|
103 | Image format | Definite Bug | 3.70 beta 37 | Very Low | Low | JPEG output does not conform to baseline JFIF standard | Closed | |
3.70 beta 38 |
Task Description
POV-Ray 3.7-generated JPEG image output files do not conform to the JFIF standard. Most importantly, the files written do not use the standard YCbCr color model (they seem to use plain RGB instead), nor do they have a proper JFIF tag.
As a consequence, some software may be unable to read the generated JPEG files properly. In addition, it seems that POV-Ray mixes up the Red and Blue channels.
|
|
134 | Image format | Feature Request | 3.70 beta 37a | Very Low | Low | INI option to overlay render information on output imag ... | Closed | |
|
Task Description
It would be nice to configure an INI option to add render information like render time, date, and input file to output images.
|
|
211 | Image format | Feature Request | 3.70 RC3 | Very Low | Low | Fill blank space with pixels on quit rendering | Closed | |
|
Task Description
It would be nice when quitting a render if the remaining space were filled with empty pixels. That way the partial render will still be viewable in all image apps.
|
|
88 | Image format | Definite Bug | 3.70 beta 36 | Very Low | Low | File output code does not properly handle negative colo ... | Closed | |
3.70 beta 37 |
Task Description
File output code for virtually all file formats performs gamma correction on unclipped color values, which leads to issues when color values happen to be negative for some reason and gamma does not happen to be an integer value such as 1.0 or 2.0. As a consequence, subsequent steps (clipping and converting to integer) apparently produce compiler-dependent results. Compiled with Microsift or Intel compilers, POV-Ray seems to write zero brightness in such cases, while compiled with g++ 4.4 (and possibly other compilers) it seems to write full brightness instead.
(See thread news://news.povray.org:119/4ba819f6@news.povray.org for examples.)
The proper solution should be to apply gamma correction after clipping.
|
|
161 | Image format | Definite Bug | 3.70 beta 38 | Very Low | Medium | error when writing jpg format (linux build) | Closed | |
3.70 release |
Task Description
There is a confirmed bug when writing jpg file format with the current linux build (beta39). when specifying +fj output format the following error occurs:
JPEG parameter struct mismatch: library thinks size is 372, caller expects 376 JPEG parameter struct mismatch: library thinks size is 372, caller expects 376 Render failed
this has been confirmed on ubuntu 10.4 and openSuSe 11.2 (assuming 32 bit version) as openSuSe 11.2 64-bit reports no problem
there has been a proposed fix to ~smp/source/base/image/jpeg.cpp that appears to work, however it requires some additional work to make it a platform (linux) and compiler (gcc) specific fix.
|
|
229 | Image format | Feature Request | 3.70 RC3 | Very Low | Low | Clock value into EXIF data for PNG | Tracked on GitHub | |
|
Task Description
The best time for a picture....
I set the day time and so the position of the sun by “clock=”
Normal I document my source very good, but this time, I forgot the clock seting for the picture of my book cover.
So I would find it very practicall to put the clock value and other setings for rendering into EXIF data of the picture.
|
|
64 | Image format | Feature Request | Not applicable | Very Low | Low | Add "POV-Ray" metatags to images | Closed | |
3.70 beta 41 |
Task Description
Add metatags to output images identifying the file as having been created using POV-Ray.
|
|
101 | Include files | Feature Request | 3.70 beta 36 | Very Low | Low | woodmaps.inc dependency | Closed | |
3.70 beta 38 |
Task Description
woodmaps.inc depends on colors.inc, more specifically the definition of the color “Clear” perhaps a #ifndef colors.inc belongs in woodmaps.inc or probably more correctly changing the call of “Clear” to rgbf 1
|
|
157 | Include files | Definite Bug | 3.70 beta 37a | Very Low | Medium | Warnings when parsing include file provided by distribu ... | Closed | |
3.70 beta 39 |
Task Description
Include file golds.inc still provides warnings when parsed, a shame for a standard include file. (colors.inc is ok, I did not test the other includes)
File '/usr/local/share/povray-3.7/include/golds.inc' line 118: Parse Warning:
Expected pure RGB color expression, unexpected filter and transmit components
will have no effect.
File '/usr/local/share/povray-3.7/include/golds.inc' line 119: Parse Warning:
Expected pure RGB color expression, unexpected filter and transmit components
will have no effect.
File '/usr/local/share/povray-3.7/include/golds.inc' line 129: Parse Warning:
Expected pure RGB color expression, unexpected filter and transmit components
will have no effect.
File '/usr/local/share/povray-3.7/include/golds.inc' line 130: Parse Warning:
Expected pure RGB color expression, unexpected filter and transmit components
will have no effect.
File '/usr/local/share/povray-3.7/include/golds.inc' line 140: Parse Warning:
Expected pure RGB color expression, unexpected filter and transmit components
will have no effect.
File '/usr/local/share/povray-3.7/include/golds.inc' line 141: Parse Warning:
Expected pure RGB color expression, unexpected filter and transmit components
will have no effect.
File '/usr/local/share/povray-3.7/include/golds.inc' line 151: Parse Warning:
Expected pure RGB color expression, unexpected filter and transmit components
will have no effect.
File '/usr/local/share/povray-3.7/include/golds.inc' line 152: Parse Warning:
Expected pure RGB color expression, unexpected filter and transmit components
will have no effect.
File '/usr/local/share/povray-3.7/include/golds.inc' line 162: Parse Warning:
Expected pure RGB color expression, unexpected filter and transmit components
will have no effect.
