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104 | Image format | Definite Bug | 3.70 beta 37 | Medium | Critical | Output file gamma broken for File_Gamma=1.0 | Closed | |
3.70 beta 37a |
Task Description
Setting File_Gamma=1.0 produces unexpectedly bright output files for most output file formats, as if File_Gamma was set to 2.2 instead.
The underlying problem is a bug that, when File_Gamma is set to exactly 1.0, causes the encoding gamma function to be undefined, which was not meant to happen in current versions, and instead was reserved for future versions to signal that a file-format-specific default encoding gamma should be used. The image file output handlers already support this, most of them choosing the sRGB transfer function, giving roughly the same output as setting File_Gamma=2.2.
As a preliminary workaround, users may want to set File_Gamma=1.02 (any value smaller than 0.99 or greater than 1.01 should do).
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270 | Other | Definite Bug | 3.70 release | Medium | High | render abort-continue (+C) sometimes skips blocks | Closed | |
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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.
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48 | Geometric Primitives | Definite Bug | All | Low | High | CSG bounding box computation broken with shearing trans ... | Closed | |
|
Task Description
Bounding box computation for CSG intersection appears to be broken when one member is an arbitrarily transformed plane.
POV-Ray 3.6.2 has the same problem (can’t test for 3.6.1).
// +W640 +H480 +MB1
#include "transforms.inc"
camera {
location <-0.2, 0.5, -4.0>
direction 1.5*z
right x*image_width/image_height
look_at <0.0, 0.0, 0.0>
}
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>]
}
}
}
light_source {
<0, 0, 0> // light's position (translated below)
color rgb <1, 1, 1> // light's color
translate <-30, 30, -30>
}
plane {
y, -1
pigment { color rgb <0.7,0.5,0.3> }
}
intersection {
sphere {
0.0, 1 }
plane { -x, 0 transform { Shear_Trans(x,y+x*0.3,z) } }
texture {
pigment {
radial
frequency 8
color_map {
[0.00 color rgb <1.0,0.4,0.2> ]
[0.33 color rgb <0.2,0.4,1.0> ]
[0.66 color rgb <0.4,1.0,0.2> ]
[1.00 color rgb <1.0,0.4,0.2> ]
}
}
finish{
specular 0.6
}
}
rotate -y*5
}
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70 | Photons | Unimp. Feature/TODO | 3.70 beta 34 | Low | High | load/save photons should be controlled via command line | Tracked on GitHub | |
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Task Description
Just like radiosity load/save, the photon mapping load/save mechanism should be moved to the frontend and controlled via command-line switch, instead of being SDL-driven in the backend.
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95 | Photons | Definite Bug | 3.70 beta 36 | Low | High | Photons are over-attenuated by semi-transparent surface ... | Closed | |
3.70 beta 37 |
Task Description
The code to attenuate transmitted photons according to surface texture was apparently duplicated during refactoring of the source code for version 3.7. Behavior has changed from 3.6 to 3.7 (beta.36) accordingly, as can be demonstrated with the following scene:
global_settings {
assumed_gamma 1.0
max_trace_level 10
photons { spacing 0.02 }
}
camera {
right x*image_width/image_height
location <0,2.6,-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 <1.0, 0.8, 0.6> } }
}
#declare M_Glass=
material {
texture {
pigment {rgbt 1}
finish {
ambient 0.0
diffuse 0.05
specular 0.6
roughness 0.005
reflection { 0.1, 1.0 fresnel on }
conserve_energy
}
}
interior {
ior 1.5
fade_power 1001
fade_distance 0.9
fade_color <0.5,0.8,0.6>
}
}
#declare M_PseudoGlass2=
material {
texture {
pigment {rgbf <0.8,0.2,0.2,0.8>}
finish {
ambient 0.0
diffuse 0.05
specular 0.6
roughness 0.005
reflection { 0.1, 1.0 fresnel on }
conserve_energy
}
}
interior {
ior 1.0
}
}
sphere {
<1.1,1,-1.3>, 1
material { M_Glass }
photons {
target 1.0
refraction on
reflection on
}
}
box {
<2.4,0,-2.3>, <2.6,4,0.3>
material { M_PseudoGlass2 }
photons { target 1.0 refraction on reflection on }
}
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113 | Texture/Material/Finish | Definite Bug | 3.70 beta 37a | Low | High | Multi-layered reflections broken | Closed | |
