ViewVC Help
View File | Revision Log | Show Annotations | Download File | Root Listing
root/radiance/doc/ray.html
(Generate patch)

Comparing doc/ray.html (file contents):
Revision 1.3 by greg, Thu Jan 1 19:31:44 2004 UTC vs.
Revision 1.35 by greg, Fri Nov 17 20:02:07 2023 UTC

# Line 1 | Line 1
1   <html>
2 + <!-- RCSid $Id$ -->
3   <head>
4   <title>
5 < The RADIANCE 3.5 Synthetic Imaging System
5 > The RADIANCE 6.0 Synthetic Imaging System
6   </title>
7   </head>
8   <body>
9  
9 – Copyright � 2003 Regents, University of California
10 –
10   <p>
11  
12   <h1>
13 < The RADIANCE 3.5 Synthetic Imaging System
13 > The RADIANCE 6.0 Synthetic Imaging System
14   </h1>
15  
16   <p>
17  
18 < Building Technologies Department<br>
18 > Building Technologies Program<br>
19   Lawrence Berkeley National Laboratory<br>
20   1 Cyclotron Rd., 90-3111<br>
21   Berkeley, CA  94720<br>
# Line 84 | Line 83 | The diagram in Figure 1 shows the flow between program
83   (ovals).  
84   The central program is <i>rpict</i>, which produces a picture from a scene
85   description.
86 < <i>Rview</i> is a  variation  of  rpict  that  computes  and displays images
86 > <i>Rvu</i> is a  variation  of  rpict  that  computes  and displays images
87   interactively, and rtrace computes single ray values.
88   Other programs (not shown) connect many of these elements together,
89   such as the executive programs
# Line 566 | Line 565 | A material defines the way light interacts with a  sur
565          </a>
566  
567   <dd>
568 <        Mirror is used for planar surfaces that produce  secondary source reflections.  
568 >        Mirror is used for planar surfaces that produce  virtual source reflections.  
569          This material should be used sparingly, as it may cause the light source calculation to  blow up  if  it is applied to many small surfaces.  
570          This material is only supported for flat surfaces  such  as  <a HREF="#Polygon">polygons</a>  and <a HREF="#Ring">rings</a>.  
571          The arguments are simply the RGB reflectance values, which should be between 0 and 1.  
# Line 589 | Line 588 | This is only appropriate if the surface hides other (m
588          </a>
589  
590   <dd>
591 <        The prism1 material is for  general  light  redirection from prismatic glazings, generating secondary light sources.
591 >        The prism1 material is for  general  light  redirection from prismatic glazings, generating virtual light sources.
592          It can only be used  to  modify  a  planar  surface  
593          (i.e.,  a <a HREF="#Polygon">polygon</a>  or <a HREF="#Ring">disk</a>)
594          and should not result in either light concentration or scattering.  
595          The new direction of the ray  can be  on either side of the material,
596 <        and the definitions must have the correct bidirectional properties to  work  properly with  secondary light sources.  
596 >        and the definitions must have the correct bidirectional properties to  work  properly with virtual light sources.  
597          The arguments give the coefficient for the redirected light and its direction.
598  
599   <pre>
# Line 661 | Line 660 | a perfectly scattering medium (no absorption).
660   The scattering eccentricity parameter will likewise override the global
661   setting if it is present.
662   Scattering eccentricity indicates how much scattered light favors the
663 < forward direction, as fit by the Heyney-Greenstein function:
663 > forward direction, as fit by the Henyey-Greenstein function:
664  
665   <pre>
666          P(theta) = (1 - g*g) / (1 + g*g - 2*g*cos(theta))^1.5
# Line 799 | Line 798 | unless the line integrals consider enclosed geometry.
798  
799   <dd>
800          Trans2 is the anisotropic version of <a HREF="#Trans">trans</a>.  
801 <        The string arguments  are  the same as for plastic2, and the real arguments are the same as  for  trans  but  with  an  additional roughness value.
801 >        The string arguments  are  the same as for <a HREF="#Plastic2">plastic2</a>,
802 >        and the real arguments are the same as  for  trans  but  with  an  additional roughness value.