File '/usr/local/share/povray-3.7/include/golds.inc' line 163: Parse Warning:
Expected pure RGB color expression, unexpected filter and transmit components
will have no effect.
|
|
291 | Include files | Possible Bug | 3.70 RC7 | Very Low | Low | Math.inc: error in VDist function | Closed | |
|
Task Description
Included math.inc into scene and recieved this fatal error from povray:
File '/usr/local/share/povray-3.7/include/math.inc' line 248: Parse Error: Expected 'string expression', float function 'vlength' found instead
Appropriate place in math.inc:
245 > #end
246 >
247 > // Distance between V1 and V2
248 > #macro VDist(V1, V2) vlength(V1 - V2) #end
249 >
250 > // Returns a vector perpendicular to V
Running newly-downloaded/newly-compiled POV-Ray 3.7.0, on Linux x86_64 system
|
|
137 | Include files | Feature Request | 3.70 beta 37a | Very Low | Low | atand function | Closed | |
3.70 beta 38 |
Task Description
There already exist atan, atan2 and atan2d functions, why not atand?
|
|
225 | Light source | Definite Bug | 3.70 RC3 | Very Low | Low | translating a light source fails to translate looks_lik ... | Closed | |
3.70 RC4 |
Task Description
The following scene reders differently with POV-Ray 3.7.0.RC3 than with POV-Ray 3.6.2:
camera
{
right x*image_width/image_height
location <0, 0, -5>
look_at <0, 0, 0>
}
light_source
{
<0,0,0>
color rgb 1
looks_like
{
box {
<-1,-1,-0.1>, <1,1,0.1>
pigment { wood }
finish { ambient 5.0 diffuse 0 specular 0 phong 0 reflection 0 }
scale 0.5
}
}
translate <1,0,0>
}
plane
{
<0, 1, 0>, -1
texture
{
pigment { color rgb <0.5, 0.5, 0.55> }
finish { specular 1.0 }
}
}
See attachments for the output. As can be seen, POV-Ray 3.7 does translate the shape of the looks_like object along with the light source, but fails to translate the textures.
|
|
118 | Light source | Feature Request | 3.70 beta 37a | Very Low | Low | More efficient handling of fading lights | Tracked on GitHub | |
3.71 release |
Task Description
Currently, fading light sources are used for lighting and shadow calculations even when so far away as to no longer have any effect on the outcome. The proposed solution is to add a new keyword fade_cutoff_distance which tells povray to ignore the light source when alluminating a point at larger distance.
A sample implementation is provided in the attached files. These changes are still based on beta 34 as sources for the current beta are not yet available, and starting to merge changes to beta 35 only at this time didn’t seem worth the effort. Also, please disregard, changes in the CVS header comments (I also use CVS locally for managing source files).
Further considerations regarding this feature:
- For special effects this feature can also be used if the light source does not actually use fading. On the other hand, cutting the light at some distances can be considered an extreme form of fading which may justify the keyword name anyhow.
- Depending on how FS#46 is implemented, the test for cutoff may then be needed at another location as well.
- The default value currently is 0 (or *no* cutoff distance). For #version 3.7 of higher, the default could be chosen automatically based on the light source intensity and adc_bailout, although it may then need to be overriden by the user for extreme pigments.
|
|
275 | Light source | Definite Bug | 3.70 RC7 | Very Low | Low | circular area lights exhibit anisotropy | Tracked on GitHub | |
Future release |
Task Description
circular area lights exhibit some anisotropy, being brighter along the diagonals than on average, as can be demonstrated with the following scene:
//+w800 +h800
#version 3.7;
global_settings{assumed_gamma 1}
plane{-z,-10 pigment{rgb 1} finish{ambient 0 brilliance 0}}
disc{0,z,10000,0.5}
camera{orthographic location z look_at 10*z up y*12 right x*12}
light_source{-10*z rgb 10 area_light 10*x 10*y 257 257 adaptive 4 circular}
|
|
289 | Light source | Possible Bug | 3.70 RC7 | Very Low | Low | area_illumination with light fading and scattering medi... | Tracked on GitHub | |
|
Task Description
with reference to http://bugs.povray.org/task/46
still some issue with area illumination and light fading when interacting with media
seems light fade is not taken into account with scattering media. emission and absorption media seem to work fine. occurs with all scattering types.
#version 3.7;
global_settings {
ambient_light 0
assumed_gamma 1
}
camera {
location <0, 3, -5>
look_at <0, 2, 0>
}
#declare Light = 3; // light 1 = individual lights
// light 2 = standard area light
// light 3 = area light with area illumination
#declare Fade = 1; // light fading: 1 on, 0 off
#declare Media = 1; // media 1 = scattering
// media 2 = emission
// media 3 = absorption
#declare Type = 1; // scattering media type
#switch(Light)
#case(1)
#declare Ls = light_source {
0
1/7
#if(Fade) fade_distance 2 fade_power 2 #end
}
union {
object { Ls }
object { Ls translate .5*x }
object { Ls translate x }
object { Ls translate 1.5*x }
object { Ls translate -.5*x }
object { Ls translate -x }
object { Ls translate -1.5*x }
translate y
}
#break
#case(2)
light_source{
y
1
area_light 3*x, z, 7, 1
#if(Fade) fade_distance 2 fade_power 2 #end
}
#break
#case(3)
light_source{
y
1
area_light 3*x, z, 7, 1
#if(Fade) fade_distance 2 fade_power 2 #end
area_illumination on
}
#break
#end
cylinder { <0, .01, 0>, <0, 5, 0>, 2 pigment { rgbt 1 } hollow no_shadow
interior {
media {
#if(Media = 1) scattering {Type, 30 } #end
#if(Media = 2) emission 2 #end
#if(Media = 3) absorption 2 #end
density { cylindrical turbulence 1.5 scale <1, .14, 1> }
}
}
scale <.15, 1, .4> translate 4*z
}
plane { y,0 pigment { rgb .7 } }
plane { -z,-7 pigment { gradient y color_map { [.5 rgb 1][.5 rgb 0] } } }
union {
sphere { 0,.05 }
sphere { .5*x,.05 }
sphere { x,.05 }
sphere { 1.5*x,.05 }
sphere { -.5*x,.05 }
sphere { -x,.05 }
sphere { -1.5*x,.05 }
translate y
hollow pigment { rgbt 1 } interior { media { emission 10 } }
}
|
|
287 | Light source | Definite Bug | 3.70 RC7 | Very Low | Low | area_illumination shadow calculation | Tracked on GitHub | |
Future release |
Task Description
not sure if this is something needing further work or an intended effect.
