man/man1/rhpict.1

.\" RCSid "$Id: rhpict.1,v 1.2 2003/12/09 15:59:06 greg Exp $"
.TH RHPICT 1 3/10/99 RADIANCE
.SH NAME
rhpict - render a RADIANCE picture from a holodeck file
.SH SYNOPSIS
.B rhpict
[
.B options
]
.B holodeck
.SH DESCRIPTION
.I Rhpict
generates one or more pictures from the RADIANCE holodeck file
.I holodeck
and sends them to the standard output.
The
.I \-o
option may be used to specify an alternate output file.
Other options specify the viewing parameters and provide
some control over the calculation.
.PP
The view as well as some of the other controls
are shared in common with the
.I rpict(1)
command.
The options that are unique to
.I rhpict
are given first, followed by the more familiar ones.
.TP 10n
.BI -s
Use the smooth resampling algorithm, which amounts to linear interpolation
between ray samples with additional edge detection along color and object
boundaries.
This is the default.
.TP
.BI -r \ rf
Use random resampling, where
.I rf
is a fraction from 0 to 1 indicating the desired degree of randomness.
A random fraction of 0 is not the same as smooth resampling,
because there is no linear interpolation, just Voronoi regions.
Values greater than 1 produce interesting underwater effects.
.TP
.BI -x \ res
Set the maximum x resolution to
.I res.
.TP
.BI -y \ res
Set the maximum y resolution to
.I res.
.TP
.BI -pa \ rat
Set the pixel aspect ratio (height over width) to
.I rat.
Either the x or the y resolution will be reduced so that the pixels have
this ratio for the specified view.
If
.I rat
is zero, then the x and y resolutions will adhere to the given maxima.
.TP
.BI -pe \ expval
Set the exposure value for the output pictures to
.I expval.
Since filtering is performed by
.I rhpict,
there is little sense in passing the output through
.I pfilt(1),
other than changing the exposure.
This option eliminates that need.
The value may be specified either as a multiplier, or as a number
f-stops preceeded by a '+' or '-' character.
.TP
.BI -vt t
Set view type to
.I t.
If
.I t
is 'v', a perspective view is selected.
If
.I t
is 'l', a parallel view is used.
A cylindrical panorma may be selected by setting
.I t
to the letter 'c'.
This view is like a standard perspective vertically, but projected
on a cylinder horizontally (like a soupcan's-eye view).
Two fisheye views are provided as well; 'h' yields a hemispherical fisheye
view and 'a' results in angular fisheye distortion.
A hemispherical fisheye is a projection of the hemisphere onto a circle.
The maximum view angle for this type is 180 degrees.
An angular fisheye view is defined such that distance from the center of
the image is proportional to the angle from the central view direction.
An angular fisheye can display a full 360 degrees.
Note that there is no space between the view type
option and its single letter argument.
.TP
.BI -vp " x y z"
Set the view point to
.I "x y z".
This is the focal point of a perspective view or the
center of a parallel projection.
.TP
.BI -vd " xd yd zd"
Set the view direction vector to
.I "xd yd zd".
.TP
.BI -vu " xd yd zd"
Set the view up vector (vertical direction) to
.I "xd yd zd".
.TP
.BI -vh \ val
Set the view horizontal size to
.I val.
For a perspective projection (including fisheye views),
.I val
is the horizontal field of view (in degrees).
For a parallel projection,
.I val
is the view width in world coordinates.
.TP
.BI -vv \ val
Set the view vertical size to
.I val.
.TP
.BI -vo \ val
Set the view fore clipping plane at a distance of
.I val
from the view point.
The plane will be perpendicular to the view direction for
perspective and parallel view types.
For fisheye view types, the clipping plane is actually a clipping
sphere, centered on the view point with radius
.I val.
Objects in front of this imaginary surface will not be visible.
This may be useful for seeing through walls (to get a longer
perspective from an exterior view point) or for incremental
rendering.
A value of zero implies no foreground clipping.
A negative value produces some interesting effects, since it creates an
inverted image for objects behind the viewpoint.
This possibility is provided mostly for the purpose of rendering
stereographic holograms.
.TP
.BI -va \ val
Set the view aft clipping plane at a distance of
.I val
from the view point.
Like the view fore plane, it will be perpendicular to the view
direction for perspective and parallel view types.
For fisheye view types, the clipping plane is actually a clipping
sphere, centered on the view point with radius
.I val.
Objects behind this imaginary surface will not be visible.
A value of zero means no aft clipping, and is the only way to see
infinitely distant objects such as the sky.
.TP
.BI -vs \ val
Set the view shift to
.I val.
This is the amount the actual image will be shifted to the right of
the specified view.
This is option is useful for generating skewed perspectives or
rendering an image a piece at a time.
A value of 1 means that the rendered image starts just to the right of
the normal view.