803  
804   <pre>
805          mod trans2 id
# Line 811 | Line 811 | unless the line integrals consider enclosed geometry.
811   <p>
812  
813   <dt>
814 +        <a NAME="Ashik2">
815 +        <b>Ashik2</b>
816 +        </a>
817 +
818 + <dd>
819 +        Ashik2 is the anisotropic reflectance model by Ashikhmin & Shirley.
820 +        The string arguments are the same as for <a HREF="#Plastic2">plastic2</a>, but the real
821 +        arguments have additional flexibility to specify the specular color.
822 +        Also, rather than roughness, specular power is used, which has no
823 +        physical meaning other than larger numbers are equivalent to a smoother
824 +        surface.
825 +        Unlike other material types, total reflectance is the sum of
826 +        diffuse and specular colors, and should be adjusted accordingly.
827 + <pre>
828 +        mod ashik2 id
829 +        4+ ux uy uz funcfile transform
830 +        0
831 +        8 dred dgrn dblu sred sgrn sblu u-power v-power
832 + </pre>
833 +
834 + <p>
835 +
836 + <dt>
837          <a NAME="Dielectric">
838          <b>Dielectric</b>
839          </a>
# Line 1055 | Line 1078 | unless the line integrals consider enclosed geometry.
1078   <p>
1079  
1080   <dt>
1081 +        <a NAME="BSDF">
1082 +        <b>BSDF</b>
1083 +        </a>
1084 +
1085 + <dd>
1086 +        The BSDF material type loads an XML (eXtensible Markup Language)
1087 +        file describing a bidirectional scattering distribution function.
1088 +        Real arguments to this material may define additional
1089 +        diffuse components that augment the BSDF data.
1090 +        String arguments are used to define thickness for proxied
1091 +        surfaces and the &quot;up&quot; orientation for the material.
1092 +
1093 + <pre>
1094 +        mod BSDF id
1095 +        6+ thick BSDFfile ux uy uz funcfile transform
1096 +        0
1097 +        0|3|6|9
1098 +                rfdif gfdif bfdif
1099 +                rbdif gbdif bbdif
1100 +                rtdif gtdif btdif
1101 + </pre>
1102 +
1103 + <p>
1104 +        The first string argument is a &quot;thickness&quot; parameter that may be used
1105 +        to hide detail geometry being proxied by an aggregate BSDF material.
1106 +        If a view or shadow ray hits a BSDF proxy with non-zero thickness,
1107 +        it will pass directly through as if the surface were not there.
1108 +        Similar to the illum type, this permits direct viewing and
1109 +        shadow testing of complex geometry.
1110 +        The BSDF is used when a scattered (indirect) ray hits the surface,
1111 +        and any transmitted sample rays will be offset by the thickness amount
1112 +        to avoid the hidden geometry and gather samples from the other side.
1113 +        In this manner, BSDF surfaces can improve the results for indirect
1114 +        scattering from complex systems without sacrificing appearance or
1115 +        shadow accuracy.
1116 +        If the BSDF has transmission and back-side reflection data,
1117 +        a parallel BSDF surface may be
1118 +        placed slightly less than the given thickness away from the front surface
1119 +        to enclose the complex geometry on both sides.
1120 +        The sign of the thickness is important, as it indicates
1121 +        whether the proxied geometry is behind the BSDF
1122 +        surface (when thickness is positive) or in front (when
1123 +        thickness is negative).
1124 + <p>
1125 +        The second string argument is the name of the BSDF file,
1126 +        which is found in the usual auxiliary locations.  The
1127 +        following three string parameters name variables for an
1128 +        &quot;up&quot; vector, which together with the surface
1129 +        normal, define the local coordinate system that orients the
1130 +        BSDF.  These variables, along with the thickness, are defined
1131 +        in a function file given as the next string argument.  An
1132 +        optional transform is used to scale the thickness and
1133 +        reorient the up vector.