Shadows from and area light with area_illumination on seem to follow the same shadow calculation as a standard area light by giving more weight to lights near the center of the array. I would assume the shadows would be calculated similarly to individual lights in the same pattern as the array by evenly distributing the amount of shadow equally for each light. But this is not what I see.
The code sample below when rendered with scene 1 will show shadows grouped near the center from the area light with area_illumination. If scene 1 is commented out and scene 2 is uncommented then rendered, you will see evenly distributed shadows from individual lights. Area lighting with area_illumination I would assume should give a result identical to scene 2. If scene 1 is rendered with area_illumination off, the shadow calculation is exactly the same as with area_illumination on.
example images rendered on win32 XP
#version 3.7;
global_settings {
ambient_light 0
assumed_gamma 1
}
camera {
location <0, 3, -5>
look_at <0, 2, 0>
}
background { rgb <.3, .5, .8> }
plane { y,0 pigment { rgb .7 } }
torus { 1.5,.1 rotate 90*x translate 4*z pigment { rgb .2 } }
plane { -z,-7 pigment { rgb .7 } }
/*
// scene 1
light_source{
y
1
area_light 3*x, z, 7, 1
area_illumination on
}
union {
sphere { 0,.05 }
sphere { .5*x,.05 }
sphere { x,.05 }
sphere { 1.5*x,.05 }
sphere { -.5*x,.05 }
sphere { -x,.05 }
sphere { -1.5*x,.05 }
translate y
hollow pigment { rgbt 1 } interior { media { emission 10 } }
}
// end scene 1
*/
// scene 2
#declare Light = light_source {
0
1/7
looks_like { sphere { 0,.05 hollow pigment { rgbt 1 } interior { media { emission 10 } } } }
}
union {
object { Light }
object { Light translate .5*x }
object { Light translate x }
object { Light translate 1.5*x }
object { Light translate -.5*x }
object { Light translate -x }
object { Light translate -1.5*x }
translate y
}
// end scene 2
|
|
279 | Light source | Possible Bug | 3.70 RC7 | Very Low | Low | area_illumination causes artifacts when used with radio ... | Closed | |
|
Task Description
see my post titled: “area light and radiosity problem?” in povray.binary.images [Edit - copied that post’s text here - clipka]
wondering about what’s going on here with this series of images. the radiosity and area light settings are unchanged from image to image, and all I did was radiosity on/off and area_light on/off (btw: using rad_def “Normal” settings)
the 1st image is radiosity only, the 2nd is area light only, and the 3rd combines them:
what’s up with blotches? change #5819/5820 (octree) or maybe something still with area lights?
|
|
46 | Light source | Unimp. Feature/TODO | 3.70 beta 32 | Very Low | Low | area_illuminate in area lights is not taking fade_dista ... | Closed | |
3.70 RC4 |
Task Description
It seems that the new area_illuminate flag for area lights does not take into account fade_power and fade_distance. The illumination falloff is still being calculated from the center of the light_source.
Here’s some relevant code:
camera{
location<0,10,-10>
look_at 0
}
plane{y,0 pigment{rgb 1}}
light_source{
y*.1,100
area_light x*10, z*1, 8, 8
jitter
area_illumination
fade_power 2 fade_distance 1
}
|
|
177 | Light source | Feature Request | 3.70 beta 39 | Very Low | Low | Add support for conserve_energy to shadow computations | Tracked on GitHub | |
|
Task Description
The following scene gives a comparison of current conserve_energy handling in standard shadow computations vs. photons.
Note how the rather highly reflective slabs fail to cast shadows, except where the photons target sphere enforces computation of shadow brightness to be done by the photons algorithm.
For more realistic shadowing without the need to enable photons, I suggest do add proper conserve_energy handling to the shadow computation code (which shouldn’t be too much effort).
global_settings {
max_trace_level 10
photons { spacing 0.003 media 10 }
}
camera {
right x*image_width/image_height
location <-2,2.6,-10>
look_at <0,0.75,0>
}
light_source {
<500,300,150>
color rgb 1.3
photons {
refraction on
reflection on
}
}
sky_sphere {
pigment {
gradient y
color_map {
[0.0 rgb <0.6,0.7,1.0>]
[0.7 rgb <0.0,0.1,0.8>]
}
}
}
plane {
y, 0
texture { pigment { color rgb 0.7 } }
}
#declare M_Glass=
material {
texture {
pigment {rgbt 1}
finish {
ambient 0.0
diffuse 0
specular 0.2 // just to give a hint where the sphere is
}
}
interior { ior 1.0 }
}
#declare M_PseudoGlass=
material {
texture {
pigment {rgbt 1}
finish {
ambient 0.0
diffuse 0.5
specular 0.6
roughness 0.005
reflection { 0.3, 1.0 fresnel on }
conserve_energy
}
}
interior { ior 1.5 }
}
sphere {
<1.1,1,-1.3>, 1
material { M_Glass }
photons {
target 1.0
refraction on
reflection on
}
}
// behind target object
box {
<-0.2,0,-2.3>, <0.0,4,0.3>
material { M_PseudoGlass }
rotate z*1 // just to better see the reflection of the horizon
}
// before target object
box {
<2.4,0,-2.3>, <2.6,4,-0.3>
material { M_PseudoGlass }
photons { pass_through }
rotate z*1 // just to better see the reflection of the horizon
}
|
|
185 | Other | Definite Bug | 3.70 beta 41 | Very Low | Very Low | wrong message about image resolution | Closed | |
3.70 RC2 |
Task Description
‘povray -H10 -W20 myscene.pov’ will generate a file with a picture 10 pixels high and 20 pixels wide, BUT in the message pane it displays
Image resolution.....20 by 10 (rows 1 to 20, columns 1 to 10)
instead of
Image resolution.....20 by 10 (rows 1 to 10, columns 1 to 20)
or
Image resolution.....20 by 10 (columns 1 to 20, rows 1 to 10)
|
|
303 | Other | Definite Bug | 3.70 RC7 | Defer | Very Low | wrong bit depth reported for OpenEXR file format | Tracked on GitHub | |
|
Task Description
When using OpenEXR output file format, POV-Ray erroneously reports it as “24 bpp EXR” in the message output, while in fact it generates a 3×16 = 48 bpp file.