A value of -1 would be to the left.
Larger or fractional values are permitted as well.
.TP
.BI -vl \ val
Set the view lift to
.I val.
This is the amount the actual image will be lifted up from the
specified view, similar to the
.I \-vs
option.
.TP
.BI -vf \ file
Get view parameters from
.I file,
which may be a picture or a file created by rvu (with the "view" command).
.TP
.BI -S \ seqstart
Instead of generating a single picture based only on the view
parameters given on the command line, this option causes
.I rhpict
to read view options from the standard input and for each line
containing a valid view specification, generate a corresponding
picture.
.I Seqstart
is a positive integer that will be associated with the first output
frame, and incremented for successive output frames.
By default, each frame is concatenated to the output stream, but it
is possible to change this action using the
.I \-o
option (described below).
Multiple frames may be later extracted from a single output stream using the
.I ra_rgbe(1)
command.
.TP
.BI -o \ fspec
Send the picture(s) to the file(s) given by
.I fspec
instead of the standard output.
If this option is used in combination with
.I \-S
and
.I fspec
contains an integer field for
.I printf(3)
(eg., "%03d") then the actual output file name will include
the current frame number.
.TP
.BR \-w
Turn off warning messages.
.SH EXAMPLE
rhpict -vp 10 5 3 -vd 1 -.5 0 scene.hdk > scene.pic
.PP
rpict -S 1 -o frame%02d.pic scene.hdk < keyframes.vf
.SH AUTHOR
Greg Ward
.SH "SEE ALSO"
getinfo(1), pfilt(1), pinterp(1),
printf(3), ra_rgbe(1), rholo(1), rpict(1), rvu(1)
Revision:	1.3
Committed:	Thu Jan 1 19:31:45 2004 UTC (20 years, 4 months ago) by greg
Branch:	MAIN
CVS Tags:	rad3R7P2, rad3R7P1, rad3R6, rad3R6P1, rad3R8
Changes since 1.2:	+3 -3 lines
Log Message:	Renamed rview, lam, calc, and neat to rvu, rlam, icalc, and neaten
#	Content
1	.\" RCSid "$Id: rhpict.1,v 1.2 2003/12/09 15:59:06 greg Exp $"
2	.TH RHPICT 1 3/10/99 RADIANCE
3	.SH NAME
4	rhpict - render a RADIANCE picture from a holodeck file
5	.SH SYNOPSIS
6	.B rhpict
7	[
8	.B options
9	]
10	.B holodeck
11	.SH DESCRIPTION
12	.I Rhpict
13	generates one or more pictures from the RADIANCE holodeck file
14	.I holodeck
15	and sends them to the standard output.
16	The
17	.I \-o
18	option may be used to specify an alternate output file.
19	Other options specify the viewing parameters and provide
20	some control over the calculation.
21	.PP
22	The view as well as some of the other controls
23	are shared in common with the
24	.I rpict(1)
25	command.
26	The options that are unique to
27	.I rhpict
28	are given first, followed by the more familiar ones.
29	.TP 10n
30	.BI -s
31	Use the smooth resampling algorithm, which amounts to linear interpolation
32	between ray samples with additional edge detection along color and object
33	boundaries.
34	This is the default.
35	.TP
36	.BI -r \ rf
37	Use random resampling, where
38	.I rf
39	is a fraction from 0 to 1 indicating the desired degree of randomness.
40	A random fraction of 0 is not the same as smooth resampling,
41	because there is no linear interpolation, just Voronoi regions.
42	Values greater than 1 produce interesting underwater effects.
43	.TP
44	.BI -x \ res
45	Set the maximum x resolution to
46	.I res.
47	.TP
48	.BI -y \ res
49	Set the maximum y resolution to
50	.I res.
51	.TP
52	.BI -pa \ rat
53	Set the pixel aspect ratio (height over width) to
54	.I rat.
55	Either the x or the y resolution will be reduced so that the pixels have
56	this ratio for the specified view.
57	If
58	.I rat
59	is zero, then the x and y resolutions will adhere to the given maxima.
60	.TP
61	.BI -pe \ expval
62	Set the exposure value for the output pictures to
63	.I expval.
64	Since filtering is performed by
65	.I rhpict,
66	there is little sense in passing the output through
67	.I pfilt(1),
68	other than changing the exposure.
69	This option eliminates that need.
70	The value may be specified either as a multiplier, or as a number
71	f-stops preceeded by a '+' or '-' character.
72	.TP
73	.BI -vt t
74	Set view type to
75	.I t.
76	If
77	.I t
78	is 'v', a perspective view is selected.
79	If
80	.I t
81	is 'l', a parallel view is used.
82	A cylindrical panorma may be selected by setting
83	.I t
84	to the letter 'c'.
85	This view is like a standard perspective vertically, but projected
86	on a cylinder horizontally (like a soupcan's-eye view).
