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greg |
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.\" RCSid "$Id: rtpict.1,v 1.11 2022/04/11 04:03:36 greg Exp $"
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greg |
1.1 |
.TH RTPICT 1 3/19/2018 RADIANCE
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.SH NAME
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greg |
1.7 |
rtpict - generate a RADIANCE picture or layered image using rtrace
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greg |
1.1 |
.SH SYNOPSIS
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.B rtpict
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.B "-n nproc"
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1.1 |
[
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1.3 |
.B "-o[vrxlLRXnNsmM] out_dir"
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][
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.B "-d ref_depth/unit"
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]
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[
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1.1 |
.B "rpict options"
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]
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[
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.B @file
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]
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.B octree
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.SH DESCRIPTION
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.I Rtpict
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is a script that generates a picture from the RADIANCE scene given in
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.I octree
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and sends it to the standard output, or to a file specified with the
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.I \-o
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option.
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Most options and defaults are the same as
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.I rpict(1),
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although a few switches are silently ignored.
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Options incompatible with multi-processing can generate an error.
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.PP
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The
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.I rtrace(1)
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tool is called with
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.I vwrays(1)
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to perform the actual work.
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This enables the
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.I \-n
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option for multiprocessing on platforms that support it.
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If the
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.I \-n
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option is not specified or is set to 1, then
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.I rpict
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is called directly.
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There is no benefit in setting the number of processes to anything
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greater than the number of virtual cores available on your machine.
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Also, it is very important to set the
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.I \-af
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option if an irradiance cache is being generated;
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otherwise, your speed-up will be far from linear.
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greg |
1.3 |
.PP
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If the
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.I \-o
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option has additional characters corresponding to output types from
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.I rtrace,
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it must be followed by the name of a directory that either exists or
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will be created to contain image layers, one per output type.
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The supported types are listed below, and do not include types that
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are useless or have no convenient representation.
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The table below shows the correspondence between output type and file name
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in the specified directory:
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.sp
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.nf
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v radiance.hdr
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1.4 |
r r_refl.hdr
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x r_unrefl.hdr
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l d_effective.dpt
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L d_firstsurf.dpt
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R d_refl.dpt
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X d_unrefl.dpt
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1.3 |
n perturbed.nrm
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N unperturbed.nrm
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s surface.idx
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m modifier.idx
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M material.idx
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.fi
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.sp
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Different encodings are associated with different data types.
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Color data (from the 'v', 'r', and 'x' types) will be converted to
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a flat RGBE picture by
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.I pvalue(1).
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Distances (from the 'l', 'L', 'R', and 'X' types) will be
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converted to a 16-bit representation by
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.I rcode_depth(1),
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and the
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.I \-d
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1.5 |
option should be used to assign the reference (median) depth and world
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units, which applies to the overall scene.
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greg |
1.3 |
Surface normals (from the 'n' and 'N' types) will be converted
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to a 32-bit representation by
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.I rcode_norm(1).
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Finally, identifiers (from the 's', 'm', and 'M' types) will be
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converted to a 16-bit index format by
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.I rcode_ident(1).
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.PP
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If the
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.I \-i
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option is used to turn on irradiane output, then the picture associated
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with the 'v' type will be renamed
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.I "irradiance.hdr"
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and some other output types become irrelevant (i.e., 'r', 'x', 'R', and 'X').
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If one or more of the associated output files already exists in the
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greg |
1.8 |
destination directory, an error will be printed and the command will abort.
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greg |
1.3 |
.SH EXAMPLES
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greg |
1.1 |
To render a scene with four processes:
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.IP "" .2i
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rtpict -n 4 -vf mypers.vf -ab 1 -af scene.amb scene.oct > scene_pers.hdr
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greg |
1.3 |
.PP
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To render radiance, first surface distance, and normals in a layered image:
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.IP "" .2i
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rtpict -n 8 -vf fish.vf @render.opt -ovLn fisholay scene.oct
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greg |
1.1 |
.SH AUTHOR
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Greg Ward
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.SH "SEE ALSO"
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greg |
1.3 |
getinfo(1), mkpmap(1), oconv(1), pfilt(1),
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greg |
1.12 |
pvalue(1), rad(1), rcode_depth(1), rcode_norm(1), rcode_ident(1),
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greg |
1.9 |
rcrop(1), rpiece(1), rpict(1), rsplit(1), rtrace(1), rvu(1), vwrays(1)
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