1134 + <p>
1135 +        If no real arguments are given, the BSDF is used by itself
1136 +        to determine reflection and transmission.  If there are at
1137 +        least 3 real arguments, the first triplet is an additional
1138 +        diffuse reflectance for the front side.  At least 6 real
1139 +        arguments adds diffuse reflectance to the rear side of the
1140 +        surface.  If there are 9 real arguments, the final triplet
1141 +        will be taken as an additional diffuse transmittance.  All
1142 +        diffuse components as well as the non-diffuse transmission
1143 +        are modified by patterns applied to this material.  The
1144 +        non-diffuse reflection from either side are unaffected.
1145 +        Textures perturb the effective surface normal in the usual
1146 +        way.
1147 + <p>
1148 +        The surface normal of this type is not altered to face the
1149 +        incoming ray, so the front and back BSDF reflections may
1150 +        differ.  (Transmission is identical front-to-back by physical
1151 +        law.) If back visibility is turned off during rendering and
1152 +        there is no transmission or back-side reflection, only then
1153 +        the surface will be invisible from behind.  Unlike other
1154 +        data-driven material types, the BSDF type is fully supported
1155 +        and all parts of the distribution are properly sampled.
1156 + <p>
1157 +
1158 + <dt>
1159 +        <a NAME="aBSDF">
1160 +        <b>aBSDF</b>
1161 +        </a>
1162 +
1163 + <dd>
1164 +        The aBSDF material is identical to the BSDF type with two
1165 +        important differences.  First, proxy geometry is not
1166 +        supported, so there is no thickness parameter.  Second, an
1167 +        aBSDF is assumed to have some specular through component
1168 +        (the &rsquo;a&rsquo; stands for &quot;aperture&quot;),
1169 +        which is treated specially during the direct calculation
1170 +        and when viewing the material.  Based on the BSDF data, the
1171 +        coefficient of specular transmission is determined and used
1172 +        for modifying unscattered shadow and view rays.
1173 +
1174 + <pre>
1175 +        mod aBSDF id
1176 +        5+ BSDFfile ux uy uz funcfile transform
1177 +        0
1178 +        0|3|6|9
1179 +             rfdif gfdif bfdif
1180 +             rbdif gbdif bbdif
1181 +             rtdif gtdif btdif
1182 + </pre>
1183 +
1184 + <p>
1185 +        If a material has no specular transmitted component, it is
1186 +        much better to use the BSDF type with a zero thickness
1187 +        than to use aBSDF.
1188 + <p>
1189 +
1190 + <dt>
1191          <a NAME="Antimatter">
1192          <b>Antimatter</b>
1193          </a>
# Line 1328 | Line 1461 | or:
1461          A section of text meant to  depict  a  picture, perhaps using a special purpose font such as hexbit4x1.fnt, calls for uniform  spacing.  
1462          Reasonable  magnitudes  for  proportional  spacing are between 0.1 (for tightly spaced characters) and 0.3 (for wide spacing).
1463  
1464 + <p>
1465 +
1466 + <dt>
1467 +        <a NAME="Spectrum">
1468 +        <b>Spectrum</b>
1469 +        </a>
1470 +
1471 + <dd>
1472 +        The spectrum primitive is the most basic type for introducing spectral
1473 +        color to a material.
1474 +        Since materials only provide RGB parameters, spectral patterns
1475 +        are the only way to superimpose wavelength-dependent behavior.
1476 +
1477 + <pre>
1478 +        mod spectrum id
1479 +        0
1480 +        0
1481 +        5+ nmA nmB s1 s2 .. sN
1482 + </pre>
1483 +
1484 + <p>
1485 +        The first two real arguments indicate the extrema of the
1486 +        spectral range in nanometers.
1487 +        Subsequent real values correspond to multipliers in at each wavelength.
1488 +        The nmA wavelength may be greater or less than nmB,
1489 +        but they may not be equal, and their ordering matches
1490 +        the order of the spectral values.
1491 +        A minimum of 3 values must be given, which would act
1492 +        more or less the same as a constant RGB multiplier.
1493 +        As with RGB values, spectral quantities normally range between 0
1494 +        and 1 at each wavelength, or average to 1.0 against a standard
1495 +        sensitivity functions such as V(lambda).
1496 +        The best results obtain when the spectral range and number
1497 +        of samples match rendering options, though resampling will handle
1498 +        any differences, zero-filling wavelenths outside the nmA to nmB
1499 +        range.