3.70 beta 38 |
Task Description
Reflections in multi-layered textures are broken in 3.7 betas, as can be demonstrated with the following scene showing two reflective hemispheres on a checkered plane:
camera {
location <1.0, 0.5, -4.0>
direction 1.5*z
right x*image_width/image_height
look_at <0.0, 0.0, 0.0>
}
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>]
}
}
}
light_source {
<0, 0, 0> // light's position (translated below)
color rgb <1, 1, 1> // light's color
translate <-30, 30, -30>
}
default {
finish { diffuse 0 ambient 0 specular 0 }
}
// ----------------------------------------
plane { // checkered floor
y, -1
texture
{
pigment { checker color rgb 1 color blue 1 }
finish{ diffuse 0.8 ambient 0.1 }
}
}
// left hemisphere
intersection {
sphere { 0, 1 }
plane { x, -0.002 }
texture {
pigment { color rgb 1 }
finish{ reflection { 0.5 } }
}
texture {
pigment { color rgbt 1 }
finish{ reflection { 0.4 } }
}
texture {
pigment { color rgbt 1 }
finish{ reflection { 0.1 } }
}
}
// right hemisphere
intersection {
sphere { 0, 1 }
plane { -x, -0.002 }
texture {
pigment { color rgb 1 }
finish{ reflection { 1.0 } }
}
}
Note that the reflection parameters of the left, multi-layered hemisphere sum up to 1.0, i.e. the same value as used in the single layer in the right hemisphere.
The first attached file (test_3.6.2.png), rendered with POV-Ray 3.6.2, shows the expected output: Both hemispheres appear to have the same reflectivity.
The second attached file (test_3.7.0.beta37a.png), rendered with POV-Ray 3.7.0.beta.37a, shows a much brighter left (multi-layered) sphere.
As it turns out, in order to get the expected result with POV-Ray 3.7.0.beta.37a, the reflectivity of each layer must be divided by 3, 2 and 1, respectively (which obviously does not sum up to 1.0):
...
texture {
pigment { color rgb 1 }
finish{ reflection { 0.5 / 3 } }
}
texture {
pigment { color rgbt 1 }
finish{ reflection { 0.4 / 2 } }
}
texture {
pigment { color rgbt 1 }
finish{ reflection { 0.1 / 1 } }
}
...
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182 | Texture/Material/Finish | Definite Bug | 3.70 beta 40 | Low | High | multi-textured blobs in intersections / differences bro ... | Closed | |
3.70 beta 41 |
Task Description
Multi-textured blobs are broken with 3.7 beta 40 when used inside an intersection, as can be demonstrated by the following scene:
#default { texture { pigment { rgb 1 } } }
camera {
right x*image_width/image_height
location <0,1.5,-4>
look_at <0,1,0>
}
light_source { <500,500,-500> color rgb 1 }
difference { blob {
threshold 0.6
sphere { < 0.75, 0, 0>, 1, 1 texture { pigment { color red 1 } } }
sphere { <-0.375, 0.65, 0>, 1, 1 texture { pigment { color green 1 } } }
sphere { <-0.375, -0.65, 0>, 1, 1 }
} }
With POV-Ray 3.7.0 beta 40, the entire blob is rendered with the default texture.
The same problem can be seen with “difference” or “merge” instead of “intersection”.
Omitting the CSG “envelope”, using “union”, or assigning the blob to a variable first and then using it inside an intersection, will yield the expected result.
POV-Ray 3.62 renders all variants as expected.
According to initial analysis, the problem appears to be caused by the dual use of the “MULTITEXTURE_FLAG”, which is used in CSG to indicate use of the “cutaway_textures” feature, and in blobs to indicate per-element texturing. (The same flag is also used in meshes to indicate per-face or per-vertex texturing, so similar problems are to expected there.)
My proposal is to use an entirely separate flag for the “cutaway_textures” feature (the blob and mesh can safely continue to share the MULTITEXTURE_FLAG).
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7 | Radiosity | Unimp. Feature/TODO | 3.70 beta 32 | Low | Medium | Re-implement Radiosity render abort/continue support | Tracked on GitHub | |
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Task Description
For proper render abort/continue support, radiosity cache data must be written to (or read from) disk even if the user does not explicitly opt to have a sample data file written/read. This feature has temporarily been dropped from 3.7 beta and is still pending re-implementation.
