Documentation:Tutorial Section 3.2

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Isosurface Object

Simple functions

Let's begin with something simple. In this first series of images, let's explore the user defined function shown as function { x } that we see in the code example below. It produces the first image on the left, a simple box. The container, which is a requirement for the isosurface object, is represented by the box object and the contained_by keyword in the isosurface definition.

  isosurface {
    function { x }
    contained_by { box { -2, 2 } }
  }

You should have also noticed that in the image on the left, only half the box was produced, that's because the threshold keyword was omitted, so the default value 0 was used to evaluate the x-coordinate.

In this next code example threshold 1 was added to produce the center image.

  isosurface {
    function { x }
    threshold 1
    contained_by { box { -2, 2 } }
  }

It is also possible to remove the visible surfaces of the container by adding the open keyword to the isosurface definition.

For the final image on the right, the following code example was used. Notice that the omission of the threshold keyword causes the x-coordinate to be again evaluated to zero.

  isosurface {
    function { x }
    open
    contained_by { box { -2, 2 } }
  }

function { x }	function { x } with threshold 1	function { x } with open

Hint: The checkered ground plane is scaled to one unit squares.

For the last series of images in this section, let's try something different. These next two code examples were used to show the results of changing the user defined function to function { x+y } and function { x+y+z } respectively. They describe planes going through the origin, the function just describes the normal vector of the plane.

  isosurface {
    function { x+y }
    max_gradient 4
    contained_by { box { -2, 2 } }
  }

Note: To properly render these examples max_gradient 4 was added to the isosurface definition, and will be explained later.

  isosurface {
    function { x+y+z }
    max_gradient 4
    contained_by { box { -2, 2 } }
  }

plane function { x+y }	plane function { x+y+z }

Note: When appropriate, to better visualize the difference between the isosurface and the container object, the images in this tutorial have been color coded.

Several surfaces

Now that you're starting to become familiar with isosurface syntax, there really isn't any need to show a code example for each and every image. You can always look back at the earlier examples when needed. The image captions will most often contain additional keyword hints when appropriate.

Note: The user defined function portion will always use this color coded format: function { x+y+z }

For the first image on the left, these two functions lead to identical results: function { abs(x)-1 } and function { sqrt(x*x)-1 } because both of these formulas have the same solution where the function value is 0, specifically x=-1 and x=1 in this example.

You can easily mix any of these elements in different combinations, but the results always produce planar surfaces. The last two images in this series used function { abs(x)-1+y } and function { abs(x)+abs(y)+abs(z)-2 } respectively.

identical results with open	linear functions x & y axis	linear functions x, y & z axis

Non-linear functions

	Curved surfaces of many different kinds can be achieved with non-linear functions. A square function creates the parabolic shape: function { pow(x,2)+y }
a parabolic shape

If you describe a circle in 2 dimensions with a constant in the 3rd dimension you get a cylinder: function { sqrt(pow(x,2)+pow(z,2))-1 }
	the cylinder shape

	It's easy to change a cylinder into a cone, we just need to add a linear component in y-direction: function { sqrt(pow(x,2)+pow(z,2))+y }
the cone shape

No worries, creating a sphere is easy too. In this example 2 specifies the radius: function { sqrt(pow(x,2)+pow(y,2)+pow(z,2))-2 }
	the sphere shape

Specifying functions

Until now, we have seen, the functions used to define the isosurface were literally written in the function {...} block:

#declare Threshold = 1;

isosurface {
function {pow(x,2) + pow(y,2) + pow(z,2)}
  threshold Threshold
  ...
}

Let's expand on that concept, and add some flexibility. Remember that user defined functions (like equations), all float expressions and operators which are legal in POV-Ray can be used, and that functions should be declared first, and then used in the isosurface. See the section User-Defined Functions for more information.

This next example takes the above equation, and rewrites it as a user defined function. By default a function that takes three parameters (x,y,z) does not require you to explicitly specify the parameter names when declaring it, however when using the identifier, the parameters must be specified.

#declare Threshold = 1;

#declare Sphere = function {pow(x,2) + pow(y,2) + pow(z,2)};

isosurface {
  function { Sphere(x,y,z) }
  threshold Threshold
  ...
}

However, if you need more or less than three parameters when declaring a function, you will also have to explicitly specify the parameter names.

#declare Sphere = function (x,y,z,Radius) {pow(x,2) + pow(y,2) + pow(z,2) - pow(Radius,2)};

isosurface {
  function { Sphere(x,y,z,1) }
  ...
}

Internal functions

There are a lot of internal functions available in POV-Ray. For example a sphere could also be generated with function { f_sphere(x, y, z, 2) }, for these and other functions, see the functions.inc include file. Most of them are more complicated and it is usually faster to use them instead of a hand coded equivalent.

See the complete list for details.

