Difference between revisions of "Documentation Talk:Tutorial Section 3.7"
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</tr> | </tr> | ||
</table> | </table> | ||
+ | |||
+ | ====Radiosity without conventional lighting==== | ||
+ | <!--<indexentry primary "Radiosity, without conventional lighting">---> | ||
+ | |||
+ | <p>You can also leave out all light sources and have pure radiosity lighting. The situation then is similar to a cloudy day outside, when the light comes from no specific direction but from the whole sky.</p> | ||
+ | |||
+ | <p>The following 2 images show what changes with the scene used in part 1, when the light source is removed (still using <code>recursion_limit 1</code>, <code>error_bound 0.2</code> and <code>low_error_factor 1.0</code>):</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadA14.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB_35.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">with light source</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">without light source</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>You can see that when the light source is removed the whole picture becomes very blue, because the scene is illuminated by a blue sky, while on a cloudy day, the color of the sky should be somewhere between grey and white.</p> | ||
+ | |||
+ | <p>We'll be using the sample scene <code>~/scenes/radiosity/radiosity3.pov</code> for demonstration now, although we will use different radiosity parameters again (same as those initially used for the conventionally-lit scene).</p> | ||
+ | |||
+ | <p>For starters, here it is with the default settings, our reference settings, and those maddeningly high-quality settings used earlier:</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB01.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB_22.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB99.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">default settings</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">tutorial reference settings</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">maddeningly high-quality settings</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>The default settings look much worse than in the first part, because they are mainly selected for use with conventional light sources; radiosity-only scenes are less forgiving to low-quality settings.</p> | ||
+ | |||
+ | <p>The following images demonstrate the effect of different settings for <code>recursion_limit</code>:</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB03.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB_22.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB04.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">recursion_limit 1</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">recursion_limit 3</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">recursion_limit 2</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB0203.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB0204.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">recursion_limit 1 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">recursion_limit 2 (difference)</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>The next three images show the effect of <code>error_bound</code>. Without light sources, this is even more important than with, good values mostly depend on the scenery and the other settings, lower values do not necessarily lead to better results. (We're using our <code>error_bound 0.5</code> image as reference.)</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB05.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB06.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB07.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">error_bound 0.01</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">error_bound 1.0</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">error_bound 1.8</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB0205.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB0206.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB0207.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">error_bound 0.01 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">error_bound 1.0 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">error_bound 1.8 (difference)</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>If there are artifacts it often helps to increase <code>count</code>, it does affect quality in general and often helps removing them (the following three images use <code>error_bound 0.2</code>).</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB09.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB08.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB10.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">count 2</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">count 50</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">count 200</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB0809.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB0810.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">count 35 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">count 150 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>As can be seen upon closer inspection however, this is no magic cure-all - some bright speckles remain even with extremely high <code>count</code> values.</p> | ||
+ | |||
+ | <p>In this case, the reason is that the pretrace is simply too short to provide the number of samples we aim for. This is a job for <code>pretrace_end</code>: Together with <code>pretrace_start</code> it specifies how many pretrace steps are done, and how high their resolution is. Lower values of <code>pretrace_end</code> lead to more pretrace steps and more accurate results but also to significantly slower rendering.</p> | ||
+ | |||
+ | <p>We're still using <code>error_bound 0.1</code> for these images.</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB11.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB08.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB12.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">pretrace_end 0.4</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">pretrace_end 0.01</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">pretrace_end 0.001</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB0811.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB0812.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">pretrace_end 0.4 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">pretrace_end 0.001 (difference)</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>The next sequence shows the effect of <code>nearest_count</code>, the difference is not very strong, but larger values always lead to better results (maximum is 20). We'll be using <code>error_bound 0.5</code> again, but also the following modifications to emphasize the effect: <code>recursion_limit 1</code>, <code>low_error_factor 1.0</code> and <code>pretrace_end 0.001</code>; from now on we'll stick to these values.</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB14.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB15.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB16.