To meet high-reproducibility requirements in conjunction with SMP operation, it may be necessary to extend the 3.6 radiosity cache file format.
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61 | Other | Definite Bug | 3.70 beta 34 | Low | Medium | Dispersion does not give proper results | Closed | |
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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.
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210 | Geometric Primitives | Definite Bug | 3.70 RC3 | Low | Medium | UV mapping broken for parametric | Closed | |
3.70 RC4 |
Task Description
UV-mapped textures for parametrics are broken in POV-Ray 3.70 RC3, in cases where two (or more) parametrics overlap in a scene.
In the following scene, note how the texture per se is always taken properly from whichever parametric is in front, while the UV coordinates are erroneously taken always from the red parametric where both overlap, no matter whether it is in front or back.
camera {
location <0.0, 1.5, -3.0>
direction 1.5*z
right x*image_width/image_height
look_at 0
}
light_source { <-30, 30, -30> color rgb 1 }
#declare Param = parametric {
function { u*v*sin (15*v) },
function { v },
function { u*v*cos (15*v) }
0, 1
contained_by { box { -1,1 } }
accuracy 0.002
precompute 15 x,y,z
rotate 180*x
translate <0.3,0.5,0>
}
object {
Param
uv_mapping
texture {
pigment {
gradient x frequency 3
color_map {
[0 color red .5 ]
[1 color red 1 ]
}
}
}
}
object {
Param
uv_mapping
texture {
pigment {
gradient x frequency 7
color_map {
[0 color green .5 ]
[1 color green 1 ]
}
}
}
rotate y*180
}
POV-Ray 3.62 renders the scene properly.
As this bug has been found during code inspection, the uderlying cause has already been identified; I’m currently working on a fix.
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51 | Parser/SDL | Definite Bug | 3.70 beta 32 | Very Low | Critical | POV-Ray crashes hard on missing parenthesis | Closed | |
3.70 beta 35 |
Task Description
The following (bogus) SDL code causes POV-Ray 3.7 beta to crash hard with an access violation:
#include "fubar.inc"
Bar(42)
#macro FooBar() #end
//fubar.inc
#macro Foo(Fnord) #end
#macro Bar(Ignord) Foo(23 #end
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59 | Geometric Primitives | Definite Bug | 3.70 beta 34 | Very Low | High | Cone intersection test broken | Closed | |
3.70 beta 35 |
Task Description
The following scene, showing an almost cylindrical cone floating above a plane, renders fine in POV 3.6.2, but is obviously broken in 3.7.0.beta.34:
camera {
right x
up y*image_height/image_width
location <80,50,40>
look_at <0,0,0>
}
light_source { <500,500,500> color rgb 1 }
cone {
<0,0,30>, 11.303000, <0,0,-30>, 11.302999
texture { pigment { color rgb 1 } }
}
plane { y, -20 texture { pigment { color rgb 0.3 } } }
The error occurs even with the -MB option, indicating that the problem has nothing to do with bounding, but is in the cone intersection testing code.
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238 | Parser/SDL | Possible Bug | 3.70 RC4 | Very Low | High | Error during #read causes file to be kept open | Closed | |
3.70 RC7 |
Task Description
Consider the following script:
#fopen F "foo.txt" read
#read (F, Foo)
#debug concat ("'", Foo, "'\n")
#fclose F
Now assume that foo.txt erroneously contains unquoted text (which will result in a parse error):
Blah
When the error is reported, POV-Ray for Windows will helpfully open foo.txt, but any attempt to save a corrected version of foo.txt will fail until you exit the POV-Ray GUI, presumably because foo.txt is not properly closed by the parser.
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306 | Subsurface Scattering | Definite Bug | 3.70 RC7 | Very Low | High | finish subsurface block before global_settings subsurfa... | Tracked on GitHub | |
3.71 release |
Task Description
The following scene causes a crash:
sphere {
<0,0,0>, 1
finish { subsurface { translucency 1.0 } }
}
global_settings {
subsurface { }
}
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10 | Parser/SDL | Feature Request | 3.70 beta 32 | Very Low | Medium | Add support for specifying input images' gamma pre-corr ... | Closed | |
3.70 beta 40 |
Task Description
Input image files may have been created with gamma pre-correction for some specific target gamma, which may vary from image to image. Some file formats like PNG or HDR support embedding gamma pre-correction information in the image file, but this information may be missing or faulty, and some formats don’t support it at all. Additionally, it may be desirable to tamper with an input image’s gamma for artistic reasons.