The following makes a torus just like POV-Ray's torus object:

  #include "functions.inc"

  isosurface {
    function { f_torus(x, y, z, 1.6, 0.4) }
    contained_by { box { -2, 2 } }
  }

	The 4th and 5th parameters are the major and minor radius, just like the corresponding values in the torus{} object. The parameters x, y and z are required, because it is a declared function. You can also declare functions yourself like it is explained in the reference section.
the torus function

Combining isosurface functions

We can also simulate some Constructive Solid Geometry with isosurface functions. If you do not know about CSG we suggest you have a look at What is CSG? or the corresponding part of the reference section first.

For this next group of images, consider the two functions for a cylinder and a rotated box:

  #declare fn_A = function { sqrt(pow(y,2) + pow(z,2)) - 0.8 }
  #declare fn_B = function { abs(x)+abs(y)-1 }

1. If we combine them the following way, we get a merge:
   function { min(fn_A(x, y, z), fn_B(x, y, z)) }
2. An intersection can be obtained by using max() instead of min():
   function { max(fn_A(x, y, z), fn_B(x, y, z)) }
3. A difference is possible, by adding a minus (-) before the second function:
   function { max(fn_A(x, y, z), -fn_B(x, y, z)) }

merge example	intersection example	difference example

Apart from basic CSG you can also obtain smooth transits between the different surfaces, for instance the blob object:

  #declare Blob_Threshold=0.01;

  isosurface {
    function {
      (1+Blob_Threshold)
      -pow(Blob_Threshold, fn_A(x,y,z))
      -pow(Blob_Threshold, fn_B(x,y,z))
    }
    max_gradient 4
    contained_by { box { -2, 2 } }
  }

	The Blob_Threshold value influences the smoothness of the transit between the shapes. A lower value leads to sharper edges, and it's function looks like: function{fn_A(x,y,z) + pow(Blob_threshold,(Fn_B(x,y,z) + Strength))}
smooth transitions using blob

Noise and pigment functions

Some of the internal functions have a random or noise-like structure

Together with the pigment functions they are one of the most powerful tools for designing isosurfaces. We can add real surface displacement to the objects rather than only normal perturbation known from the normal statement.

The relevant internal functions are:

• f_noise3d(x,y,z)
  uses the noise generator specified in global_settings and generates structures like the bozo pattern.
• f_noise_generator(x, y, z, noise_generator)
  generates noise with a specified noise generator.
• f_ridged_mf(x, y, z, H, Lacunarity, Octaves, Offset, Gain, noise_generator)
  generates a ridged multifractal pattern.
• f_ridge(x, y, z, Lambda, Octaves, Omega, Offset, Ridge, noise_generator)
  generates another noise with ridges.
• f_hetero_mf(x, y, z, H, Lacunarity, Octaves, Offset, T, noise_generator)
  generates heterogenic multifractal noise.

Using this simple noise3d function results in the image on the right. The value -0.5 matches the default threshold value of zero. The f_noise3d function returns values between 0 and 1: function { f_noise3d(x,y,z)-0.5 }
	simple noise3d function

In these next two images the noise function was added to a plane function. The x-parameter was set to 0 so the noise function is constant in x-direction. This way we achieve the typical heightfield structure.

	With this and the other functions you can generate objects similar to heightfields, having the advantage that a high resolution can be achieved without high memory requirements: function { x + f_noise3d(0,y,z) }
a noise3d heightfield

The noise function can of course also be subtracted which results in an inverted version: function { x - f_noise3d(0,y,z) }
	a noise3d heightfield - inverted

	Of course we can also add noise to any other function. If the noise function is very strong this can result in several separated surfaces. function { f_sphere(x,y,z,1.2) - f_noise3d(x,y,z) }
noise3d on a sphere

This is a noise function applied to a sphere surface, we can influence the intensity of the noise by multiplying it with a factor and change the scale by multiplying the coordinate parameters: function {   f_sphere(x,y,z,1.6) -     f_noise3d(x*5,y*5,z* ) * 0.5     }
	noise3d on a sphere - scaled

As alternative to noise functions we can also use any pigment in a function:

  #declare fn_Pigm=function {
    pigment {
      agate
      color_map {
        [0 color rgb 0]
        [1 color rgb 1]
      }
    }
  }

This is a vector function, it returns a color vector for use in isosurface functions. They must be pre-declared first. When using the identifier, you have to specify which component of the color vector should be used.

To do this, the dot notation is used. Refer to the above example: fn_Pigm(x,y,z).red

A color vector has five components, their supported dot types to access these components are:

1. fn_Pigm( ).x | fn_Pigm( ).u | fn_Pigm( ).red
   to get the red value of the color vector
2. fn_Pigm( ).y | fn_Pigm( ).v | fn_Pigm( ).green
   to get the green value of the color vector
3. fn_Pigm( ).z | fn_Pigm( ).blue
   to get the blue value of the color vector
4. fn_Pigm( ).filter | fn_Pigm( ).f
   to get the filter value of the color vector
5. fn_Pigm( ).transmit | fn_Pigm( ).t
   to get the transmit value of the color vector

And two special purpose operators, their supported dot types to access these operators are:

Note: The .hf operator is experimental and will generate a warning.