|
|
265 | Other | Possible Bug | 3.70 RC6 | Very Low | Low | Warnings from clang that might need consideration | Closed | |
|
Task Description
Compiling the sources with clang instead of g++ (on ubuntu 12.10 with boost 1.50)
./configure COMPILED_BY=”your name here <also@email>” LIBS=-lboost_system –disable-io-restrictions CC=clang CXX=clang
there is a few warnings that catch the eyes (and other as well that I dismiss so far, such as cases not covered in switch and empty body in if, or extraneous parentheses in tests):
support/randomsequences.cpp:553:15: warning: field is uninitialized when used here [-Wuninitialized]
startIndex(startIndex)
^
support/randomsequences.cpp:553:15: warning: field is uninitialized when used here [-Wuninitialized]
support/randomsequences.cpp:974:40: note: in instantiation of member function 'pov::PrecomputedNumberGenerator<int>::PrecomputedNumberGenerator' requested here
SeedableIntGeneratorPtr generator(new PrecomputedIntGenerator(factory, count));
^
support/randomsequences.cpp:553:15: warning: field is uninitialized when used here [-Wuninitialized]
startIndex(startIndex)
^
support/randomsequences.cpp:984:43: note: in instantiation of member function 'pov::PrecomputedNumberGenerator<double>::PrecomputedNumberGenerator' requested here
SeedableDoubleGeneratorPtr generator(new PrecomputedDoubleGenerator(factory, count));
^
support/randomsequences.cpp:553:15: warning: field is uninitialized when used here [-Wuninitialized]
startIndex(startIndex)
^
support/randomsequences.cpp:1011:43: note: in instantiation of member function 'pov::PrecomputedNumberGenerator<pov::Vector3d>::PrecomputedNumberGenerator' requested here
return SequentialVectorGeneratorPtr(new PrecomputedVectorGenerator(factory, count));
^
support/randomsequences.cpp:553:15: warning: field is uninitialized when used here [-Wuninitialized]
startIndex(startIndex)
^
support/randomsequences.cpp:1056:45: note: in instantiation of member function 'pov::PrecomputedNumberGenerator<pov::Vector2d>::PrecomputedNumberGenerator' requested here
return SequentialVector2dGeneratorPtr(new PrecomputedVector2dGenerator(factory, count));
Self referencing member in creator does not seems to be great for a reproducible pseudorandom generator (some compiler/architecture might force to 0, other might not... seems bad karma).
povmscpp.cpp:1875:4: warning: delete called on 'POVMS_MessageReceiver::HandlerOO' that is abstract but has non-virtual destructor [-Wdelete-non-virtual-dtor]
delete nodeptr->handleroo;
^
povmscpp.cpp:1877:4: warning: delete called on 'POVMS_MessageReceiver::Handler' that is abstract but has non-virtual destructor [-Wdelete-non-virtual-dtor]
delete nodeptr->handler;
^
Maybe just a missing keyword (virtual) in the header file ? Or is it harder ?
shelloutprocessing.cpp:260:28: warning: expression result unused [-Wunused-value]
for (s = str.c_str(); *s; *s++)
^~~~
Why “*s++” ? why not just “s++” ?
renderfrontend.cpp:1165:57: warning: trigraph ignored [-Wtrigraphs]
default: t = "(???)"; break;
I guess it’s not an intended trigraph. Might nevertheless perturb some compiler/result.
|
|
283 | Other | Definite Bug | 3.70 RC7 | Very Low | High | Transparent or semi-transparent background color comes ... | Closed | |
|
Task Description
When using the ‘background’ directive with a transparent color, for example:
background { color rgbt <0, 0, 0, 1> }
the final image is still opaque (both the one displayed in the render window and the PNG actually saved to disk).
Expected behaviour is for it to be transparent.
|
|
32 | Other | Definite Bug | 3.70 beta 32 | Very Low | Medium | tiff file extention error | Closed | |
|
Task Description
The parser is failing to read the .tiff file extension from the input string...
bump_map { tiff "earth03_hf2.tiff" }
Results in file not found, but
bump_map { tiff "earth03_hf2" }
will find the file. It might be that it’s not a three character extension?
|
|
247 | Other | Feature Request | 3.70 RC6 | Very Low | Low | Set no_radiosity in Screen_Object() | Closed | |
Future release |
Task Description
Suggestion:
In file screen.inc, have macro Screen_Object() set no_radiosity on the object.
|
|
326 | Other | Definite Bug | 3.70 release | Very Low | Low | restricted setting ignored in 3.7 | Tracked on GitHub | |
|
Task Description
Due to a typo in the conf file parser (introduced, I think, in refactoring after 3.6), the restricted setting is ignored, and access checks aren’t performed.
Fixing this reveals some other issues:
%INSTALLDIR%/../../etc is incompletely canonicalized to /usr/local/share/../etc , not /usr/local/etc
read+write paths are added to the read list only, so writing is impossible
See attached patch.