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">nearest_count 2</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">nearest_count 5 (default)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">nearest_count 20</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB1314.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB1315.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB1316.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">nearest_count 2 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">nearest_count 5 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">nearest_count 20 (difference)</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>The <code>minimum_reuse</code> is a geometric value related to the size of the render in pixel and affects whether previous radiosity calculations are reused at a new point. Lower values lead to more often and therefore more accurate calculations, but care must be taken to balance this setting with the others.</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB17.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB18.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB13.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">minimum_reuse 0.1</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">minimum_reuse 0.015 (default)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">minimum_reuse 0.05</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB1317.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB1318.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">minimum_reuse 0.1 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">minimum_reuse 0.015 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>In most cases it is not necessary to change the <code>low_error_factor</code>. This factor reduces the <code>error_bound</code> value during the final pretrace step. Changing this value can sometimes help to remove persistent artifacts.</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB19.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB13.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB20.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">low_error_factor 0.01</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">low_error_factor 0.5 (default)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">low_error_factor 1.0</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB1319.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB1320.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">low_error_factor 0.01 (difference)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">low_error_factor 1.0 (difference)</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p><code>gray_threshold</code> reduces the color in the radiosity calculations. As mentioned above the blue sky affects the color of the whole scene when radiosity is calculated. To reduce this coloring effect without affecting radiosity in general you can increase <code>gray_threshold</code>. 1.0 means no color in radiosity at all.</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB13.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB21.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB22.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">gray_threshold 0.0 (default)</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">gray_threshold 0.5</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">gray_threshold 1.0</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>It is worth experimenting with the things affecting radiosity to get some feeling for how things work. The next 3 images show some more experiments. (We're back with the original reference settings from now on.)</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB23.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB24.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB25.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">emission 3 for two objects</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">emission 0.3 for all objects, sky: emission 0</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">emission -3 for one object</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>Finally you can strongly change the appearance of the whole scene with the sky's texture. The following images give some examples.</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10px"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB26.png|center|220px<!--class="leftpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB27.png|center|220px<!--class="centerpanel"--->]] | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB28.png|center|220px<!--class="rightpanel"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <p class="caption">rgb <1,0.8,0> to blue 1 gradient from left to right</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">light-dark gradient from left to right</p> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">light-dark gradient from bottom to top</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | <p>Really good results mostly depend on the single situation and how the scene is meant to look. Here is some <em>higher quality</em> render of this particular scene, but requirements can be much different in other situations.</p> | ||
+ | |||
+ | <table class="matte" width="700px" cellpadding="0" cellspacing="10"> | ||
+ | <tr> | ||
+ | <td> | ||
+ | <pre> | ||
+ | global_settings { | ||
+ | radiosity { | ||
+ | pretrace_start 0.128 | ||
+ | pretrace_end 0.002 | ||
+ | count 500 | ||
+ | nearest_count 20 | ||
+ | error_bound 0.5 | ||
+ | recursion_limit 2 | ||
+ | low_error_factor 1.0 | ||
+ | gray_threshold 0.0 | ||
+ | minimum_reuse 0.005 | ||
+ | maximum_reuse 0.1 | ||
+ | brightness 1 | ||
+ | adc_bailout 0.005 | ||
+ | } | ||
+ | } | ||
+ | </pre> | ||
+ | </td> | ||
+ | <td> | ||
+ | [[Image:TutImgRadB29.png|center|320px<!--class="right"--->]] | ||
+ | </td> | ||
+ | </tr> | ||
+ | <tr> | ||
+ | <td> | ||
+ | </td> | ||
+ | <td> | ||
+ | <p class="caption">Higher quality radiosity scene</p> | ||
+ | </td> | ||
+ | </tr> | ||
+ | </table> | ||
+ | |||
+ | ====Normals and Radiosity==== | ||
+ | ====Performance Considerations==== |
Revision as of 20:43, 21 January 2011
Radiosity with conventional lighting
This section will introduce you to the technique of combining conventional and radiosity lighting. In this part of the tutorial, we'll be using basically the same sample scene that's located at ~/scenes/radiosity/radiosity2.pov
, however by changing various radiosity parameters, we'll be able to explore the effects that those changes can have on the scenes appearance and in some cases the render time. Later on, in this tutorial, you can find examples of pure radiosity illumination.
Note: Unless otherwise stated all the images in this section were rendered with the following radiosity settings:
global_settings { radiosity { pretrace_start 0.08 pretrace_end 0.01 count 150 nearest_count 10 error_bound 0.5 recursion_limit 3 low_error_factor 0.5 gray_threshold 0.0 minimum_reuse 0.005 maximum_reuse 0.2 brightness 1 adc_bailout 0.005 } }
Finally, a few more things about the scene setup. All objects except the sky have diffuse 0.65
and emission 0
in their finish block. The sky sphere has a bright blue pigment (what a surprise) with diffuse 0
and emission 1.0
as finish attributes.