Therefore, I suggest adding a means to explicitly specify input images’ originally intended target gamma on a per-image basis, like:
image_map { jpeg "MyImage.jpg" assumed_gamma 1.8 }
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39 | Distribution | Definite Bug | 3.70 beta 32 | Very Low | Medium | "cats" and "life" sample scenes broken | Closed | |
3.70 release |
Task Description
The following files were garbled in changelist #4648 by stripping all line terminators, making the files unusable:
.../scenes/advanced/cats/cattext.inc
.../scenes/animations/life/blink4.inc
.../scenes/animations/life/walker.inc
Line terminators of these files were already problematic in previous versions of the file, having been CR-only.
The following files changed with #4648 should be reviewed closely as well, as they were previously CR-only, too, and at least some of them exhibit some peculiarities regarding line and/or file terminators:
.../scenes/animations/pentmap/pentmap.ini
.../scenes/animations/pentmap/pentmap.pov
.../scenes/animations/slinky/slnk.ini
.../scenes/incdemo/metals/metals.doc
.../scenes/incdemo/stones/stones.doc
.../scenes/incdemo/woods/morewood.doc
.../scenes/incdemo/woods/woods.doc
.../scenes/textures/pigments/skies/skies.doc
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42 | Other | Definite Bug | 3.70 beta 32 | Very Low | Medium | command line parameters are not parsed properly on Unix | Tracked on GitHub | |
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Task Description
POV-Ray does not follow common practice on command-line handling; for instance:
povray +i"My File"
entered on a Unix shell would be passed to POV-Ray as
povray
+iMy File
(each line representing a distinct parameter here), which POV-Ray would further dissect, interpreting it as
povray
+iMy
File
To achieve the desired effect, one would actually have to quote the string twice:
povray +i"'My File'"
which the shell would translate to
povray
+i'My File'
which POV-Ray would interpret as
povray
+iMy File
In both cases, this is obviously not what a Unix user would expect.
The further dissecting of individual command-line parameters may have had its valid roots in the peculiarities of DOS’ command-line handling, but to my knowledge all major contemporary operating systems follow a concept akin to Unix, passing a list of parameters instead of a monolithic command line, and burdening the respective command shells with the task of dissecting command lines into parameters.
Therefore I suggest to disable this anachronistic feature in favor of contemporary standards; a compiler flag might be used to allow for easy re-enabling of the feature, for compiling POV-Ray on exotic targets.
- edit -
It has been pointed out that the described behaviour differs from 3.6, so I’m promoting this to a bug and changing the title.
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50 | Runtime error | Possible Bug | 3.70 beta 32 | Very Low | Medium | Frequent segfaults with photon scenes | Tracked on GitHub | |
|
Task Description
I observe frequent segfaults with POV-Ray 3.7 betas when rendering scenes using photons:
Segfaults are sporadic but frequent (occurring in roughly 50% of all photon renders).
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57 | Texture/Material/Finish | Definite Bug | 3.70 beta 34 | Very Low | Medium | Compressed TIFF image_map renders all transparent | Closed | |
|
Task Description
The attached TIFF file was created with IC using compression. When used in an image_map, POV-Ray 3.7.0.beta.34 on Windows XP x64 renders the image all transparent, while POV-Ray 3.6.2 renders the file fine. The same effect can be seen with LZW-compressed TIFF files created with Adobe Photoshop 6.0.
Uncompressed TIFF files created with either IC or Photoshop render fine in both versions of POV-Ray.
Stepping through the code of POV-Ray 3.7.0 shows that the same code path is taken regardless of compression, but the libtiff library returns different alpha channel values, indicating a problem in that library. POV-Ray 3.7 still uses libtiff 3.6.1, whereas the POV-Ray 3.6 branch has been updated to libtiff 3.8.2, which according to the change history includes a few alpha-related changes.
