| 148 |
|
... |
| 149 |
|
</pre> |
| 150 |
|
|
| 151 |
+ |
<p> |
| 152 |
+ |
|
| 153 |
|
A comment line begins with a pound sign, `#'. |
| 154 |
|
|
| 155 |
|
<p> |
| 396 |
|
0 |
| 397 |
|
</pre> |
| 398 |
|
|
| 399 |
+ |
<p> |
| 400 |
|
If the modifier is "void", then surfaces will |
| 401 |
|
use the modifiers given in the original description. |
| 402 |
|
Otherwise, the modifier specified is used in their place. |
| 441 |
|
0 |
| 442 |
|
</pre> |
| 443 |
|
|
| 444 |
+ |
<p> |
| 445 |
+ |
|
| 446 |
|
If the modifier is "void", then surfaces will |
| 447 |
|
use the modifiers given in the original mesh description. |
| 448 |
|
Otherwise, the modifier specified is used in their place. |
| 537 |
|
4 red green blue maxrad |
| 538 |
|
</pre> |
| 539 |
|
|
| 540 |
+ |
<p> |
| 541 |
|
If maxrad is zero, then the surface will never be tested for shadow, although it may participate in an interreflection calculation. |
| 542 |
|
If maxrad is negative, then the surface will never contribute to scene illumination. |
| 543 |
|
Glow sources will never illuminate objects on the other side of an illum surface. |
| 586 |
|
3 red green blue |
| 587 |
|
</pre> |
| 588 |
|
|
| 589 |
+ |
While alternate materials that are reflective will appear as normal, |
| 590 |
+ |
indirect rays will use the mirror's reflectance rather than the |
| 591 |
+ |
alternate type. |
| 592 |
+ |
Transmitting materials are an exception, where both transmission and |
| 593 |
+ |
reflection will use the alternate type for all rays not specifically |
| 594 |
+ |
targeting virtual light sources. |
| 595 |
+ |
Therefore, transmitting alternate types should only have pure specular |
| 596 |
+ |
reflection if they reflect at all, to maintain a valid calculation. |
| 597 |
+ |
|
| 598 |
|
<p> |
| 599 |
|
|
| 600 |
+ |
The mirror material type reflects light sources only from the front side |
| 601 |
+ |
of a surface, regardless of any alternate material. |
| 602 |
+ |
If virtual source generation is desired on both sides, two coincident |
| 603 |
+ |
surfaces with opposite normal orientations may be employed to achieve |
| 604 |
+ |
this effect. |
| 605 |
+ |
The reflectance and alternate material type may be |
| 606 |
+ |
different for the overlapped surfaces, |
| 607 |
+ |
and the two sides will behave accordingly. |
| 608 |
+ |
|
| 609 |
+ |
<p> |
| 610 |
+ |
|
| 611 |
|
<dt> |
| 612 |
|
<a NAME="Prism1"> |
| 613 |
|
<b>Prism1</b> |
| 629 |
|
n A1 A2 .. An |
| 630 |
|
</pre> |
| 631 |
|
|
| 632 |
+ |
<p> |
| 633 |
+ |
|
| 634 |
|
The new direction variables dx, dy and dz need not produce a normalized vector. |
| 635 |
|
For convenience, the variables DxA, DyA and DzA are defined as the normalized direction to the target light source. |
| 636 |
|
See <a HREF="#Function">section 2.2.1</a> on function files for further information. |
| 674 |
|
3 source1 mirror1>source10 mirror2>mirror1>source3 |