Relatedly, I think it would be nice to add a new replacement token %CONFDIR% instead of %INSTALLDIR%/../../etc .
Also, there’s a realpath function that could simplify path handling, though I’m not sure if it’s available on all platforms.
|
|
312 | Other | Possible Bug | 3.70 release | Very Low | Low | Rendering stuck at 99% | Closed | |
|
Task Description
After a long parse period and a relatively quick rendering, POVray gets stuck at 99% when rendering the attached file.
Rendered at 6144x3072px with antialiasing set to 0.3.
Can anyone confirm?
|
|
270 | Other | Definite Bug | 3.70 release | Medium | High | render abort-continue (+C) sometimes skips blocks | Closed | |
|
Task Description
When aborting a render when there are unfinished blocks among finished ones, under certain conditions some of those blocks are skipped when continuing the render later.
|
|
246 | Other | Possible Bug | 3.70 RC6 | Very Low | Low | Regression on scale limit between 3.7 and previous rele... | Tracked on GitHub | |
|
Task Description
From Thomas de Groot
Using the following code for a (sky) sphere in a scene, with light source well outside the sphere; works correctly until the above scale value. Use a value of >=100*10e4 and the sphere becomes black.
#version 3.7;
global_settings{ assumed_gamma 1.0 }
#declare T_sky =
texture {
pigment {
gradient y
pigment_map {
[0.0 srgb <1.0,0.7,0.6>*1 transmit 0.5]
[1.0 srgb <0.8,0.1,0.0>*1 transmit 0.5]
}
}
finish {
emission 0.9
diffuse 0.0
}
}
#declare T_cosmos =
texture {
pigment {
color rgbt <0,0,0,1>
}
finish {
ambient 0.0
diffuse 0.0
}
}
sphere {
<0,0,0>,1
texture {T_sky}
interior_texture {T_cosmos}
no_shadow
no_reflection
inverse
scale 99.9*10e4
}
Working with windows version of POV-Ray and Win7 x64
Is this normal for version 3.7 RC5? I seem to remember that with lower versions of POV-Ray on could go at least to 10e6. Especially with the Ringworld scenes back in 2010 the scales used where much larger without any black out.
I can indeed confirm that the Ringworld scene does not render correctly anymore, with identical black out.
|
|
300 | Other | Feature Request | 3.70 RC7 | Defer | Very Low | Reference Documentation Support | Tracked on GitHub | |
|
Task Description
As emerged as an idea during the discussion of FS#299, an SDL / POV-Ray editor feature would be useful that allows API documentation via formal comments, e.g. in include files:
/**
* Creates a car object.
* @param a
* description of param a
* ...
*/
#macro car(a,b,c)
...
#end
In addition to the ability of (auto-)generating a documentation file from such comments, an editor window feature would be convenient that allows popup display of a macro’s (object’s / parameter’s / ...) documentation section.
|
|
176 | Other | Feature Request | Not applicable | Very Low | Low | Raise maxpower of the Poly Oject to 16. | Closed | |
|
Task Description
At the moment in the Poly Object the maximum power is 15. The mathematics for converting the three parametric equations for x, y and z into a formula for the Poly Object require that the equations are squared several times given max-powers of 4, 8 and even 16. I’ve one eqaution that needs power 16. At the moment this is just one power short. Please raise this to 16. That’s all I ask for.
|
|
217 | Other | Possible Bug | 3.70 RC3 | Very Low | High | raddem.ini with +C and some frames already done: failur ... | Closed | |
|
Task Description
How to do it: (with raddem.ini & raddem.pov from distributed scenes, copied in local directory)
1. run “povray raddem.ini” until frame 6 or more (irrelevant, at least frame 1 & 2 are needed), interrupt the render. 2. restart “povray raddem.ini +C”
It fails at frame 2 with Possible Parse Error: Cannot find file ‘raddem.pov’, even after trying to append file type extension. Parse Error: Cannot open input file. Fatal error in parser: Cannot parse input. Render failed
The detection of frame 1 is fine.
|
|
173 | Other | Feature Request | 3.70 beta 39 | Very Low | Low | Prevent POV-Ray for Windows from stealing focus | Closed | |
|
Task Description
In some cases it may be desirable to run POV-Ray from a batch file, without causing it to “steal the focus”.
I suggest making this dependant on whether POV-Ray is run with the /EXIT parameter.
|
|
195 | Other | Compatibility Issue | 3.70 RC3 | Very Low | Medium | povray-3.7.0rc3 incompatible with NetBSD | Closed | |
|
Task Description
While testing if the png support was working, I tried 3.7.0rc3 on NetBSD-5.99.45/amd64, and had the following problems:
1. lseek64 (used in source/base/image/image.cpp) is not portable, and not necessary on NetBSD (off_t there is large-file-safe) 2. unix/Makefile.am doesn’t add -lboost_thread to povray_LDADD, which breaks linking the executable. 3. vfe/unix/platformbase.cpp uses CLOCK_THREAD_CPUTIME_ID, which is not provided on NetBSD (I hacked around it by defining the symbol to “0”, but that’s of course not a correct fix). 4. vfe/unix/platformbase.cpp uses CLOCK_PROCESS_CPUTIME_ID, which is not provided on NetBSD – it’s called CLOCK_REALTIME like on FreeBSD, so we could just add defined(NetBSD) to the FreeBSD case, except for point 3. 5. vfe/unix/vfeplatform.cpp uses WEXITSTATUS. For this, sys/wait.h should be included. The obvious fix is #ifdef HAVE_SYS_WAIT_H # include <sys/wait.h> #endif but this also needs a check in the configure script.
