3d images;
ftp://wuarchive.wustl.edu/graphics/ray
ftp://princeton.edu/pub/Graphics
3d Information:
http://www.mindspring.com/~cwatkins/algor.html
http://archpropplan.auckland.ac.nz/People/Paul/Paul.html
ftp://x2ftp.oulu.fi/pub/msdos/programming/docs/zed3d023.zip
http://www.csh.rit.edu/~pat/misc/3dFaq.html
3d geometry files:
http://archpropplan.auckland.ac.nz/People/Paul/Paul.html
ftp://ftp.kgc.com/pub/mirror/avalon
ray tracers:
ftp://alfred.ccs.carleton.ca/pub/pov-ray
http://www.mindspring.com/~cwatkins/algor.html
stereograms:
ftp://ftp.comlab.ox.ac.uk/pub/Documents/3d
http://enigma.phys.utk.edu/stereo/index.html
ftp://sugrfx.acs.syr.edu/3d/stereograms
Sorry... This is a FAQ in-progress. Will do more later. Please
feel free to send me a paragraph for this section.
17) Books on the topics.
Computer Graphics: Principles and Practice Foley, van Dam, Feiner, and
Hughes; Addison Wesley -- Reading, Massachusetts; (c) 1990. ISBN
0-201-12110-7.
I highly reccomend this book for the person seriously interested in
understanding Computer Graphics concepts for 2-D image-generation
and 3-D representation. As a warning though, if you're struggling
to follow vector math and such, you might not spend the $60-$80
bucks on this one yet.
Computer Graphics Handbook: Geometry and Mathematics, Michael E.
Mortenson. ISBN 0-8311-1002-3
I've never seen this one, but it comes net-recommended. Anyone
care to make a more complete statement?
Programming in 3 Dimensions Christopher D. Watkins and Larry Sharp;
Barnes & Noble. ISBN: 1-55851-220-9 $39.95
I've never seen this book. I've got an ad for it in front of me.
I would guess it's a very low-density version of some of the 3-D
things from Foley. The book boasts sample source code on MS/PC-DOS
floppy included. "This one is for all graphics enthusiasts who
want a detailed look at 3-D graphics and modeling. Also features
discussions of popular ray tracinge methods and computer
animation." [sic]
From: MarsSaxMan@aol.com
You mentioned Watkins & Sharp's book "Programming in 3
Dimensions" in your FAQ... I have this book, so I thought I'd
give you a capsule review.
I like the book overall. It is cleanly written & they give a
pretty good explanation of the mathematics (of course, having
spent eons in advanced math has probably bent my perspective
on what's clear in mathematics). However it doesn't get too
bogged down in theory, which is nice. There are also a bunch
of interesting side issues that get covered, such as fractals,
color cycling, color tables, etc. Complete source code to a
ray tracer, an animation interface to the ray tracer, and some
interesting display hacks are included.
Overall a very practical way to get into 3-D graphics; it's
pretty easy to see how the code could be modified for this or
that purpose. It'll take some work to turn its raytracer into
a Doom engine or whatever but it could be done & would still
be worth it.
Only thing I didn't really like (though this is probably a
natural consequence of the down-to-earth real-world nature of
the book) is that it is a bit too DOS PC specific. I hack
Macintosh so a lot of the graphics code is unusable and some
of the memory things have to be changed; one chapter on VGA
graphics is wasted on me. But overall I think the book is a
good buy. Also it's $39.95, so it's not a bad buy compared to
some other 3-D books I've seen (gacckkk!)
Just thought you might like to know, and maybe have a bit more
filler to stash in the FAQ...
-MarsSaxMan Red Planet Software
And, if you liked that... Christopher Watkins sent me a more complete
book list (most of which follows). Feel free to send me any
personal reviews of any of these books. Like or dislike.
Stereogram Programming Techniques. Christopher D. Watkins and Vincent
P. Mallette (Charles River Media, Inc.), 1995 ISBN: 1-886801-00-2
$34.95 Learning Windows(tm) Programming Using Virtual Reality.
Christopher D. Watkins and Russ Berube (Academic Press
Professional, Inc.), 1994 ISBN: 0-12-737842-1
learning Microsoft Windows(tm) programming by developing a
texturing 3-D game engine and application similar to Wolfenstein
3-D(tm) and the popular game DOOM(tm)
Virtual Reality ExCursions with Programs in C. Christopher D. Watkins
and Stephen R. Marenka (Academic Press Professional, Inc.), 1994
ISBN: 0-12-737865-0 $39.95
produce polygonal 3-D virtual worlds on your PC, understand human
perception issues, near complete list of VR information and
technology sources, includes all source code, includes anaglyph 3-D
glasses
Photorealism and Ray Tracing in C Christopher D. Watkins and Stephen B.
Coy (M&T Books, Inc.), 1992 ISBN: 1-55851-247-0 $44.95
generate photorealistic ray-traced computer graphics, includes all
source code for a photorealistic renderer and assorted fractal (and
other) database generators, includes many 3-D models
Exploring Photorealism and Ray Tracing Christopher D. Watkins, Vincent
Mallette, Stephen R. Marenka and Robert Johnson (M&T Books, Inc.),
1995 ISBN: 1-55851-383-3 $29.95
source code for a beginner's ray tracer, the definitive beginner's
book on ray tracing, faster BOB/VIVID executable than in the
original, Photorealism and Ray Tracing in C book with even more
texture mapping and texturing capabilities, a CD ROMs worth of 3-D
models, worlds and tools, various 3-D modeling tools (blobs,
polygonal, etc.), learn how to raytrace the beautiful quaternion
Julia set fractals (Quaternion -> 4-dimensional object)
Advanced Graphics Programming in C and C++ Roger Stevens and Christopher
D. Watkins (M&T Books, Inc.), 1991 ISBN: 1-55851-171-7 $39.95
beginners book to computer graphics, includes a simple ray tracer,
polygon renderer, and height-field renderer, and fractals, includes
all source code, PASCAL version of this book also available, 1990
18) Other forums.
Sorry... This is a FAQ in-progress. Will do more later. Please
feel free to send me a paragraph for this section.
19) Current Contents of Archive ftp.csh.rit.edu::/pub/3dfaq
2 -rw-r--r-- 1 pat member 219 Apr 2 20:40 README
16 -rw-r--r-- 1 pat member 7787 Mar 28 19:11 DoomTechniques.gz
10 -rw-r--r-- 1 pat member 4243 May 23 12:34 bsp.gz
14 -rw-r--r-- 1 pat vr 6266 Apr 2 20:38 imath.gz
22 -rw-r--r-- 1 pat vr 11262 Apr 2 20:43 imath.tar.gz
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Date this article was posted to GameDev.net: 7/16/1999
(Note that this date does not necessarily correspond to the date the article was written)
See Also:
General Math
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