Man1 - ppmshadow.1

Table of Contents

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NAME

ppmshadow - add simulated shadows to a PPM image

SYNOPSIS

ppmshadow [*-b* /blur_size/] [*-k*] [*-t*] [*-x* /xoffset/] [*-y* /yoffset/] [/ppmfile/]

DESCRIPTION

This program is part of *Netpbm*(1)

ppmshadow adds a simulated shadow to an image, giving the appearance that the contents of the image float above the page, casting a diffuse shadow on the background. Shadows can either be black, as cast by opaque objects, or translucent, where the shadow takes on the color of the object which casts it. You can specify the crispness of the shadow and its displacement from the image with command line options.

ppmshadow sees your image as a foreground on a background. The background color is whatever color the top left pixel of your image is. The background is all the pixels that are that color and the foreground is everything else. The shadow that ppmshadow generates is a shadow of the foreground, cast on the background.

The shadow is the same size as the foreground, plus some fringes as determined by the -b option. It is truncated to fit in your image. The output image is the same dimensions as the input image.

You can use pamcomp to place a foreground image over a background before running ppmshadow on it. You can use ppmmake to make the background image (just an image of a solid color).

OPTIONS

-b blur_size
Sets the distance of the light source from the image. Larger values move the light source closer, casting a more diffuse shadow, while smaller settings move the light further away, yielding a sharper shadow. blur_size is the number of pixels of fringe there is on the shadow, beyond where the shadow would be if there were no blurring.

The default is 11 pixels.

Note that this option controls only the fringing effect of moving the light source closer to the object. It does not make the shadow grow or shrink as would happpen in the real world if you moved a point light source closer to and further from an object.

-k
Keep the intermediate temporary image files. When debugging, these intermediate files provide many clues as to the source of an error. See for a list of the contents of each file.
-t
Consider the non-background material in the image translucent – it casts shadows of its own color rather than a black shadow, which is default. This often results in fuzzy, difficult-to-read images but in some circumstances may look better.
*-x*/ xoffset/
Specifies the displacement of the light source to the left of the image. Larger settings of xoffset displace the shadow to the right, as would be cast by a light further to the left. If not specified, the horizontal offset is half of /blur_size / (above), to the left.
*-y*/ yoffset/
Specifies the displacement of the light source above the top of the image. Larger settings displace the shadow downward, corresponding to moving the light further above the top of the image. If you don’t specify -y, the vertical offset defaults to the same as the horizontal offset (above), upward.

FILES

Input is a PPM file named by the ppmfile command line argument; if you don’t specify ppmfile, the input is Standard Input.

The output is a PPM file, written to Standard Output.

ppmshadow creates a number of temporary files as it executes. It creates a new directory for them, tmp/ppmshadow*/pid, where pid is the process ID of the *ppmshadow process. If the TMPDIR environment variable is set, ppmshadow creates the directory there instead of /tmp.

In normal operation, ppmshadow deletes each temporary file as soon as it is done with it and leaves no debris around after it completes. To preserve the intermediate files for debugging, use the -k command line option.

The temporary files are:

infile.ppm
A copy of the input.
bgmask.ppm
Positive binary mask
convkernel.ppm
Convolution kernel for blurring shadow
blurred.ppm
Blurred, colored shadow image
blurred2.ppm
Blurred shadow image before coloring
shadow.ppm
Clipped shadow image, offset as requested
background.ppm
Blank image with background of source image
shadow.ppm
Offset shadow
fgmask.ppm
Inverse mask file
justfg.ppm
Just the foreground. Rest is black. Original image times inverse mask.
shadback.ppm
Generated shadow times positive mask
allbutfg.ppm
Everything but the foreground (foreground area is black).

LIMITATIONS

The source image must contain sufficient space on the edges in the direction in which the shadow is cast to contain the shadow – if it doesn’t some of the internal steps may fail. You can usually expand the border of a too-tightly-cropped image with pnmmargin before processing it with ppmshadow.

Black pixels and pixels with the same color as the image background don’t cast a shadow. If this causes unintentional ’holes’ in the shadow, fill the offending areas with a color which differs from black or the background by RGB values of 1, which will be imperceptible to the viewer. Since the comparison is exact, the modified areas will now cast shadows.

The background color of the source image (which is preserved in the output) is deemed to be the color of the pixel at the top left of the input image. If that pixel isn’t part of the background, simply add a one-pixel border at the top of the image, generate the shadow image, then delete the border from it.

If something goes wrong along the way, the error messages from the various Netpbm programs ppmshadow calls will, in general, provide little or no clue as to where ppmshadow went astray. In this case, Specify the -k option and examine the intermediate results in the temporary files (which this option causes to be preserved). If you manually run the commands that ppmshadow runs on these files, you can figure out where the problem is. In problem cases where you want to manually tweak the image generation process along the way, you can keep the intermediate files with the -k * option, modify them appropriately with an image editor, then recombine them with the steps used by the code in *ppmshadow.

See the ppmshadow.doc file in the Netpbm source tree for additional details and examples of the intermediate files and debugging ppmshadow.

Shadows are by default black, as cast by opaque material in the image occluding white light. Use the -t option to simulate translucent material, where the shadow takes on the color of the object that casts it. If the contrast between the image and background is insufficient, the -t option may yield unattractive results which resemble simple blurring of the original image.

Because Netpbm used to have a maximum maxval of 255, which meant that the largest convolution kernel pnmconvol could use was 11 by 11, ppmshadow includes a horrid, CPU-time-burning kludge which, if a blur of greater than 11 is requested, performs an initial convolution with an 11 x 11 kernel, then calls pnmsmooth (which is itself a program that calls pnmconvol with a 3 x 3 kernel) as many times as the requested blur exceeds 11. It’s ugly, but it gets the job done on those rare occasions where you need a blur greater than 11.

If you wish to generate an image at high resolution, then scale it to publication size with pamscale in order to eliminate jagged edges by resampling, it’s best to generate the shadow in the original high resolution image, prior to scaling it down in size. If you scale first and then add the shadow, you’ll get an unsightly jagged stripe between the edge of material and its shadow, due to resampled pixels intermediate between the image and background obscuring the shadow.

EXIT STATUS

ppmshadow returns status 0 if processing was completed without errors, and a nonzero Unix error code if an error prevented generation of output. Some errors may result in the script aborting, usually displaying error messages from various Netpbm components it uses, without returning a nonzero error code. When this happens, the output file will be empty, so be sure to test this if you need to know if the program succeeded.

SEE ALSO

*pnm*(5) , *pnmmargin*(1) , *pnmconvol*(1) , *pamscale*(1) , *pnmsmooth*(1) , *ppm*(5)

AUTHOR

John Walker http://www.fourmilab.ch August 8, 1997

COPYRIGHT

This software is in the public domain. Permission to use, copy, modify, and distribute this software and its documentation for any purpose and without fee is hereby granted, without any conditions or restrictions.

Author: dt

Created: 2022-02-22 Tue 16:34