1. fn_Pigm( ).gray to get the gray value of the color vector
   gray value = Red*29.7% + Green*58.9% + Blue*11.4%
2. fn_Pigm( ).hf to get the height_field value of the color vector
   hf value = (Red + Green/255)*0.996093

	There are quite a lot of things possible with pigment functions. However, it should be noted that, some functions can cause longer render times: function {   f_sphere(x, y, z, 1.6) -     fn_Pigm(x/2, y/2, z/2).gray*0.5     }
noise using a pigment function

Conditional directives and loops

Conditional directives are allowed in functions:

#declare Rough = yes;
#include "functions.inc"
isosurface {
  function { y #if(Rough=1)-f_noise3d(x/0.5,y/0.3,z/0.4)*0.8 #end }
  ...
}

Loops can also be used in functions:

#include "functions.inc"
#declare Thr = 1/1000;
#declare Ang = radians(45);
#declare Offset = 1.5;
#declare Scale = 1.2;
#declare TrSph = function { f_sphere(x-Offset,y,z,0.7*Scale) }

function {
  (1-Thr)
  #declare A = 0;
  #while (A<8)
  -pow(Thr, TrSph(x*cos(A*Ang) + y*sin(A*Ang),
                  y*cos(A*Ang) -x*sin(A*Ang), z) )
    #declare A=A+1;
  #end
}

Note: The loops and conditionals are evaluated at parse time, not at render time.

Transformations on functions

Transforming an isosurface object is done like transforming any POV-Ray object. Simply use the object modifiers, scale, translate, and rotate. However, when you want to transform functions within the contained_by object, you have to substitute parameters in the functions.

The results seem inverted to what you would normally expect, here's why:

Remember the sphere function we created earlier in this tutorial: Sphere(x,y,z)

We know it sits at the origin because x=0. If we want to translate it 2 units to the right to x=2 we need to write the second equation in the same form: x-2=0. Now that both equations equal zero, we can replace the parameter x with x-2, call our function as: Sphere(x-2,y,z) and it's translated two units to the right.

Let's look at how to scale our test sphere by 0.5 in the y direction. Given the default value of y=1 one unit we'd want y=0.5. To do this we need to have the equation in the same form as the first one, so we'll multiply both sides by two: y*2 = 0.5*2 which gives y*2=1.

Now we can replace the y parameter in our sphere: Sphere(x,y*2,z). This scales the y-size of the sphere by half.

Here is an overview of some useful substitutions, we'll be using a pseudo-object designated as P(x,y,z) in the following examples:

Scale:

  To scale x replace x with x/scale:
  P(x/2,y,z)

Scale Infinitely:

  To scale y infinitely replace y with 0:
  P(x,0,z)

Translate:

  To translate z replace z with z - translation:
  P(x,y,z-3)

Shear:

  To shear in xy-plane replace x with x + y*tan(radians(Angle)):
  P(x+y*tan(radians(Angle)),y,z)

Rotate:

Note: These rotation substitutions work like normal POV-rotations, they already compensate for the inverse behavior.

To rotate around the X-axis:

  replace y with z*sin(radians(Angle)) + y*cos(radians(Angle))

  replace z with z*cos(radians(Angle)) - y*sin(radians(Angle))

To rotate around the Y-axis:

  replace x with x*cos(radians(Angle)) - z*sin(radians(Angle))

  replace z with x*sin(radians(Angle)) + z*cos(radians(Angle))

To rotate around the Z-axis:

  replace x with x*cos(radians(Angle)) + y*sin(radians(Angle))

  replace y with -x*sin(radians(Angle)) + y*cos(radians(Angle))

Flip:

To flip X - Y:

  replace x with y AND replace y with -x

To flip Y - Z:

  replace y with z AND replace z with -y

To flip X - Z:

  replace x with -z AND replace z with x

Twist:

To twist N turns/unit around the x axis:

    replace y with z*sin(x*2*pi*N) + y*cos(x*2*pi*N)

    replacez with z*cos(x*2*pi*N) - y*sin(x*2*pi*N)

Improving Isosurface Speed

To optimize the approximation of the isosurface and to get maximum rendering speed it is important to adapt certain values;

accuracy

The accuracy value influences how accurate the surface geometry is calculated. Lower values lead to a more precise, but slower result. The default value of 0.001 is fairly low. We used this value in all the previous samples, but often you can raise this quite a lot and thereby make things faster.

max_gradient

For finding the actual surface it is important for POV-Ray to know the maximum gradient of the function, meaning how fast the function value changes. We can specify a value with the max_gradient keyword. Lower max_gradient values lead to faster rendering, but if the specified value is below the actual maximum gradient of the function, there can be holes or other artefacts in the surface.