| 675 |
|
</pre> |
| 676 |
|
|
| 677 |
+ |
<p> |
| 678 |
|
Normally, only one source is given per mist material, and there is an |
| 679 |
|
upper limit of 32 to the total number of active scattering sources. |
| 680 |
|
The extinction coefficient, if given, is added the the global |
| 695 |
|
P(theta) = (1 - g*g) / (1 + g*g - 2*g*cos(theta))^1.5 |
| 696 |
|
</pre> |
| 697 |
|
|
| 698 |
+ |
<p> |
| 699 |
+ |
|
| 700 |
|
A perfectly isotropic scattering medium has a g parameter of 0, and |
| 701 |
|
a highly directional material has a g parameter close to 1. |
| 702 |
|
Fits to the g parameter may be found along with typical extinction |
| 711 |
|
0|3|6|7 [ rext gext bext [ ralb galb balb [ g ] ] ] |
| 712 |
|
</pre> |
| 713 |
|
|
| 714 |
+ |
<p> |
| 715 |
+ |
|
| 716 |
|
There are two usual uses of the mist type. |
| 717 |
|
One is to surround a beam from a spotlight or laser so that it is |
| 718 |
|
visible during rendering. |
| 867 |
|
<p> |
| 868 |
|
|
| 869 |
|
<dt> |
| 870 |
+ |
<a NAME="WGMDfunc"> |
| 871 |
+ |
<b>WGMDfunc</b> |
| 872 |
+ |
</a> |
| 873 |
+ |
|
| 874 |
+ |
<dd> |
| 875 |
+ |
WGMDfunc is a more programmable version of <a HREF="#Trans2">trans2</a>, |
| 876 |
+ |
with separate modifier paths and variables to control each component. |
| 877 |
+ |
(WGMD stands for Ward-Geisler-Moroder-Duer, which is the basis for |
| 878 |
+ |
this empirical model, similar to previous ones beside Ashik2.) |
| 879 |
+ |
The specification of this material is given below. |
| 880 |
+ |
<pre> |
| 881 |
+ |
mod WGMDfunc id |
| 882 |
+ |
13+ rs_mod rs rs_urough rs_vrough |
| 883 |
+ |
ts_mod ts ts_urough ts_vrough |
| 884 |
+ |
td_mod |
| 885 |
+ |
ux uy uz funcfile transform |
| 886 |
+ |
0 |
| 887 |
+ |
9+ rfdif gfdif bfdif |
| 888 |
+ |
rbdif gbdif bbdif |
| 889 |
+ |
rtdif gtdif btdif |
| 890 |
+ |
A10 .. |
| 891 |
+ |
</pre> |
| 892 |
+ |
|
| 893 |
+ |
<p> |
| 894 |
+ |
|
| 895 |
+ |
The sum of specular reflectance (<I>rs</I>), specular transmittance (<I>ts</I>), |
| 896 |
+ |
diffuse reflectance (<I>rfdif gfdif bfdif</I> for front and <I>rbdif gbdif bbdif</I> for back) |
| 897 |
+ |
and diffuse transmittance (<I>rtdif gtdif btdif</I>) should be less than 1 for each |
| 898 |
+ |
channel. |
| 899 |
+ |
|
| 900 |
+ |
<p> |
| 901 |
+ |
|
| 902 |
+ |
Unique to this material, separate modifier channels are |
| 903 |
+ |
provided for each component. |
| 904 |
+ |
The main modifier is used on the diffuse reflectance, both |
| 905 |
+ |
front and back. |
| 906 |
+ |
The <I>rs_mod</I> modifier is used for specular reflectance. |
| 907 |
+ |
If "void" is given for <I>rs_mod</I>, |
| 908 |
+ |
then the specular reflection color will be white. |
| 909 |
+ |
The special "inherit" keyword may also be given, in which case |
| 910 |
+ |
specular reflectance will share the main modifier. |
| 911 |
+ |