1500 +        A warning will be issued if the given wavelength range does not
1501 +        adequately cover the visible spectrum.
1502 +
1503 + <p>
1504 +
1505 + <dt>
1506 +        <a NAME="Specfile">
1507 +        <b>Specfile</b>
1508 +        </a>
1509 +
1510 + <dd>
1511 +        The specfile primitive is equivalent to the spectrum type, but
1512 +        the wavelength range and values are contained in a 1-dimensional
1513 +        data file.
1514 +        This may be a more convenient way to specify a spectral color,
1515 +        especially one corresponding to a standard illuminant such as D65
1516 +        or a library of measured spectra.
1517 +
1518 + <pre>
1519 +        mod specfile id
1520 +        1 datafile
1521 +        0
1522 +        0
1523 + </pre>
1524 +
1525 + <p>
1526 +        As with the spectrum type, rendering wavelengths outside the defined
1527 +        range will be zero-filled.
1528 +        Unlike the spectrum type, the file may contain non-uniform samples.
1529 +
1530 + <p>
1531 +
1532 + <dt>
1533 +        <a NAME="Specfunc">
1534 +        <b>Specfunc</b>
1535 +        </a>
1536 +
1537 + <dd>
1538 +        The specfunc primitive offers dynamic control over a spectral
1539 +        pattern, similar to the colorfunc type.
1540 +
1541 + <pre>
1542 +        mod specfunc id
1543 +        2+ sval funcfile transform
1544 +        0
1545 +        2+ nmA nmB A3 ..
1546 + </pre>
1547 +
1548 + <p>
1549 +        Like the spectrum primitive, the wavelength range is specified
1550 +        in the first two real arguments, and additional real values are
1551 +        accessible to the sval function.
1552 +        This function is fed a wavelenth sample
1553 +        between nmA and nmB as its only argument,
1554 +        and it returns the corresponding spectral intensity.
1555 +
1556   </dl>
1557  
1558   <p>
# Line 1338 | Line 1563 | or:
1563   </h4>
1564  
1565   A mixture is a blend of one or more materials or textures and patterns.
1566 + Blended materials should not be light source types or virtual source types.
1567   The basic types are given below.
1568  
1569   <p>
# Line 1367 | Line 1593 | A mixfunc mixes  two  modifiers  procedurally.   It  i
1593          which serves as a form of opacity control when used with a material.)
1594          Vname is the coefficient defined in funcfile that determines  the  influence  of  foreground.  
1595          The background coefficient is always (1-vname).  
1370 –        Since the references are not resolved until run-time,  the  last  definitions  of  the modifier id's will be used.  
1371 –        This can result in modifier loops, which are detected by the renderer.
1596  
1597   <p>
1598  
# Line 1412 | Line 1636 | A mixfunc mixes  two  modifiers  procedurally.   It  i
1636          arguments, the red, green and blue values
1637          corresponding to the pixel at (u,v).
1638  
1415 – </dl>
1639   <p>
1640  
1641   <dt>
# Line 1530 | Line 1753 | If no file is needed by a given primitive because all
1753   the  required  variables  are global,  
1754   a  period  (`.')  can be given in place of the file name.  
1755   It is also possible to give an expression instead
1756 < of a  straight  variable  name  in  a scene file,
1757 < although such expressions should be kept
1535 < simple if possible.
1536 < Also, functions (requiring parameters) must be given
1756 > of a  straight  variable  name  in  a scene file.
1757 > Functions (requiring parameters) must be given
1758   as names and not as expressions.
1759  
1760   <p>
# Line 1680 | Line 1901 | The details of this process  are  not  important, but
1901   directs the use of a scene description.
1902   <ul>
1903   <li>
1904 < <a NAME="rvu" HREF="../man_html/rvu.1.html"><b>Rview</b></a>  is  ray-tracing  program  for  viewing  a  scene interactively.  
1904 > <a NAME="rvu" HREF="../man_html/rvu.1.html"><b>Rvu</b></a>  is  ray-tracing  program  for  viewing  a  scene interactively.  
1905   When  the user specifies a new perspective, rvu quickly displays a rough image on the  terminal,  
1906   then progressively increases the resolution as the user looks on.