87	Two fisheye views are provided as well; 'h' yields a hemispherical fisheye
88	view and 'a' results in angular fisheye distortion.
89	A hemispherical fisheye is a projection of the hemisphere onto a circle.
90	The maximum view angle for this type is 180 degrees.
91	An angular fisheye view is defined such that distance from the center of
92	the image is proportional to the angle from the central view direction.
93	An angular fisheye can display a full 360 degrees.
94	Note that there is no space between the view type
95	option and its single letter argument.
96	.TP
97	.BI -vp " x y z"
98	Set the view point to
99	.I "x y z".
100	This is the focal point of a perspective view or the
101	center of a parallel projection.
102	.TP
103	.BI -vd " xd yd zd"
104	Set the view direction vector to
105	.I "xd yd zd".
106	.TP
107	.BI -vu " xd yd zd"
108	Set the view up vector (vertical direction) to
109	.I "xd yd zd".
110	.TP
111	.BI -vh \ val
112	Set the view horizontal size to
113	.I val.
114	For a perspective projection (including fisheye views),
115	.I val
116	is the horizontal field of view (in degrees).
117	For a parallel projection,
118	.I val
119	is the view width in world coordinates.
120	.TP
121	.BI -vv \ val
122	Set the view vertical size to
123	.I val.
124	.TP
125	.BI -vo \ val
126	Set the view fore clipping plane at a distance of
127	.I val
128	from the view point.
129	The plane will be perpendicular to the view direction for
130	perspective and parallel view types.
131	For fisheye view types, the clipping plane is actually a clipping
132	sphere, centered on the view point with radius
133	.I val.
134	Objects in front of this imaginary surface will not be visible.
135	This may be useful for seeing through walls (to get a longer
136	perspective from an exterior view point) or for incremental
137	rendering.
138	A value of zero implies no foreground clipping.
139	A negative value produces some interesting effects, since it creates an
140	inverted image for objects behind the viewpoint.
141	This possibility is provided mostly for the purpose of rendering
142	stereographic holograms.
143	.TP
144	.BI -va \ val
145	Set the view aft clipping plane at a distance of
146	.I val
147	from the view point.
148	Like the view fore plane, it will be perpendicular to the view
149	direction for perspective and parallel view types.
150	For fisheye view types, the clipping plane is actually a clipping
151	sphere, centered on the view point with radius
152	.I val.
153	Objects behind this imaginary surface will not be visible.
154	A value of zero means no aft clipping, and is the only way to see
155	infinitely distant objects such as the sky.
156	.TP
157	.BI -vs \ val
158	Set the view shift to
159	.I val.
160	This is the amount the actual image will be shifted to the right of
161	the specified view.
162	This is option is useful for generating skewed perspectives or
163	rendering an image a piece at a time.
164	A value of 1 means that the rendered image starts just to the right of
165	the normal view.
166	A value of -1 would be to the left.
167	Larger or fractional values are permitted as well.
168	.TP
169	.BI -vl \ val
170	Set the view lift to
171	.I val.
172	This is the amount the actual image will be lifted up from the
173	specified view, similar to the
174	.I \-vs
175	option.
176	.TP
177	.BI -vf \ file
178	Get view parameters from
179	.I file,
180	which may be a picture or a file created by rvu (with the "view" command).
181	.TP
182	.BI -S \ seqstart
183	Instead of generating a single picture based only on the view
184	parameters given on the command line, this option causes
185	.I rhpict
186	to read view options from the standard input and for each line
187	containing a valid view specification, generate a corresponding
188	picture.
189	.I Seqstart
190	is a positive integer that will be associated with the first output
191	frame, and incremented for successive output frames.
192	By default, each frame is concatenated to the output stream, but it
193	is possible to change this action using the
194	.I \-o
195	option (described below).
196	Multiple frames may be later extracted from a single output stream using the
197	.I ra_rgbe(1)
198	command.
199	.TP
200	.BI -o \ fspec
201	Send the picture(s) to the file(s) given by
202	.I fspec
203	instead of the standard output.
204	If this option is used in combination with
205	.I \-S
206	and
207	.I fspec
208	contains an integer field for
209	.I printf(3)
210	(eg., "%03d") then the actual output file name will include
211	the current frame number.
212	.TP
213	.BR \-w
214	Turn off warning messages.
215	.SH EXAMPLE
216	rhpict -vp 10 5 3 -vd 1 -.5 0 scene.hdk > scene.pic
217	.PP
218	rpict -S 1 -o frame%02d.pic scene.hdk < keyframes.vf
219	.SH AUTHOR
220	Greg Ward
221	.SH "SEE ALSO"
222	getinfo(1), pfilt(1), pinterp(1),
223	printf(3), ra_rgbe(1), rholo(1), rpict(1), rvu(1)