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.\" RCSid "$Id$" |
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.TH RTPICT 1 3/19/2018 RADIANCE |
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.SH NAME |
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rtpict - generate a RADIANCE picture or layerd image using rtrace |
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rtpict - generate a RADIANCE picture, hyperspectral image, or layers using rtrace |
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.SH SYNOPSIS |
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.B rtpict |
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.B "-n nproc" |
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[ |
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.B -co |
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][ |
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.B "-o[vrxlLRXnNsmM] out_dir" |
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][ |
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.B "-d ref_depth/unit" |
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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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is a script that generates a picture or hyperspectral image |
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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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although a few options are silently ignored, and the |
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.I rtrace(1) |
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.I \-co |
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boolean switch is supported. |
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Options incompatible with multi-processing may generate an error. |
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.PP |
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The |
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.I rtrace(1) |
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.I rtrace |
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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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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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.I pvalue(1), |
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unless the |
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.I \-co+ |
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option is specified and |
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.I \-cs |
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is greater than 3. |
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In this case, a hyperspectral image will be generated for each |
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of the value types, converted by |
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.I rcomb(1) |
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and with its suffix set to ".hsr" rather than ".hdr". |
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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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option should be used to assign the reference (median) depth and units. |
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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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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_normal(1). |
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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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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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or |
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.I "irradiance.hsr" |
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and some other output types become irrelevant |
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(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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destination directory, it will be overwritten with the new data. |
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destination directory, an error will be printed and the command will abort. |
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.SH EXAMPLES |
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To render a scene with four processes: |
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.IP "" .2i |
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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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.PP |
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To render a hyperspectral irradiance image with 18 spectral samples: |
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.IP "" .2i |
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rtpict -vf inside.vf -i+ -cs 18 -co+ scene.oct > scene_inside.hsr |
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.SH AUTHOR |
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Greg Ward |
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.SH "SEE ALSO" |
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getinfo(1), mkpmap(1), oconv(1), pfilt(1), |
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pvalue(1), rad(1), rcode_depth(1), rcode_normal(1), rcode_ident(1), |
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rpiece(1), rpict(1), rsplit(1), rtrace(1), rvu(1), vwrays(1), |
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pvalue(1), rad(1), rcode_depth(1), rcode_norm(1), rcode_ident(1), |
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rcomb(1), rcrop(1), rmtxop(1), |
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rpiece(1), rpict(1), rsplit(1), rtrace(1), rvu(1), rxpiece(1), vwrays(1) |