This behavior is replicated for the specular transmittance modifier |
| 912 |
+ |
<I>ts_mod</I>, which also has its own independent roughness expressions. |
| 913 |
+ |
Finally, the diffuse transmittance modifier is given as |
| 914 |
+ |
<I>td_mod</I>, which may also be "void" or "inherit". |
| 915 |
+ |
Note that any spectra or color for specular components must be |
| 916 |
+ |
carried by the named modifier(s). |
| 917 |
+ |
|
| 918 |
+ |
<p> |
| 919 |
+ |
|
| 920 |
+ |
The main advantage to this material over |
| 921 |
+ |
<a HREF="#BRTDfunc">BRTDfunc</a> and |
| 922 |
+ |
other programmable types described below is that the specular sampling is |
| 923 |
+ |
well-defined, so that all components are fully computed. |
| 924 |
+ |
|
| 925 |
+ |
<p> |
| 926 |
+ |
|
| 927 |
+ |
<dt> |
| 928 |
|
<a NAME="Dielectric"> |
| 929 |
|
<b>Dielectric</b> |
| 930 |
|
</a> |
| 985 |
|
tn = (sqrt(.8402528435+.0072522239*Tn*Tn)-.9166530661)/.0036261119/Tn |
| 986 |
|
</pre> |
| 987 |
|
|
| 988 |
+ |
<p> |
| 989 |
+ |
|
| 990 |
|
Standard 88% transmittance glass has a transmissivity of 0.96. |
| 991 |
|
(A <a HREF="#Patterns">pattern</a> modifying glass will affect the transmissivity.) |
| 992 |
|
If a fourth real argument is given, it is interpreted as the index of refraction to use instead of 1.52. |
| 1018 |
|
4+ red green blue spec A5 .. |
| 1019 |
|
</pre> |
| 1020 |
|
|
| 1021 |
+ |
<p> |
| 1022 |
+ |
|
| 1023 |
|
The function refl takes four arguments, the x, y and z |
| 1024 |
|
direction towards the incident light, and the solid angle |
| 1025 |
|
subtended by the source. |
| 1061 |
|
6+ red green blue rspec trans tspec A7 .. |
| 1062 |
|
</pre> |
| 1063 |
|
|
| 1064 |
+ |
<p> |
| 1065 |
+ |
|
| 1066 |
|
Where trans is the total light transmitted and tspec is the non-Lambertian fraction of transmitted light. |
| 1067 |
|
The function brtd should integrate to 1 over each projected hemisphere. |
| 1068 |
|
|
| 1090 |
|
A10 .. |
| 1091 |
|
</pre> |
| 1092 |
|
|
| 1093 |
+ |
<p> |
| 1094 |
+ |
|
| 1095 |
|
The variables rrefl, grefl and brefl specify the color coefficients for the ideal specular (mirror) reflection of the surface. |
| 1096 |
|
The variables rtrns, gtrns and btrns specify the color coefficients for the ideal specular transmission. |
| 1097 |
|
The functions rbrtd, gbrtd and bbrtd take the direction to the incident light (and its solid angle) and |
| 1136 |
|
4+ red green blue spec A5 .. |
| 1137 |
|
</pre> |
| 1138 |
|
|
| 1139 |
+ |
<p> |
| 1140 |
+ |
|
| 1141 |
|
The coordinate indices (x1, x2, etc.) are themselves functions of the x, y and z direction to the incident light, plus the solid angle |
| 1142 |
|
subtended by the light source (usually ignored). |
| 1143 |
|
The data function (func) takes five variables, the |
| 1304 |
|
0 |
| 1305 |
|
</pre> |
| 1306 |
|
|
| 1307 |
+ |
<p> |
| 1308 |
+ |
|
| 1309 |
|