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60 | Geometric Primitives | Definite Bug | 3.70 beta 34 | Very Low | Medium | Artifacts using prism in CSG | Tracked on GitHub | |
Future release |
Task Description
Using prisms in intersecion or difference CSG objects may cause artifacts in POV-Ray 3.6.2 as well as 3.7.0.beta.34, as demonstrated by the following code:
camera {
right -x
up y*image_height/image_width
location <-24,19,12>
look_at <0,0,0>
}
light_source { <100,200,100> color rgb 1 }
plane { y, -2 pigment { color rgb 1 } }
#declare KeyValue = 1.366; // pick any you like
difference {
prism {
linear_sweep -0.5,0.5, 4
<-3,20-17>,
<-3,KeyValue>,
<-6,-3>,
<-0,-5>
}
intersection {
cylinder { <-7,-0.51,1>, <-7, 0.51,1>, 4.0 }
plane { z, KeyValue }
}
pigment { color rgb 0.5 }
}
Apparently the surface of the other object becomes visible when it exactly coincides with a vertex of the prism; probably there is a failure of the inside() test for such values.
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93 | Photons | Definite Bug | 3.70 beta 36 | Very Low | Medium | Photons are unnaturally amplified by pass_through objec ... | Closed | |
3.70 release |
Task Description
The following scene shows how photons are “boosted” by pass_through objects; removing one of the boxes will reduce the effect; the effect can be seen with 3.6 as well as current betas:
global_settings {
max_trace_level 10 // makes a difference!
photons { spacing 0.02 }
}
camera {
right x*image_width/image_height
location <0,2.6,-10>
look_at <0,0.75,0>
}
light_source {
<500,500,150>
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 <1.0, 0.8, 0.6> } }
}
#declare M_Glass=
material {
texture {
pigment {rgbt 1}
finish {
ambient 0.0
diffuse 0.05
specular 0.6
roughness 0.005
reflection { 0.1, 1.0 fresnel on }
conserve_energy
}
}
interior {
ior 1.5
fade_power 1001
fade_distance 0.9
fade_color <0.5,0.8,0.6>
}
}
sphere {
<1.1,1,-1.3>, 1
material { M_Glass }
photons {
target 1.0
refraction on
reflection on
}
}
cylinder {
<-1.2,0.01,0.8>, <-1.2,2.5,0.8>, 1
material { M_Glass }
photons { // photon block for an object
target 1.0
refraction on
reflection on
}
}
box {
<2.4,0,-2.3>, <2.6,4,-0.3>
material { M_Glass }
photons { pass_through }
}
box {
<2.9,0,-2.3>, <3.1,4,-0.3>
material { M_Glass }
photons { pass_through }
}
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251 | Parser/SDL | Possible Bug | 3.70 RC6 | Very Low | Medium | Scene / include files of >2GB size may cause problems | Tracked on GitHub | |
3.71 release |
Task Description
Code inspection shows that we’re still using fseek() and ftell() in various places (including text file input), which can’t handle file positions of 2GB and beyond (except on 64-bit linux machines); those calls need to be examined and (where appropriate) replaced with the fseek64() macro we’re already defining (but currently not using), and a to-be-defined ftell64() macro.
One potential (untested) error scenario would be a scene file calling a macro that is defined at the end of a > 2GB long include file.
|
|
4 | Subsurface Scattering | Unimp. Feature/TODO | 3.70 beta 32 | Very Low | Low | Integrate Subsurface Scattering with standard lighting ... | Tracked on GitHub | |
Future release |
Task Description
Subsurface Scattering still uses its own rudimentary code to compute illumination from classic light sources; this must be changed to use the standard light source & shadow handling code, to add support for non-trivial light sources (e.g. spotlights, cylindrical lights, area lights), partially-transparent shadowing objects etc.
|
|
5 | Subsurface Scattering | Unimp. Feature/TODO | 3.70 beta 32 | Very Low | Low | Integrate Subsurface Scattering with Radiosity | Closed | |
Future release |
Task Description
Subsurface scattering must be made radiosity-aware.
|
|
9 | Parser/SDL | Feature Request | 3.70 beta 32 | Very Low | Low | Add support for tuning brightness of image-mapped sky s ... | Closed | |
3.70 RC4 |
Task Description
Adjusting the brightness of an image-mapped sky sphere, although not an uncommon task especially when using HDR light probes, currently is cumbersome at best, as it is not possible to specify a “finish { ambient ... }” statement.