Fixing all this, I get it to build, but core dump when run against the demo file from http://www.csb.yale.edu/userguides/graphics/povray/demo.pov.html. Backtrace is Program terminated with signal 11, Segmentation fault. #0 0x00000000004ac479 in boost::gregorian::date::date () (gdb) bt #0 0x00000000004ac479 in boost::gregorian::date::date () #1 0x00000000004d29f7 in boost::gregorian::date::date () #2 0x0000000000479a85 in std::vector<std::string, std::allocator<std::string> >::operator= () #3 0×0000000000461570 in std::vector<std::string, std::allocator<std::string> >::operator= () #4 0x00000000004656c7 in std::vector<std::string, std::allocator<std::string> >::operator= () #5 0x00000000005efc9f in Imf::TypedAttribute<std::string>::typeName () #6 0x00000000005fd890 in Imf::TypedAttribute<std::string>::typeName () #7 0x00000000005fe5d8 in Imf::TypedAttribute<std::string>::typeName () #8 0x000000000045d6dc in std::vector<std::string, std::allocator<std::string> >::operator= () #9 0x00007f7ffd80d9cf in thread_proxy ()
from /usr/pkg/lib/libboost_thread.so.1.45.0
#10 0x00007f7ffd00b24e in pthreadcreate_tramp (cookie=<value optimized out>) at /archive/cvs/src/lib/libpthread/pthread.c:473 #11 0x00007f7ff8871780 in _lwp_park50 () from /usr/lib/libc.so.12
Please advise on how to proceed.
|
|
76 | Other | Feature Request | 3.6 | Very Low | Medium | Povray returns incorrect exit code when aborting render | Closed | |
3.70 release |
Task Description
If you abort a render with ^C, Povray exits with a ‘success’ error code.
To test:
povray scene.ini
(^C to abort it)
echo $?
Right now 0 is returned (’success’). A non-zero value should be returned (’failure’).
This is particularly important for scripting, where command lines like:
povray scene.ini && halt
...can be used. I only want the halt to be executed if the scene renders successfully. If I change my mind and ^C it, I don’t want the machine to shut down!
|
|
245 | Other | Feature Request | All | Defer | Low | POVMS message queue can fill up with GB of data for ver... | Tracked on GitHub | |
Future release |
Task Description
With very fast renders and very large output files, the message queue can fill up because the producers are not limited by IO, while the consumer performance is limited by disk IO. Consequently, the message queue can fill up to exhaust all available memory. The solution is to build in some better control of pending output data in the message queue on the producer side. This will also pave the way for message communication over slow links (i.e. a network).
|
|
257 | Other | Definite Bug | 3.70 RC6 | Very Low | Low | POV-Ray cannot find input file when resuming to render ... | Closed | |
3.70 RC7 |
Task Description
How to reproduce:
# An empty directory, an empty source file.
$ mkdir test && cd test && touch test.pov
# Generate the first 24 frames.
$ povray -D +KFF24 +Itest.pov +Otest.png
# Try to generate the 25th frame.
# `25' after `+KFF' can be changed to any integer greater than 24.
$ povray -D +C +KFF25 +Itest.pov +Otest.png
What happens:
==== [Parsing...] ==========================================================
Possible Parse Error: Cannot find file 'test.pov', even after trying to append
file type extension.
Parse Error: Cannot open input file.
Fatal error in parser: Cannot parse input.
Render failed
OS: Gentoo AMD64 unstable POV-Ray version: 3.7.0 rc5
|
|
160 | Other | Feature Request | All | Very Low | Very Low | Parallel GPU processing support | Closed | |
|
Task Description
...for instance nVidia’s CUDA architecture, discussed here and other places.
General consensus is that it’s not worth the effort if only a partial set of POV-Ray’s features are possible.
|
|
273 | Other | Definite Bug | 3.70 RC6 | Very Low | Medium | No automatic backup files from inc files | Tracked on GitHub | |
|
Task Description
If enabled, POVray always created backups of pov and inc files once per session. Now using 3.7 RC6 only pov file backups are created but not from inc files.
|
|
272 | Other | Feature Request | 3.70 RC6 | Defer | Very Low | Minor change, significant speedup in cubic polynomial s... | Tracked on GitHub | |
3.71 release |
Task Description
While familiarizing myself with the code, I found some small changes in the solve_cubic function that lead to a significant speedup.
In my experience, “pow” is by far the slowest function in math.h and replacing it with simpler functions usually makes a tremendous impact on the speed (it’s an order of magnitude slower than sqrt/exp/cbrt/log).
solve_cubic has a “pow” function that can be replaced by cbrt (cubic root), which is standard in ISO-C99 and should be available on all systems. Separate benchmarks of solve_cubic function show this change almost doubles the speed and does not lower the accuracy. As solve_cubic is part of the solution of quartic equation, this improves the speed for many primitives. Testing with a scene containing many torus intersection tests (attached below) I still observed almost 10% speedup (Intel, 4 threads, 2 hyperthreaded cores, antialiasing on, 600×600: from 91 to 84 seconds). And this is for a torus, where a lot of time is spent in the solve_quartic and cubic solver is only called once! Similar speedup should be expected for prism, ovus, sor and blob.
I do believe the cubic solver can be done without trigonometry, but that would mean changing the algorithm, introducing new bugs and requiring a lot of testing. However, the trigonometric evaluation can still be simplified (3% speedup in full torus benchmark).
These changes don’t affect the algorithm at all, they are mathematically identical to the existing code, so the changes can be applied immediately. I also included other changes just as suggestions. Every change is commented and marked with [SC 2.2013].
This sadly does not speedup the sturm solver, which uses bisection and regula-falsi and looks very optimized already.
The test scene I used has a lot of torus intersections from various directions (shadow rays, main rays, transmitted rays).
|
|
277 | Other | Possible Bug | 3.70 RC7 | Very Low | Medium | Max Image Buffer Memory Does not Seem to Work | Closed | |
|
Task Description
In POV-Ray’s documentation it says:
3.2.2.2 Max Image Buffer Memory
This INI parameter sets the number of megabytes of RAM to allow for output image caching. If the output image happens to use more than this, a file backed temporary image is used instead.