The first modifier will also be used to shade the area leaving the antimatter volume and entering the regular volume. |
| 1310 |
|
If mod1 is void, the antimatter volume is completely invisible. |
| 1311 |
|
Antimatter does not work properly with the material type <a HREF="#Trans">"trans"</a>, |
| 1360 |
|
n A1 A2 .. An |
| 1361 |
|
</pre> |
| 1362 |
|
|
| 1363 |
+ |
<p> |
| 1364 |
+ |
|
| 1365 |
|
</dl> |
| 1366 |
|
|
| 1367 |
|
<p> |
| 1501 |
|
[spacing] |
| 1502 |
|
</pre> |
| 1503 |
|
|
| 1504 |
+ |
<p> |
| 1505 |
+ |
|
| 1506 |
|
or: |
| 1507 |
|
|
| 1508 |
|
<pre> |
| 1540 |
|
[spacing] |
| 1541 |
|
</pre> |
| 1542 |
|
|
| 1543 |
+ |
<p> |
| 1544 |
+ |
|
| 1545 |
|
or: |
| 1546 |
|
|
| 1547 |
|
<pre> |
| 1662 |
|
between nmA and nmB as its only argument, |
| 1663 |
|
and it returns the corresponding spectral intensity. |
| 1664 |
|
|
| 1665 |
+ |
<dt> |
| 1666 |
+ |
<a NAME="Specdata"> |
| 1667 |
+ |
<b>Specdata</b> |
| 1668 |
+ |
</a> |
| 1669 |
+ |
|
| 1670 |
+ |
<dd> |
| 1671 |
+ |
Specdata is like brightdata and colordata, but with more |
| 1672 |
+ |
than 3 specular samples. |
| 1673 |
+ |
|
| 1674 |
+ |
<pre> |
| 1675 |
+ |
mod specdata id |
| 1676 |
+ |
3+n+ |
| 1677 |
+ |
func datafile |
| 1678 |
+ |
funcfile x1 x2 .. xn transform |
| 1679 |
+ |
0 |
| 1680 |
+ |
m A1 A2 .. Am |
| 1681 |
+ |
</pre> |
| 1682 |
+ |
|
| 1683 |
+ |
<p> |
| 1684 |
+ |
The data file must have one more dimension than the coordinate |
| 1685 |
+ |
variable count, as this final dimension corresponds to the covered |
| 1686 |
+ |
spectrum. |
| 1687 |
+ |
The starting and ending wavelengths are specified in "datafile" |
| 1688 |
+ |
as well as the number of spectral samples. |
| 1689 |
+ |
The function "func" will be called with two parameters, the |
| 1690 |
+ |
interpolated spectral value for the current coordinate and the |
| 1691 |
+ |
associated wavelength. |
| 1692 |
+ |
If the spectrum is broken into 12 components, then 12 calls |
| 1693 |
+ |
will be made to "func" for the relevant ray evaluation. |
| 1694 |
+ |
|
| 1695 |
+ |
<dt> |
| 1696 |
+ |
<a NAME="Specpict"> |
| 1697 |
+ |
<b>Specpict</b> |
| 1698 |
+ |
</a> |
| 1699 |
+ |
|
| 1700 |
+ |
<dd> |
| 1701 |
+ |
Specpict is a special case of specdata, where the pattern is |
| 1702 |
+ |
a hyperspectral image stored in the common-exponent file format. |
| 1703 |
+ |
The dimensions of the image data are determined by the picture |
| 1704 |
+ |
just as with the colorpict primitive. |
| 1705 |
+ |
|
| 1706 |
+ |
<pre> |
| 1707 |
+ |
mod specpict id |
| 1708 |
+ |
5+ |
| 1709 |
+ |
func specfile |
| 1710 |
+ |
funcfile u v transform |
| 1711 |
+ |
0 |
| 1712 |
+ |
m A1 A2 .. Am |
| 1713 |
+ |
</pre> |
| 1714 |
+ |
|
| 1715 |
+ |
<p> |
| 1716 |
+ |
The function "func" is called with the interpolated pixel value |
| 1717 |
+ |
and the wavelength sample in nanometers, the same as specdata, |
| 1718 |
+ |
