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- Rayshade and Utah Raster Toolkit slides
- ==============================================================================
-
- Mark Maimone
- Carnegie Mellon School of Computer Science
- mwm@cmu.edu
-
- 3 June 1992
-
- ==============================================================================
-
- This is a collection of 33+ slides I generated to introduce Rayshade (and
- the Utah Raster Toolkit) to my deparment. They won't be right for
- everybody, because I didn't attempt to cover things in great detail; I just
- wanted to whet some appetites. Also, several of the slides are very
- site-specific (enhancements I added, physical location of the code on our
- filesystem, etc). So feel free to pick and choose, and make changes to
- anything. I've provided the text of the slides in LaTeX, and the .ray files
- used to generate the rendered images. If you do quote from them
- extensively, please mention where they came from, that's all I ask.
-
- I used both color and greyscale outputs; color for the actual slides,
- greyscale (in the original) for the photocopies. On my unix system, I
- stored all the greyscale in a "bw" subdirectory, color in a "color"
- subdirectory, and then did a "ln -s color ps" or "ln -s bw ps" to create a
- symbolic link to the appropriate directory. Your mileage may vary, you
- might have to play with the makefile if this doesn't work for you. Of all
- the source files, only two differ between the color and greyscale versions:
- pacbw.ray uses different backgrounds than pac.ray, and camera.bw is an idraw
- drawing with solid lines rather than colored. These exceptions are taken
- care of by the Makefile's in the bw and color directories.
-
- ==============================================================================
- HOW TO MAKE SLIDES
-
- First make sure you've got all the image-generating software:
-
- Rayshade 4.0.0 or later
- Utah Raster Toolkit 3.0
- LaTeX
- enscript [if you don't have this, plug in the name of
- any text->PostScript converter. Hopefully
- it will generate bold, 15point text]
- [optional] GNUplot 3.0
-
- Now you *SHOULDN'T NEED TO DO THIS STEP*, unless you've made changes
- to the .ray files or something. Be aware that this step will invoke GNUplot
- to generate depth.ps.
-
- % cd slides/ray [DON'T DO THIS!!!]
- % make [DON'T DO THIS!!!]
-
- Decide whether you want black and white images or color. For color
- slides, do this:
-
- COLOR % cd slides
- COLOR % ln -s color ps
- COLOR % cd color [or cd ps, doesn't matter]
- COLOR % make
-
- For black and white, do this instead:
-
- B&W % cd slides
- B&W % ln -s bw ps
- B&W % cd bw [or cd ps, doesn't matter]
- B&W % make
-
- This will convert the existing .rle files (and others) into PostScript
- format. Now, if you don't have the "enscript" program, change the file
- slides/Makefile to use a different text-to-PostScript formatter. Finally,
- generate the LaTeX output:
-
- % cd slides
- % make
-
- (ignoring the many warnings about overfull hboxs and such) to give you
- following files:
-
- ray.ps: pages 1-17 of the slides
- page18.ps: page 18
- page19.ps: page 19
- page20.ps: page 20
- urt.ps: pages 21-33 of the slides
-
- You may want to print ray.ps in a fwe different pieces, it'll be 1.7meg in
- black and white and nearly 4meg in color.
-
- ==============================================================================
- EXTENSIONS: The only extensions I mention in these slides are depth map
- generation, and conversion between our local Generalized Image Format (GIL)
- and URT format. The depth map has been incorporated into David Debry's
- 4.0.6enh version of rayshade. Unfortunately, the URT slides are highly
- biased toward comparing the URT with our GIL, so they may not be useful
- outside of CMU. But then again, if you want to contrast the URT with
- *your* local image format, you might get some ideas from them. [send me
- mail if you want the gil2rle.c and rle2gil.c programs themselves]
-
- CHEATING: OK, I cheated somewhat in making these slides. That is, several
- of the renderings aren't *exactly* generated by the sample code. Here are the
- exeptions that I remember:
-
- -- sphere.ray -- (slide 4) -- The sphere has color (although none is
- given in the example text)
- -- ap1.ray, ap2.ray, mancyl.ray, diff.ray -- (slide 5) -- The
- rendered images have a soft-colored background plane (because
- rayshade has a black background by default, which looks terrible
- on an overhead, as you can see from slide 4); the text on the
- slide doesn't mention the background.
- -- depth.plot -- (slides 8,9) -- As is explained in the Z buffer
- (depth map) extension code, I didn't use the output of "rayshade
- -z" directly; rather, it's been filtered through an awk script.
- So the data file "ray/depth.plot" is not *exactly* the output of
- "rayshade -z", but it's pretty darn close. See the code in
- 4.0.6enh for a more complete explanation.
-
- ADDITIONAL SLIDES: When giving a talk, make as many extra slides of
- rendered images as you can. People want to see pretty pictures, not words!
- In particular, I suggest making blown-up versions of pac.rle and
- depthcolor.rle (the first because it's cute, the second because it's hard to
- grasp). There's nothing in the makefile for this, just use:
-
- rletops -h 6 -C pac.rle > pac.ps
-
- or something similar. I'm not going to explain rletops, read the man page.
- They also want to know how long it takes to generate the pictures, so keep
- that in mind too.
-
- REBUILDING THE SLIDES: It can take a while to generate the slides
- initially, because you may have to run rayshade nearly a dozen times to get
- the RLE images. So try not to delete them prematurely!
-
- COMMENTS: Send your comments to me, Mark Maimone, mwm@cmu.edu.
- Unfortunately I'm in thesis mode, so I can't offer to make lots of changes.
- But I'll try to help get you started if I can.
-