1907   He can select a particular section of the image to  improve, or  move  to  a different view and start over.  
# Line 1716 | Line 1937 | Pictures may be displayed directly under X11 using the
1937   or converted a standard image format using one of the following
1938   <b>translators</b>:
1939          <ul>
1940 <        <li> <b>Ra_avs</b>
1941 <                converts to and from AVS image format.
1721 <        <li> <a HREF="../man_html/ra_pict.1.html"><b>Ra_pict</b></a>
1722 <                converts to Macintosh 32-bit PICT2 format.
1940 >        <li> <a HREF="../man_html/ra_bmp.1.html"><b>Ra_bmp</b></a>
1941 >                converts to and from BMP image format.
1942          <li> <a HREF="../man_html/ra_ppm.1.html"><b>Ra_ppm</b></a>
1943                  converts to and from Poskanzer Portable Pixmap formats.
1725 –        <li> <a HREF="../man_html/ra_pr.1.html"><b>Ra_pr</b></a>
1726 –                converts to and from Sun 8-bit rasterfile format.
1727 –        <li> <a HREF="../man_html/ra_pr24.1.html"><b>Ra_pr24</b></a>
1728 –                converts to and from Sun 24-bit rasterfile format.
1944          <li> <a HREF="../man_html/ra_ps.1.html"><b>Ra_ps</b></a>
1945                  converts to PostScript color and greyscale formats.
1946          <li> <a HREF="../man_html/ra_rgbe.1.html"><b>Ra_rgbe</b></a>
# Line 1751 | Line 1966 | or converted a standard image format using one of the
1966   <pre>
1967   The Radiance Software License, Version 1.0
1968  
1969 < Copyright (c) 1990 - 2002 The Regents of the University of California,
1969 > Copyright (c) 1990 - 2021 The Regents of the University of California,
1970   through Lawrence Berkeley National Laboratory.   All rights reserved.
1971  
1972   Redistribution and use in source and binary forms, with or without
# Line 1785 | Line 2000 | are met:
2000        nor may &quot;Radiance&quot; appear in their name, without prior written
2001        permission of Lawrence Berkeley National Laboratory.
2002  
2003 < THIS SOFTWARE IS PROVIDED ``AS IS'' AND ANY EXPRESSED OR IMPLIED
2003 > THIS SOFTWARE IS PROVIDED ``AS IS&quot; AND ANY EXPRESSED OR IMPLIED
2004   WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES
2005   OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE
2006   DISCLAIMED.   IN NO EVENT SHALL Lawrence Berkeley National Laboratory OR
# Line 1824 | Line 2039 | Ecole  Polytechnique  Federale de Lausanne (EPFL Unive
2039   </h2>
2040   <p>
2041   <ul>
2042 +    <li>Ward, Gregory J., Bruno Bueno, David Geisler-Moroder,
2043 +      Lars O. Grobe, Jacob C. Jonsson, Eleanor
2044 +      S. Lee, Taoning Wang, Helen Rose Wilson,
2045 +      &quot;<a href="https://doi.org/10.1016/j.enbuild.2022.111890">Daylight
2046 +      Simulation Workflows Incorporating Measured Bidirectional
2047 +      Scattering Distribution Functions</a>&quot;
2048 +      <em>Energy &amp; Buildings</em>, Vol. 259, No. 11890, 2022.
2049 +    <li>Wang, Taoning, Gregory Ward, Eleanor Lee,
2050 +      &quot;<a href="https://authors.elsevier.com/a/1XQ0a1M7zGwT7v">Efficient
2051 +      modeling of optically-complex, non-coplanar exterior shading:
2052 +      Validation of matrix algebraic methods</a>&quot;
2053 +      <em>Energy & Buildings</em>, vol. 174, pp. 464-83, Sept. 2018.
2054 +    <li>Lee, Eleanor S., David Geisler-Moroder, Gregory Ward,
2055 +      &quot;<a href="https://eta.lbl.gov/sites/default/files/publications/solar_energy.pdf">Modeling
2056 +      the direct sun component in buildings using matrix
2057 +      algebraic approaches: Methods and
2058 +      validation</a>,&quot; <em>Solar Energy</em>,
2059 +      vol. 160, 15 January 2018, pp 380-395.