Note: If using the sky_sphere
object, which does not support the finish
keyword, instead of a sphere
object that does, you will need define a #default
finish in order to affect it's finish properties.
For example:
#default {finish { diffuse 0 emission 1 }}
Hint: You can easily turn radiosity on/off with the use of a conditional statement.
#declare UseRad = yes; global_settings { #if (UseRad) radiosity { rad settings ... } #end }
OK, let's get started! In this set of images we first have the scene as it should appear without radiosity, in other words the radiosity
block has been removed, next with the settings noted above, and finally an image showing the difference between the two. Looking at the difference image, you can see that radiosity greatly affects the shadowed areas when applied in combination with conventional lighting.
Note: The use of emission 1
in the finish block of the blue sky is what gives the bluish touch of the whole scene in the radiosity version, as it functions as kind of a diffuse light source.
Radiosity is a highly tunable process, and it comes equipped with a variety of tunable parameters that make it easy to strike a balance between quality and rendering speed. However, as with most things, higher quality means more render time. Patience is a virtue.
For instance, let's examine our test object with default settings, with our reference settings, and finally with some maddeningly high-quality settings. For comparison, below each image you can see the difference to the high-quality version.
Changing the brightness
changes the intensity of radiosity effects. Theoretically specifying brightness 0
would be the same as without radiosity, however in practice POV-Ray doesn't accept a zero value. As a rule brightness 1
should work correctly in most cases. If the effects are too strong you can reduce this, though this is not recommended, as it's usually an indication that your textures are too bright and your illumination too dim. Larger values can lead to quite strange results in most cases.
The recursion_limit
setting primarily affects the brightness of shadows, nooks and corners. The following group of images show the results of setting this parameter to 1, 2 and 5 respectively ...
... while this next grouping shows the difference when compared to our reference setting of recursion_limit 3
. As you can see, values higher than 3 do not lead to any better results in such a quite simple scene. In most cases values of 1 or 2 are sufficient, especially for outdoor scenes.
The error_bound
setting mainly affects the structures of the shadows. Values larger than the default of 1.8 do not have much effect, they make the shadows even flatter. Extremely low values can lead to very good results, but the rendering time can become very long, and you may need to modify other parameters to avoid a grainy appearance.
Somewhat related to error_bound is low_error_factor
. It reduces error_bound setting during the pretrace phase, changing this can be useful to eliminate artifacts. The difference images used the low_error_factor 0.5
case for comparison.
This next sequence of images illustrate the effect of count
. It is a general quality and accuracy parameter leading to higher quality and slower rendering at higher values. Keep in mind that higher count
isn't necessarily a cure-for-all when it comes to quality. The difference images were compared to a count 150
case.
Note: Until otherwise noted the following settings are being used to emphasize the effects of the next parameters we'll be examining.
recursion_limit 1
error_bound 0.2
low_error_factor 1.0
Another parameter that affects quality is nearest_count
. You can use values ranging from 1 to 20 the default is 5. Just like count
, higher values can lead to less artifacts and smoother appearance but slower rendering. The nearest_count
setting also accepts a second parameter, which activates adaptive pretrace, providing a good means of speeding up pretrace without significant loss of quality (not shown here) the value must be smaller than the first parameter (e.g. nearest_count 20,10
). When set, POV-Ray will stop pretracing individual areas of the image where the average sample density already satisfies this second value, thereby avoiding tracing low-detail areas over and over again for little gain, while still being able to drill down deep into high-detail areas. A setting of nearest_count 10
was used for the comparison.
minimum_reuse
influences at which minimum distance previous radiosity samples are always reused during calculation, affecting quality and smoothness in nooks and corners. Higher values generally give a smoother appearance, at the cost of corner detail, while lower values may cause corners to look splotchy unless the other parameters (most notably count
and nearest_count
) are set for higher quality as well.
As minimum_reuse
must be lower than maximum_reuse
, to avoid a parse error with the highest setting we're using minimum_reuse 4.0
for these next three images.
Another important setting is pretrace_end
. It specifies how many pretrace steps are calculated and thereby strongly influences the speed. Usually lower values lead to better quality, but it is important to keep this in good relation to error_bound
.