To simplify tuning a sky sphere’s brightness, I suggest introducing a “brightness FLOAT” modifier (defaulting to 1.0) to either the sky_sphere block or (as a more versatile solution) the image_map statement.
|
|
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.
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|
44 | Radiosity | Feature Request | All | Very Low | Low | Improve Normals Handling in Radiosity | Tracked on GitHub | |
Future release |
Task Description
Currently, radiosity does not make use of the fact that pertubed normals would theoretically just require a different weighting of already-sampled rays, leading to the following issues:
Honoring normal pertubations in radiosity leads to an increased number of samples, slowing down sample cache lookup.
The increased number of samples is generated from a proportionally higher number of sample rays, slowing down pretrace even further.
Low-amplitude pertubations tend to be smoothed out; “reviving” these is only possible by increasing the general sample density.
Handling of multi-layered textures with different normal pertubations is currently poorly implemented.
As a solution, I propose to store for each radiosity sample not only the resulting illumination for a perfectly unpertubed normal, but from the same set of sample rays also compute the illumination for an additional set of about a dozen standardized pertubed-normal directions, and interpolate among these when computing the radiosity-based illumination for a particular point that has a pertubed normal.
For backwards compatibility, this method of dealing with pertubed normals in radiosity might be activated by a different value for the “normal” statement in the radiosity block, say, “normal 2”.
|
|
45 | Distribution | Possible Bug | 3.70 beta 32 | Very Low | Low | Check & update sample scenes | Closed | |
3.70 release |
Task Description
Some sample scenes are no longer up-to-date, causing warnings, and should be fixed. For instance, the advanced/benchmark scene still includes “Buffer_Output=Off” and “Buffer_Size=0” in its .ini file. This should be checked systematically, and fixed as appropriate.
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|
49 | Texture/Material/Finish | Possible Bug | 3.70 beta 32 | Very Low | Low | number_of_waves default value not properly initialized | Closed | |
|
Task Description
When rendering a series of scenes (e.g. animation, or render queue in POV-Ray for Windows), number_of_waves is not properly reset to its default value between scenes, causing the parameter to default to the value set by the previous scene.
For instance, rendering the following scenes from a queue will cause “arches.pov” to be rendered differently the second time:
scenes\textures\finishes\arches.pov
scenes\textures\normals\normavg.pov
scenes\textures\finishes\arches.pov (again!)
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52 | Parser/SDL | Possible Bug | 3.70 beta 32 | Very Low | Low | inside() function does not accept meshes despite valid ... | Closed | |
|
Task Description
The parser does not accept mesh objects (or CSG objects including a mesh object) as a parameter to the inside() built-in function, reporting error “Solid object identifier expected”, even if the mesh is “solidified” by specifying an inside_vector.
(see news://news.povray.org:119/4a983716@news.povray.org)
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54 | Texture/Material/Finish | Definite Bug | 3.70 beta 32 | Very Low | Low | Multi-textured blobs fail to increment trace level | Closed | |
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Task Description
Trace level is not handled properly with blobs using per-component reflective or refractive textures, leading to lockups. Stepping through the code, it seems that POV-Ray fails to properly mark the blob object as increasing the trace level.
(Until this bug is fixed, the issue can be worked around in most cases by assigning a reflective texture to the blob as a whole.)
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65 | Parser/SDL | Feature Request | 3.70 beta 34 | Very Low | Low | Add support for vectors with functions | Tracked on GitHub | |
Future release |
Task Description
Being able to have functions operate on vectors would be pretty nice to have.
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67 | Texture/Material/Finish | Definite Bug | All | Very Low | Low | alpha channel in image map is ignored for shadows | Closed | |
3.70 beta 37 |
Task Description
In the following scene, the mesh object will always cast a fully-opaque shadow, even if the image has an alpha channel:
camera {
location <0.5, 1.0, -1.0>
look_at <0.5, 0.0, 0.5>
}
light_source { <0, 30, 0> color rgb 1 }
mesh {
triangle { <0,0,0>, <1,0,0>, <1,0,1> uv_vectors <0,0>, <1,0>, <1,1> }
triangle { <0,0,0>, <1,0,1>, <0,0,1> uv_vectors <0,0>, <1,1>, <0,1> }
texture { pigment { uv_mapping image_map {png "FOOBAR.png"} } }
}
plane { y, -0.1 pigment { color rgb 1 } }
The following modification to the texture will give the expected results:
texture { uv_mapping pigment { image_map {png "FOOBAR.png"} } }
The problem can be observed with both POV-Ray 3.7 (tested with beta.34), as well as 3.6 (tested with 3.6.2).