I used this INI file option because the default value (128 megabytes) seemed insufficient. pov-state backend files were always created and they were remarkably larger than the resulting image (bmp) files. Consequently, I set
Max_Image_Buffer_Memory = 3096
in the INI file so that POV-Ray should, according to the documentation, now be able to use 3 gigabytes of RAM so no backend temporary file would be needed at all (this large they were never).
However, while POV-Ray was rendering I still discovered a pov-state file and it still had a similar size.
Now I am confused: did the INI option not work or have I misunderstood the documentation? If the former is the case, that would be a bug, wouldn’t it?
I tested both under Windows XP and Debian 6.0.5.
|
|
250 | Other | Possible Bug | 3.70 RC6 | Very Low | Low | ini shell-outs always fail | Closed | |
|
Task Description
I’ve got an ini file that looks like this:
Post_Frame_Return=U Post_Frame_Command=notepad.exe
And when I render a scene using that ini file, it renders correctly but then gives me this error:
Render halted because the post-frame shell-out (’notepad.exe’) requested POV-Ray to generate a user abort. Render failed
.....and it doesn’t open notepad.
I’ve unchecked the “Disable Starting Other Programs” and I’ve tried various variations on what exe to run and whether to do it Pre/Post Frame/Scene, and nothing has worked.
|
|
41 | Other | Feature Request | 3.70 beta 32 | Very Low | Low | improve command-line parsing error messages | Tracked on GitHub | |
|
Task Description
POV-Ray 3.6, upon encountering problems when parsing command line and/or .ini file options, would quote the offending option in the error message.
POV-Ray 3.7 currently just reports that there is some problem with the command line, without providing any details. I suggest changing this, as the information may be helpful at times.
|
|
297 | Other | Feature Request | 3.70 RC7 | Very Low | Low | Have a user-definable epsilon | Closed | |
|
Task Description
There are times when scaling an entire scene up or down is difficult or just not feasible.
One suggestion is a global_settings option.
Also, I’ve noticed that in some situations, such as interactions between certain transparent objects, the epsilon seems to kick in quite early. Perhaps there could be situational or contextual epsilons, such as the “tolerance” of sphere_sweep or the “accuracy” of isosurface.
|
|
97 | Other | Possible Bug | 3.70 beta 36 | Very Low | Low | Forward-slash pathnames not fully supported in Windows ... | Closed | |
3.70 beta 38 |
Task Description
The current Windows version of POV-Ray does not fully support forward slashes in pathnames; specifically, POV-Ray fails to recognize drive letters when followed by a forward slash, e.g. “C:/foo/bar.pov” or “C:/foo\bar.pov”, rejecting such names for e.g. Input_File_Name.
|
|
301 | Other | Definite Bug | 3.70 RC7 | Very Low | Low | Fallback to default image size causes wrong values to b... | Tracked on GitHub | |
|
Task Description
When resolution is not specified (neither via POVRAY.INI nor via QUICKRES.INI nor via command line or custom .ini file), random values are displayed for image resolution in the Image Output Options message output. (The actual render will be performed at the default size of 160×120 pixels though.)
|
|
214 | Other | Definite Bug | 3.70 RC3 | Very Low | Low | Failed to parse command-line option in Debian | Closed | |
3.70 RC4 |
Task Description
I tried to use 3.7 RC3. This was my first time with 3.7.
I got source, configured and compiled it and installed into Debian with checkinstall. And then I tried to use it. First run was with -benchmark (it took about 9 minutes, ok). Then I tried very simple scene:
rekcahx@oah:~/pov$ povray +Iaa.pov povray: This is a RELEASE CANDIDATE version of POV-Ray. General distribution is discouraged. Failed to parse command-line option
I tried to debug with strace:
rekcahx@oah:~/pov$ strace -o debug.strace povray +Iaa.pov povray: This is a RELEASE CANDIDATE version of POV-Ray. General distribution is discouraged. Persistence of Vision™ Ray Tracer Version 3.7.0.RC3 (g++ 4.6.1 @ x86_64-unknown-linux-gnu) This is a release candidate of POV-Ray version 3.7.0. General distribution is strongly discouraged.
POV-Ray is based on DKBTrace 2.12 by David K. Buck & Aaron A. Collins Copyright 1991-2003 Persistence of Vision Team Copyright 2003-2011 Persistence of Vision Raytracer Pty. Ltd.
Primary POV-Ray 3.7 Architects/Developers: (Alphabetically)
Chris Cason Thorsten Froehlich Christoph Lipka
With Assistance From: (Alphabetically)
Nicolas Calimet James Holsenback Christoph Hormann Nathan Kopp
Juha Nieminen
Past Contributors: (Alphabetically)
Steve Anger Eric Barish Dieter Bayer David K. Buck
Nicolas Calimet Chris Cason Aaron A. Collins Chris Dailey
Steve Demlow Andreas Dilger Alexander Enzmann Dan Farmer
Thorsten Froehlich Mark Gordon James Holsenback Christoph Hormann
Mike Hough Chris Huff Kari Kivisalo Nathan Kopp
Lutz Kretzschmar Christoph Lipka Jochen Lippert Pascal Massimino
Jim McElhiney Douglas Muir Juha Nieminen Ron Parker
Bill Pulver Eduard Schwan Wlodzimierz Skiba Robert Skinner
Yvo Smellenbergh Zsolt Szalavari Scott Taylor Massimo Valentini
Timothy Wegner Drew Wells Chris Young
Other contributors are listed in the documentation.
