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Comparing ray/doc/man/man1/rvu.1 (file contents):
Revision 1.3 by greg, Mon Jun 13 20:07:55 2005 UTC vs.
Revision 1.14 by greg, Fri May 2 23:56:18 2025 UTC

# Line 7 | Line 7 | rvu - generate RADIANCE images interactively
7   [
8   .B "rpict options"
9   ][
10 + .B "\-n nproc"
11 + ][
12   .B "\-o dev"
13   ][
14   .B \-b
# Line 40 | Line 42 | A command argument beginning with an at sign ('@') is
42   replaced by the contents of the given file.
43   The options are the same as for rpict(1), with a few notable exceptions.
44   The
45 < .I "\-r, \-z, \-S, \-P, \-PP"
45 > .I "\-pd, \-r, \-z, \-S, \-P, \-PP"
46   and
47   .I \-t
48   options are not supported, and
# Line 60 | Line 62 | option improves the display on greyscale monitors, and
62   .I \-pe
63   may be used to set an initial exposure value.
64   .PP
65 + The
66 + .I \-n
67 + option may be used to specify multiple processes,
68 + to accelerate rendering.
69 + .PP
70   In the second form, the default values
71   for the options are printed with a brief explanation.
72   In the third form, the list of supported output devices
# Line 152 | Line 159 | Set focus distance for depth-of-field sampling.
159   If a distance in world coordinates is absent, then the cursor
160   is used to choose a point in the scene on which to focus.
161   (The focus distance setting does not affect rendering in
162 < .I rview,
162 > .I rvu,
163   but can be used in
164   .I rpict
165   with the
166   .I \-pd
167   option to simulate depth-of-field on views saved from
168 < .I rview.)
168 > .I rvu.)
169   .TP
170   .BI frame " [ xmin ymin xmax ymax ]"
171   Set frame for refinement.
# Line 200 | Line 207 | was started by
207   .I rad,
208   then the
209   .I rfile
210 < parameter will initially default to the rad input file used.
210 > parameter will initially default to the
211 > .I rad
212 > input file used.
213   .TP
214   .BI move " [ mag [ x y z ] ]"
215   Move camera
# Line 219 | Line 228 | A negative magnification factor decreases the object s
228   The default factor is one.
229   Care must be taken to avoid moving behind or inside other objects.
230   .TP
231 < .BR new
232 < Restart the image.
231 > .BI new " [ nproc ]"
232 > Restart the image, using the specified number of rendering processes.
233   Usually used after the "set" command.
234   .TP
235 + .BI origin " [ forward [ right [up] ] ]"
236 + Move the view origin forward or backwards the distance specified by the
237 + .I forward
238 + argument, along the view direction vector.
239 + If at least two arguments are given, the second distance will be a
240 + .I right
241 + shift, or left if negative relative to the current view direction.
242 + If three arguments are given, the third distance will be a distance of
243 + .I up
244 + along the view up vector, or down if negative.
245 + The view direction and size are unchanged in any of the above cases.
246 + With no arguments, the cursor is used to select the
247 + view origin, and the direction will be determined by the
248 + (reoriented) surface normal.
249 + The view type and size will not be altered, but the up vector
250 + may be changed if the new direction coincides.
251 + .TP
252   .BI pivot " angle [ elev [ mag [ x y z ] ] ]"
253   Similar to the "move" command, but pivots the view about a selected point.
254   The
255   .I angle
256 < is measured in degrees around the view up vector using the right hand rule.
256 > is measured in degrees around the view up vector using the right hand rule,
257 > so a positive value pivots the viewer to the right of the selected point.
258   The optional
259   .I elev
260   is the elevation in degrees from the pivot point; positive raises the view point
# Line 246 | Line 273 | color table selection.
273   .BI rotate " angle [ elev [ mag ] ]"
274   Rotate the camera horizontally by
275   .I angle
276 < degrees.
276 > degrees using the right-hand rule.
277 > A positive value rotates the view towards the left, and a negative value
278 > looks to the right.
279   If an elevation is specified, the camera looks upward
280   .I elev
281   degrees.
# Line 274 | Line 303 | ambient divisions (ad),
303   ambient radius (ar),
304   ambient samples (as),
305   black&white (b),
306 + back face visibility (bv),
307   direct jitter (dj),
308   direct sampling (ds),
309   direct threshold (dt),
# Line 287 | Line 317 | medium eccentricity (mg),
317   medium sampling (ms),
318   pixel sample (ps),
319   pixel threshold (pt),
320 < back face visibility (bv),
321 < random sampling (R),
322 < specular jitter (sj), and
293 < specular threshold (st).
320 > specular jitter (sj),
321 > specular threshold (st), and
322 > uncorrelated sampling (u).
323   Once a variable has been changed, the "new" command can be used
324   to recompute the image with the new parameters.
325   If a program variable is not available here, it may show up under
# Line 337 | Line 366 | Stop the program.
366   The screen will be redrawn when the program resumes.
367   .SH ENVIRONMENT
368   RAYPATH         the directories to check for auxiliary files.
369 + .br
370   DISPLAY_GAMMA           the value to use for monitor gamma correction.
371   .SH AUTHOR
372   Greg Ward
373   .SH "SEE ALSO"
374 < getinfo(1), lookamb(1), oconv(1), pfilt(1), rad(1), rpict(1), rtrace(1)
374 > getinfo(1), lookamb(1), mkpmap(1),
375 > oconv(1), pfilt(1), rad(1), rpict(1), rtpict(1), rtrace(1)

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