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68 | Setup/Install | Possible Bug | 3.61 | Very Low | Low | Unix configure script does not accept newer libpng vers ... | Closed | |
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Task Description
The configure script for unix uses a dumb string compare to test whether libpng version is 1.2.5 or higher, leading it to reject (for instance) libpng 1.2.27 and unnecessarily compile and statically link the older libpng version it comes with.
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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.
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89 | Image format | Definite Bug | 3.70 beta 36 | Very Low | Low | PPM output garbled for bit depths other than 8 bits | Closed | |
3.70 beta 37 |
Task Description
When choosing PPM output with a bit depth other than 8 bits per color channel (e.g. +FP16), POV-Ray messes up the colors (see thread news://news.povray.org:119/4babb48f$1@news.povray.org)
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96 | Texture/Material/Finish | Feature Request | Not applicable | Very Low | Low | User-defined warps | Tracked on GitHub | |
Future release |
Task Description
User-defined warps would be nice to have, something along the lines of:
warp {
function { MyFnX(x,y,z) } // function to compute pattern-space x-coordinate from object-space <x,y,z> coordinate
function { MyFnY(x,y,z) } // ditto for pattern-space y coordinate
function { MyFnZ(x,y,z) } // ditto for pattern-space z coordinate
}
// a displacement warp:
warp {
function { x + MyFnX(x,y,z) }
function { y + MyFnY(x,y,z) }
function { z + MyFnZ(x,y,z) }
}
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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.
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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.
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105 | User interface | Unimp. Feature/TODO | 3.70 beta 37 | Very Low | Low | output options not displayed | Closed | |
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Task Description
POV-Ray 3.7 does not show output options, such as:
Output Options
Image resolution 640 by 480 (rows 1 to 480, columns 1 to 640).
Output file: D:\foo\test.png, 24 bpp PNG
Graphic display......On (gamma: 2.2)
Mosaic preview.......Off
CPU usage histogram..Off
Continued trace......Off
(the above is what 3.6 used to show)
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106 | Distribution | Unimp. Feature/TODO | 3.70 beta 37 | Very Low | Low | Update sample scenes and include files for POV-Ray 3.7 ... | Tracked on GitHub | |
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Task Description
Most sample scenes and include files were designed at times when POV-Ray did not to any proper gamma handling, or still used the inferior 3.6 “assumed_gamma” mechanism.
All the scenes and include files should be reviewed, and updated to fit the new 3.7 gamma model.
The primary task will probably be gamma-adjusting literal color values and ambient parameters; I suggest using macros (which ideally should be defined in an include file) to be set according to the #version statement, so the scene/include file could be kept compatible with older versions.
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111 | Parser/SDL | Definite Bug | 3.70 beta 37a | Very Low | Low | Remove_Bounds=off / -UR does not work properly | Closed | |
3.70 beta 38 |
Task Description
Automatic removal of user-specified bounding boxes cannot be disabled in current POV-Ray 3.7 betas; the Remove_Bounds ini file setting and the +/-UR command line option are silently ignored.
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112 | Image format | Definite Bug | 3.70 beta 37a | Very Low | Low | OpenEXR alpha is only written when it shouldn't be | Closed | |
3.70 beta 38 |
Task Description
OpenEXR output currently writes an alpha channel when Output_Alpha=off (-UA), and does not write an alpha channel when Output_Alpha=on (+UA), i.e. doing it just the wrong way round.
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116 | Texture/Material/Finish | Definite Bug | 3.70 beta 37a | Very Low | Low | assertion fails when using "filter all" with small-pale ... | Closed | |
3.70 beta 38 |
Task Description
When using “filter all VALUE” with an image_map using a 4-bit (16-color) paletted bmp image, debug builds of POV-Ray fail with an assertion.