with as many calls made as there are components in "specfile". |
| 1719 |
+ |
|
| 1720 |
|
</dl> |
| 1721 |
|
|
| 1722 |
|
<p> |
| 1749 |
|
n A1 A2 .. An |
| 1750 |
|
</pre> |
| 1751 |
|
|
| 1752 |
+ |
<p> |
| 1753 |
+ |
|
| 1754 |
|
Foreground and background are modifier names that must be |
| 1755 |
|
defined earlier in the scene description. |
| 1756 |
|
If one of these is a material, then |
| 1779 |
|
m A1 A2 .. Am |
| 1780 |
|
</pre> |
| 1781 |
|
|
| 1782 |
+ |
<p> |
| 1783 |
+ |
|
| 1784 |
|
<dt> |
| 1785 |
|
<a NAME="Mixpict"> |
| 1786 |
|
<b>Mixpict</b> |
| 1825 |
|
[spacing] |
| 1826 |
|
</pre> |
| 1827 |
|
|
| 1828 |
+ |
<p> |
| 1829 |
+ |
|
| 1830 |
|
or: |
| 1831 |
|
|
| 1832 |
|
<pre> |
| 1842 |
|
[spacing] |
| 1843 |
|
</pre> |
| 1844 |
|
|
| 1845 |
+ |
<p> |
| 1846 |
+ |
|
| 1847 |
|
</dl> |
| 1848 |
|
|
| 1849 |
|
<p> |
| 1888 |
|
cfunc(x) : 10*x / sqrt(x) ; |
| 1889 |
|
</pre> |
| 1890 |
|
|
| 1891 |
+ |
<p> |
| 1892 |
+ |
|
| 1893 |
|
Many variables and functions are already defined by the program, and they are listed in the file rayinit.cal. |
| 1894 |
|
The following variables are particularly important: |
| 1895 |
|
|
| 1904 |
|
arg(i) - i'th real argument |
| 1905 |
|
</pre> |
| 1906 |
|
|
| 1907 |
+ |
<p> |
| 1908 |
+ |
|
| 1909 |
|
For mesh objects, the local surface coordinates are available: |
| 1910 |
|
|
| 1911 |
|
<pre> |
| 1912 |
|
Lu, Lv - local (u,v) coordinates |
| 1913 |
|
</pre> |
| 1914 |
|
|
| 1915 |
+ |
<p> |
| 1916 |
+ |
|
| 1917 |
|
For BRDF types, the following variables are defined as well: |
| 1918 |
|
|
| 1919 |
|
<pre> |
| 1922 |
|
CrP, CgP, CbP - perturbed material color |
| 1923 |
|
</pre> |
| 1924 |
|
|
| 1925 |
+ |
<p> |
| 1926 |
+ |
|
| 1927 |
|
A unique context is set up for each file so |
| 1928 |
|
that the same variable may appear in different |
| 1929 |
|
function files without conflict. |
| 1978 |
|
DATA, later dimensions changing faster. |
| 1979 |
|
</pre> |
| 1980 |
|
|
| 1981 |
+ |
<p> |
| 1982 |
+ |
|
| 1983 |
|
N is the number of dimensions. |
| 1984 |
|
For each dimension, the beginning and ending coordinate values and the dimension size is given. |
| 1985 |
|
Alternatively, individual coordinate values can be given when the points are not evenly spaced. |
| 2008 |
|
... |
| 2009 |
|
</pre> |
| 2010 |
|
|
| 2011 |
+ |
<p> |
| 2012 |
+ |
|
| 2013 |
|
The ASCII codes can appear in any order. N is the number of vertices, and the last is automatically connected to the first. |
| 2014 |
|
Separate polygonal sections are joined by coincident sides. |
| 2015 |
|
The character coordinate system is a square with lower left corner at (0,0), lower right at (255,0) and upper right at (255,255). |
| 2197 |
|
OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF |
| 2198 |
|
SUCH DAMAGE. |
| 2199 |
|
</pre> |
| 2200 |
+ |
|
| 2201 |
+ |
<p> |
| 2202 |
|
|
| 2203 |
|
<hr> |
| 2204 |
|
|