Support libraries used by POV-Ray:
ZLib 1.2.3.4, Copyright 1995-1998 Jean-loup Gailly and Mark Adler
LibPNG 1.2.44, Copyright 1998-2002 Glenn Randers-Pehrson
LibJPEG 62, Copyright 1998 Thomas G. Lane
LibTIFF 3.9.5, Copyright 1988-1997 Sam Leffler, 1991-1997 SGI
Boost 1.46, http://www.boost.org/
OpenEXR, Copyright (c) 2004-2007, Industrial Light & Magic.
Parser Options
Input file: aa.pov
Remove bounds........On
Split unions.........Off
Library paths:
/usr/share/povray
/usr/share/povray/ini
/usr/share/povray/include
Clock value: 0.000 (Animation off)
Image Output Options
Image resolution.....320 by 240 (rows 1 to 240, columns 1 to 320).
Output file..........aa.png, 24 bpp PNG
Dithering............Off
Graphic display......Off
Mosaic preview.......Off
Continued trace......Off
Information Output Options
All Streams to console..........On
Debug Stream to console.........On
Fatal Stream to console.........On
Render Stream to console........On
Statistics Stream to console....On
Warning Stream to console.......On
[Parsing...]
Parse Warning: This scene did not contain a #version directive. Please be aware that as of POV-Ray 3.7, unless already specified via an INI option, a #version is expected as the first declaration in a scene file. POV-Ray may apply settings to some features that are intended to maintain compatibility with pre-3.7 scenes. You are strongly encouraged to add a #version statement to the scene to make your intent clear. Future versions of POV-Ray may make the presence of a #version statement mandatory.
Parser Statistics
Finite Objects: 1 Infinite Objects: 0 Light Sources: 1 Total: 2
Parser Time
Parse Time: 0 hours 0 minutes 0 seconds (0.001 seconds)
using 1 thread(s) with 0.000 CPU-seconds total
Bounding Time: 0 hours 0 minutes 0 seconds (0.000 seconds)
using 1 thread(s) with 0.000 CPU-seconds total
—————————————————————————- Render Options
Quality: 9
Bounding boxes.......On Bounding threshold: 3
Antialiasing.........Off
[Rendering...]
Rendered 76800 of 76800 pixels (100%)
Render Statistics Image Resolution 320 x 240
Pixels: 76800 Samples: 0 Smpls/Pxl: 0.00 Rays: 76800 Saved: 0 Max Level: 1/5
Ray→Shape Intersection Tests Succeeded Percentage
Box 78226 1426 1.82
Shadow Ray Tests: 1426 Succeeded: 0
Render Time:
Photon Time: No photons
Radiosity Time: No radiosity
Trace Time: 0 hours 0 minutes 0 seconds (0.016 seconds)
using 4 thread(s) with 0.036 CPU-seconds total
POV-Ray finished
—
Every now and then all other command line options than –version, -version, -V, –help, -help -h, -?, –benchmark and –benchmark without leading strace in command line produces “Faild to parse command-line option” error.
My system: ebian GNU/Linux unstable (sid), quadcore AMD Phenom 2.6 GHz, 8GB ram. Povray: rekcahx@oah:~/pov$ povray –version povray: This is a RELEASE CANDIDATE version of POV-Ray. General distribution is discouraged. POV-Ray 3.7.0.RC3
This is a release candidate of POV-Ray version 3.7.0. General distribution is strongly discouraged.
Copyright 1991-2003 Persistence of Vision Team Copyright 2003-2011 Persistence of Vision Raytracer Pty. Ltd.
Built-in features:
I/O restrictions: disabled
X Window display: enabled (using SDL)
Supported image formats: gif tga iff ppm pgm hdr png jpeg tiff openexr
Unsupported image formats: -
Compilation settings:
Build architecture: x86_64-unknown-linux-gnu
Built/Optimized for: x86_64-unknown-linux-gnu (using -march=native)
Compiler vendor: gnu
Compiler version: g++ 4.6.1
Compiler flags: -pipe -Wno-multichar -Wno-write-strings -fno-enforce-eh-specs -s -O3 -ffast-math -march=native -pthread
|
|
220 | Other | Compatibility Issue | 3.6 | Very Low | High | Error number -43 | Closed | |
|
Task Description
REcently I installed POV-Ray tracing software in my mac OS X version 10.6.8. When I run the software its displaying a fatal error occured and the error number is -43. I’m new to POV-Ray...pls help me guys...
|
|
61 | Other | Definite Bug | 3.70 beta 34 | Low | Medium | Dispersion does not give proper results | Closed | |
|
Task Description
Source code inspection during examination of issues with the scene published at http://povray.sitewww.ch/?p=177 show the following issues with current (beta.34) implementation of dispersion in POV-Ray 3.7:
While this still allows to use dispersion for artistic effect, it is neither physically realistic, nor does it match 3.6 behavior.
|
|
109 | Other | Compatibility Issue | 3.70 beta 37a | Defer | Very Low | Debug_File No Longer Appends Frame by Frame Debug Data | Closed | |
Future release |
Task Description
The function of the “Debug_File=” .ini option has changed from 3.6 to 3.7.37a. In 3.6, when rendering multiple frames, a debug file would be created that then appended the debug lines for each frame into the file. It was therefore able to have debug data that identified what parameters were used in which frame in case a frame did not have the desired effect.
In 3.7.37a, the debug file does not perform this function. Instead it creates a new debug file (overwriting the prior) with each new frame. Therefore the debug data is only useful for the final frame (or wherever the render was halted). This is useful for a single frame render or for identifying a fault within a series of frames (because only the last one will remain) but it is not useful for many frames that render successfully.
This problem does not cause any rendering errors or other defects. The debug file specified will only contain the debug data for the last frame rendered.
Per discussion in the forum it was unknown if this was a bug or “feature”. At this time it is causing me a problem so I am submitting the bug. No related bugs were found searching for “output” or “debug” in any status.
Operating System in use is Windows XP. I cannot test 3.7.37a in additional OSes, but it does not seem like it would be OS-specific.
|