2060 +    <li>Narain, Rahul, Rachel A. Albert, Abdullah Bulbul,
2061 +       Gregory J. Ward, Marty Banks, James F. O'Brien,
2062 +       &quot;<a href="http://graphics.berkeley.edu/papers/Narain-OPI-2015-08/index.html">Optimal
2063 +       Presentation of Imagery with Focus
2064 +       Cues on Multi-Plane Displays</a>,&quot;
2065 +       <em>SIGGRAPH 2015</em>.
2066 +    <li>Ward, Greg, Murat Kurt, and Nicolas Bonneel,
2067 +        &quot;<a href="papers/WMAM14_Tensor_Tree_Representation.pdf">Reducing
2068 +        Anisotropic BSDF Measurement to Common Practice</a>,&quot;
2069 +        <em>Workshop on Material Appearance Modeling</em>, 2014.
2070 +    <li>Banks, Martin, Abdullah Bulbul, Rachel Albert, Rahul Narain,
2071 +        James F. O'Brien, Gregory Ward,
2072 +        &quot;<a href="http://graphics.berkeley.edu/papers/Banks-TPO-2014-05/index.html">The
2073 +        Perception of Surface Material from Disparity and Focus Cues</a>,&quot;
2074 +        <em>VSS 2014</em>.
2075 +    <li>McNeil, A., C.J. Jonsson, D. Appelfeld, G. Ward, E.S. Lee,
2076 +        &quot;<a href="http://gaia.lbl.gov/btech/papers/4414.pdf">
2077 +        A validation of a ray-tracing tool used to generate
2078 +        bi-directional scattering distribution functions for
2079 +        complex fenestration systems</a>,&quot;
2080 +        <em>Solar Energy</em>, 98, 404-14,
2081 +        November 2013.
2082 +    <li>Ward, G., R. Mistrick, E.S. Lee, A. McNeil, J. Jonsson,
2083 +        &quot;<a href="http://gaia.lbl.gov/btech/papers/4414.pdf">Simulating
2084 +        the Daylight Performance of Complex Fenestration Systems
2085 +        Using Bidirectional Scattering Distribution Functions within
2086 +        Radiance</a>,&quot;
2087 +        <em>Leukos</em>, 7(4)
2088 +        April 2011.
2089 +    <li>Cater, Kirsten, Alan Chalmers, Greg Ward,
2090 +        &quot;<a href="http://www.anyhere.com/gward/papers/egsr2003.pdf">Detail to Attention:
2091 +        Exploiting Visual Tasks for Selective Rendering</a>,&quot;
2092 +        <em>Eurographics Symposium
2093 +        on Rendering 2003</em>, June 2003.
2094      <li>Ward, Greg, Elena Eydelberg-Vileshin,
2095 <        ``<a HREF="http://viz.cs.berkeley.edu/~gwlarson/papers/egwr02/index.html">Picture Perfect RGB
2096 <        Rendering Using Spectral Prefiltering and Sharp Color Primaries</a>,''
2095 >        &quot;<a HREF="http://www.anyhere.com/gward/papers/egwr02/index.html">Picture Perfect RGB
2096 >        Rendering Using Spectral Prefiltering and Sharp Color Primaries</a>,&quot;
2097          Thirteenth Eurographics Workshop on Rendering (2002),
2098          P. Debevec and S. Gibson (Editors), June 2002.
2099      <li>Ward, Gregory,
2100 <        ``<a HREF="http://viz.cs.berkeley.edu/~gwlarson/papers/cic01.pdf">High Dynamic Range Imaging</a>,''
2100 >        &quot;<a HREF="http://www.anyhere.com/gward/papers/cic01.pdf">High Dynamic Range Imaging</a>,&quot;
2101          Proceedings of the Ninth Color Imaging Conference, November 2001.
2102      <li>Ward, Gregory and Maryann Simmons,
2103 <        ``<a HREF="http://viz.cs.berkeley.edu/~gwlarson/papers/tog99.pdf">
2103 >        &quot;<a HREF="http://www.anyhere.com/gward/papers/tog99.pdf">
2104          The Holodeck Ray Cache: An Interactive Rendering System for Global Illumination in Nondiffuse
2105 <        Environments</a>,'' ACM Transactions on Graphics, 18(4):361-98, October 1999.