According to code analysis, other paletted image formats with <256 palette entries are also likely to be affected; similar assertion fails can be expected when using the “filter INDEX, VALUE” feature on such files with an index exceeding the palette size. “transmit” shows the same flaws.
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170 | Refactoring/Cleanup | Unimp. Feature/TODO | 3.70 beta 39 | Very Low | Low | Reduce memory footprint of output image buffer | Closed | |
3.70 release |
Task Description
Currently, output image is buffered using POV-Ray’s RGBFT color model and floating point values, leading to a memory consumption of 20 bit per pixel. This is an unproportionally large memory footprint, given that the only further processing performed on the buffered data is conversion of the data to the desired output file format, which will typically use only 3 bytes per pixel (at most 12 bit per pixel).
The situation can be improved by choosing the output image buffer container based on the desired output file format and parameters. To this end, the following code changes should be made:
Bundle image file format handler code into classes (typically one per file format)
Include a method to determine the best data container type for the image buffer
Instantiate the desired image file format handler object prior to rendering, querying the handler object for an image buffer
In addition to picking a suitable image data container from the already existing palette, careful design might also allow to use custom containers to directly pass the data to a library (in case the library provides its own buffering anyway), or write it directly to the output file (e.g. when writing image data to stdout). To make this compatible with multithreaded rendering, the following changes would have to be made:
Add code to detect when a row of SMP blocks has been finished, and call a certain method on the image handler object
Design the custom containers in such a way that they can buffer any number of unfinished SMP block rows as needed
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171 | Geometric Primitives | Definite Bug | 3.62 | Very Low | Low | CSG bounding box computation broken with shearing trans ... | Closed | |
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Task Description
Bounding box computation for CSG intersection appears to be broken when one member is an arbitrarily transformed plane.
// +W640 +H480 +MB1
#include "transforms.inc"
camera {
location <-0.2, 0.5, -4.0>
direction 1.5*z
right x*image_width/image_height
look_at <0.0, 0.0, 0.0>
}
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>]
}
}
}
light_source {
<0, 0, 0> // light's position (translated below)
color rgb <1, 1, 1> // light's color
translate <-30, 30, -30>
}
plane {
y, -1
pigment { color rgb <0.7,0.5,0.3> }
}
intersection {
sphere {
0.0, 1 }
plane { -x, 0 transform { Shear_Trans(x,y+x*0.3,z) } }
texture {
pigment {
radial
frequency 8
color_map {
[0.00 color rgb <1.0,0.4,0.2> ]
[0.33 color rgb <0.2,0.4,1.0> ]
[0.66 color rgb <0.4,1.0,0.2> ]
[1.00 color rgb <1.0,0.4,0.2> ]
}
}
finish{
specular 0.6
}
}
rotate -y*5
}
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172 | Image format | Unimp. Feature/TODO | 3.70 beta 39 | Very Low | Low | Re-implement progressive image output | Tracked on GitHub | |
Future release |
Task Description
With previous versions of POV-Ray, it was possible to turn off display output, but still assess the output during render by viewing the output file as it was progressively generated. This allowed e.g. to run a long render on a remote machine as a background process, and check the output from time to time via FTP or similar.
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173 | Other | Feature Request | 3.70 beta 39 | Very Low | Low | Prevent POV-Ray for Windows from stealing focus | Closed | |
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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.
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177 | Light source | Feature Request | 3.70 beta 39 | Very Low | Low | Add support for conserve_energy to shadow computations | Tracked on GitHub | |
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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
}
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178 | Texture/Material/Finish | Feature Request | 3.70 beta 39 | Very Low | Low | Modify metallic reflection code to better work with con... | Tracked on GitHub | |
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Task Description
The combination of metallic reflection with conserve_energy causes the reflection to lose colour, as demonstrated by the following scene:
global_settings {
max_trace_level 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
}
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=
material {
texture {
pigment {rgbt <1.0,0.7,0.2,0.99>}
finish {
ambient 0.0
diffuse 0.5
specular 0.6
roughness 0.005
reflection { 0.8, 1.0 metallic }
conserve_energy
}
}
interior { ior 1.5 }
}
box {
<-0.2,0,-2.3>, <0.0,4,0.3>
material { M }
rotate z*5
rotate x*2
}
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