Normally in the final trace no additional radiosity samples are taken unless absolutely needed. You can change this by adding always_sample on
allowing you to increase pretrace_end
to speed up rendering. Note however that this is very prone to artifacts such as visible render block boundaries and horizontal "smearing", so it is usually only useful for test renders. You should also use a low setting for nearest_count
, or you may actually increase the rendering time, and the probability of getting the mentioned artifacts!.
The effect of max_sample
is similar to brightness
. It does not reduce the radiosity effect in general but weakens samples with brightness above the specified value.
You can strongly affect things with an object's finish attributes. In fact that is the most important thing about radiosity. Normal objects should have an emission 0
(the default) finish. Objects with an emission setting greater than zero actually act as light sources in radiosity scenes. Remember that the default finish values used until now were diffuse 0.65
and emission 0
.
Finally you can vary the sky in outdoor radiosity scenes. In all these examples it is implemented with a sphere object.
finish { emission 1 diffuse 0 }
and the pigment of the original sample scene were used until now. The following images show some variations.
Radiosity without conventional lighting
You can also leave out all light sources and have pure radiosity lighting. The situation then is similar to a cloudy day outside, when the light comes from no specific direction but from the whole sky.
The following 2 images show what changes with the scene used in part 1, when the light source is removed (still using recursion_limit 1
, error_bound 0.2
and low_error_factor 1.0
):
You can see that when the light source is removed the whole picture becomes very blue, because the scene is illuminated by a blue sky, while on a cloudy day, the color of the sky should be somewhere between grey and white.
We'll be using the sample scene ~/scenes/radiosity/radiosity3.pov
for demonstration now, although we will use different radiosity parameters again (same as those initially used for the conventionally-lit scene).
For starters, here it is with the default settings, our reference settings, and those maddeningly high-quality settings used earlier:
The default settings look much worse than in the first part, because they are mainly selected for use with conventional light sources; radiosity-only scenes are less forgiving to low-quality settings.
The following images demonstrate the effect of different settings for recursion_limit
:
The next three images show the effect of error_bound
. Without light sources, this is even more important than with, good values mostly depend on the scenery and the other settings, lower values do not necessarily lead to better results. (We're using our error_bound 0.5
image as reference.)
If there are artifacts it often helps to increase count
, it does affect quality in general and often helps removing them (the following three images use error_bound 0.2
).
As can be seen upon closer inspection however, this is no magic cure-all - some bright speckles remain even with extremely high count
values.
In this case, the reason is that the pretrace is simply too short to provide the number of samples we aim for. This is a job for pretrace_end
: Together with pretrace_start
it specifies how many pretrace steps are done, and how high their resolution is. Lower values of pretrace_end
lead to more pretrace steps and more accurate results but also to significantly slower rendering.
We're still using error_bound 0.1
for these images.
The next sequence shows the effect of nearest_count
, the difference is not very strong, but larger values always lead to better results (maximum is 20). We'll be using error_bound 0.5
again, but also the following modifications to emphasize the effect: recursion_limit 1
, low_error_factor 1.0
and pretrace_end 0.001
; from now on we'll stick to these values.
The minimum_reuse
is a geometric value related to the size of the render in pixel and affects whether previous radiosity calculations are reused at a new point. Lower values lead to more often and therefore more accurate calculations, but care must be taken to balance this setting with the others.
In most cases it is not necessary to change the low_error_factor
. This factor reduces the error_bound
value during the final pretrace step. Changing this value can sometimes help to remove persistent artifacts.
gray_threshold
reduces the color in the radiosity calculations. As mentioned above the blue sky affects the color of the whole scene when radiosity is calculated. To reduce this coloring effect without affecting radiosity in general you can increase gray_threshold
. 1.0 means no color in radiosity at all.
It is worth experimenting with the things affecting radiosity to get some feeling for how things work. The next 3 images show some more experiments. (We're back with the original reference settings from now on.)
Finally you can strongly change the appearance of the whole scene with the sky's texture. The following images give some examples.
Really good results mostly depend on the single situation and how the scene is meant to look. Here is some higher quality render of this particular scene, but requirements can be much different in other situations.
global_settings { radiosity { pretrace_start 0.128 pretrace_end 0.002 count 500 nearest_count 20 error_bound 0.5 recursion_limit 2 low_error_factor 1.0 gray_threshold 0.0 minimum_reuse 0.005 maximum_reuse 0.1 brightness 1 adc_bailout 0.005 } } |
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