2106 <    <li>Larson, G.W., ``<a HREF="http://viz.cs.berkeley.edu/~gwlarson/papers/ewp98.pdf">The Holodeck: A Parallel
2107 <        Ray-caching Rendering System</a>,'' Proceedings of the Second
2105 >        Environments</a>,&quot; ACM Transactions on Graphics, 18(4):361-98, October 1999.
2106 >    <li>Larson, G.W., &quot;<a HREF="http://www.anyhere.com/gward/papers/ewp98.pdf">The Holodeck: A Parallel
2107 >        Ray-caching Rendering System</a>,&quot; Proceedings of the Second
2108          Eurographics Workshop on Parallel Graphics and Visualisation,
2109          September 1998.
2110      <li>Larson, G.W. and R.A. Shakespeare,
# Line 1845 | Line 2112 | Ecole  Polytechnique  Federale de Lausanne (EPFL Unive
2112          the Art and Science of Lighting Visualization</em></a>,
2113          Morgan Kaufmann Publishers, 1998.
2114      <li>Larson, G.W., H. Rushmeier, C. Piatko,
2115 <        ``<a HREF="http://radsite.lbl.gov/radiance/papers/lbnl39882/tonemap.pdf">A Visibility
2115 >        &quot;<a HREF="http://radsite.lbl.gov/radiance/papers/lbnl39882/tonemap.pdf">A Visibility
2116          Matching Tone Reproduction Operator for
2117 <        High Dynamic Range Scenes</a>,'' LBNL Technical Report 39882,
2117 >        High Dynamic Range Scenes</a>,&quot; LBNL Technical Report 39882,
2118          January 1997.
2119 <    <li>Ward, G., ``<a HREF="http://radsite.lbl.gov/radiance/papers/erw95.1/paper.html">Making
2120 <        Global Illumination User-Friendly</a>,'' Sixth
2119 >    <li>Ward, G., &quot;<a HREF="http://radsite.lbl.gov/radiance/papers/erw95.1/paper.html">Making
2120 >        Global Illumination User-Friendly</a>,&quot; Sixth
2121          Eurographics Workshop on Rendering, Springer-Verlag,
2122          Dublin, Ireland, June 1995.</li>
2123      <li>Rushmeier, H., G. Ward, C. Piatko, P. Sanders, B. Rust,
2124 <        ``<a HREF="http://radsite.lbl.gov/mgf/compare.html">
2124 >        &quot;<a HREF="http://radsite.lbl.gov/mgf/compare.html">
2125          Comparing Real and Synthetic Images: Some Ideas about
2126 <        Metrics</a>,'' Sixth Eurographics Workshop on Rendering,
2126 >        Metrics</a>,&quot; Sixth Eurographics Workshop on Rendering,
2127          Springer-Verlag, Dublin, Ireland, June 1995.</li>
2128 <    <li>Ward, G., ``<a HREF="http://radsite.lbl.gov/radiance/papers/sg94.1/paper.html">The RADIANCE
2129 <        Lighting Simulation and Rendering System</a>,'' <em>Computer
2128 >    <li>Ward, G., &quot;<a HREF="http://radsite.lbl.gov/radiance/papers/sg94.1/paper.html">The RADIANCE
2129 >        Lighting Simulation and Rendering System</a>,&quot; <em>Computer
2130          Graphics</em>, July 1994.</li>
2131 <    <li>Rushmeier, H., G. Ward, ``<a HREF="http://radsite.lbl.gov/radiance/papers/sg94.2/energy.html">Energy
2132 <        Preserving Non-Linear Filters</a>,'' <em>Computer
2131 >    <li>Rushmeier, H., G. Ward, &quot;<a HREF="http://radsite.lbl.gov/radiance/papers/sg94.2/energy.html">Energy
2132 >        Preserving Non-Linear Filters</a>,&quot; <em>Computer
2133          Graphics</em>, July 1994.</li>
2134 <    <li>Ward, G., ``A Contrast-Based Scalefactor for Luminance
2135 <        Display,'' <em>Graphics Gems IV</em>, Edited by Paul Heckbert,
2134 >    <li>Ward, G., &quot;A Contrast-Based Scalefactor for Luminance
2135 >        Display,&quot; <em>Graphics Gems IV</em>, Edited by Paul Heckbert,
2136          Academic Press 1994.</li>
2137 <    <li>Ward, G., ``<a HREF="http://radsite.lbl.gov/radiance/papers/sg92/paper.html">Measuring and
2138 <        Modeling Anisotropic Reflection</a>,'' <em>Computer
2137 >    <li>Ward, G., &quot;<a HREF="http://radsite.lbl.gov/radiance/papers/sg92/paper.html">Measuring and
2138 >        Modeling Anisotropic Reflection</a>,&quot; <em>Computer
2139          Graphics</em>, Vol. 26, No. 2, July 1992. </li>
2140 <    <li>Ward, G., P. Heckbert, ``<a HREF="http://radsite.lbl.gov/radiance/papers/erw92/paper.html">Irradiance
2141 <        Gradients</a>,'' Third Annual Eurographics Workshop on
2140 >    <li>Ward, G., P. Heckbert, &quot;<a HREF="http://radsite.lbl.gov/radiance/papers/erw92/paper.html">Irradiance
2141 >        Gradients</a>,&quot; Third Annual Eurographics Workshop on
2142          Rendering, Springer-Verlag, May 1992. </li>
2143 <    <li>Ward, G., ``<a HREF="http://radsite.lbl.gov/radiance/papers/erw91/erw91.html">Adaptive Shadow
2144 <        Testing for Ray Tracing</a>'' Photorealistic Rendering in
2143 >    <li>Ward, G., &quot;<a HREF="http://radsite.lbl.gov/radiance/papers/erw91/erw91.html">Adaptive Shadow
2144 >        Testing for Ray Tracing</a>&quot; Photorealistic Rendering in
2145          Computer Graphics, proceedings of 1991 Eurographics
2146          Rendering Workshop, edited by P. Brunet and F.W. Jansen,
2147          Springer-Verlag. </li>
2148 <    <li>Ward, G., ``Visualization,'' <em>Lighting Design and
2148 >    <li>Ward, G., &quot;Visualization,&quot; <em>Lighting Design and
2149          Application</em>, Vol. 20, No. 6, June 1990. </li>
2150 <    <li>Ward, G., F. Rubinstein, R. Clear, ``<a HREF="http://radsite.lbl.gov/radiance/papers/sg88/paper.html">A Ray Tracing Solution for
2151 <        Diffuse Interreflection</a>,'' <em>Computer Graphics</em>,
2150 >    <li>Ward, G., F. Rubinstein, R. Clear, &quot;<a HREF="http://radsite.lbl.gov/radiance/papers/sg88/paper.html">A Ray Tracing Solution for
2151 >        Diffuse Interreflection</a>,&quot; <em>Computer Graphics</em>,
2152          Vol. 22, No. 4, August 1988. </li>
2153 <    <li>Ward, G., F. Rubinstein, ``A New Technique for Computer
2154 <        Simulation of Illuminated Spaces,'' <em>Journal of the
2153 >    <li>Ward, G., F. Rubinstein, &quot;A New Technique for Computer
2154 >        Simulation of Illuminated Spaces,&quot; <em>Journal of the
2155          Illuminating Engineering Society</em>, Vol. 17, No. 1,
2156          Winter 1988. </li>
2157   </ul>
# Line 1922 | Line 2189 | SURFACES       MATERIALS       TEXTURES        PATTERNS        MIXTURES</h4>
2189                  <a HREF="#Plasdata">Plasdata</a>
2190                  <a HREF="#Metdata">Metdata</a>
2191                  <a HREF="#Transdata">Transdata</a>
2192 +                <a HREF="#BSDF">BSDF</a>
2193                  <a HREF="#Antimatter">Antimatter</a>
2194                                  
2195   </pre>

Diff Legend

– Removed lines
+ Added lines
< Changed lines
> Changed lines