For the same reason functions with infinite gradient should not be used. This applies for pigment functions with brick or checker pattern for example. You should also be careful when using select() in isosurface functions because of this.

If the real maximum gradient differs too much from the specified value POV-Ray prints a warning together with the found maximum gradient. It is usually sufficient to use this number for the max_gradient parameter to get fast and correct results.

POV-Ray can also dynamically change the max_gradient when you specify evaluate with 3 parameters the isosurface definition. Concerning the details on this and other things see the evaluate in the reference section.

contained_by

Make sure your contained_by 'object' fits as tightly as possible. An oversized container can sky-rocket the render time.
When the container has a lot of empty space around the actual isosurface, POV-Ray has to do a lot of superfluous sampling: especially with complex functions this can become very time consuming. On top of this, the max_gradient needed to get a proper surface will also increase rapidly (almost proportional to the oversize!).
You could use a transparent copy of the container (using exactly the same transformations) to check how it fits. Getting the min_extent and max_extent of the isosurface is not useful because it only gives the extent of the container and not of the actual isosurface.

Poly Object

The polynomial object (and its shortcut versions: cubic, quartic and quadric) of POV-Ray is one of the most complex and mathematical primitives of the program. One could think that it is seldom used and more or less obsolete, but we have to remember that for example the torus primitive is just a shortcut for the equivalent quartic, which is just a shortcut for the equivalent poly object. Polys are, however, seldom used in scenes due to the fact that they are so difficult to define and it is far from trivial to get the desired shape with just a polynomial equation. It is mostly used by the most mathematically oriented POV-Ray users.

This tutorial explains the process of making a polynomial object in POV-Ray.

Note: Since version 3.5, POV-Ray includes the new isosurface object which makes the polynomial object more or less obsolete. The isosurface is more versatile (you can specify any mathematical function, not just polynomials) and easier to use. You can write the function as is, without needing to put values in a gigantic vector. Isosurfaces also often (although not always) render considerably faster than equivalent polys.

However, the most mathematically oriented still like polys because isosurfaces are calculated just by approximating the right value, while the poly is calculated in a mathematically exact way. Usually isosurfaces are more than good enough for most applications, though.

Note: A maximum of 35th degree polynomial can be represented with the poly object. If a higher degree polynomial or other non-polynomial function has to be represented, then it is necessary to use the isosurface object.

Creating the polynomial function

The first step is to create the polynomial function to be represented. You will need some (high-school level) mathematical knowledge for this.

1) Let's start with an easy example, a sphere:

The sphere function is:

sphere function

Now we have to convert this to polynomial form, we will need a polynomial of the 2nd degree to represent this:

sphere polynomial

2) A more elaborated example:

Let's take the function:

function

Converting this to polynomial form we get:

polynomial

Although the highest power is 4 we will need a 5th order polynomial to represent this function (because we cannot represent y⁴z with a 4th order polynomial).

3) And since we talked about the torus, let's also take it as an example.

A torus can be represented with the function:

torus function

where r₁ is the major radius and r₂ is the minor radius.

Now, this is tougher to convert to polynomial form, but finally we get:

torus polynomial

A 4th order polynomial is enough to represent this.

Note: Not every function can be represented in polynomial form. Only functions that use addition (and substraction), multiplication (and division) and scalar powers (including rational powers, eg. the square root) can be represented. Also, the poly primitive supports only polynomials of the 35th degree at max.

Converting a function to polynomial form may be a very laborious task for certain functions. Some mathematical programs are very helpful in this matter.

Writing the polynomial vector

Now that we have the function in polynomial form, we have to write it in POV-Ray syntax. The syntax is specified in the in the chapters Poly, Cubic and Quartic and Quadric of the reference section. There is also a table in this chapter which we will be using to make the polynomial vector. It is easier to have this table printed on paper.

Note: It is also possible to make a little program with your favorite programming language which will print the poly vector from the polynomial function, but making a program like this is up to you.

1) Let's start with the easy one, ie. the sphere.

Since the sphere can be represented with a polynomial of 2nd degree, we look at the column titled 2nd in the table. We see that it has 10 items, ie. we need a vector of size 10. Each item of the vector will be the factor of the term listed in the table.

The polynomial was:

sphere polynomial function

Writing the poly in this way we get:

#declare Radius=1;
poly
{ 2,
  <1,0,0,0,1,
   0,0,1,0,-Radius*Radius>
}

Put each group of factors (separated with lines in the table) in their own lines.

In the table we see that the first item is the factor for x², which is 1 in the function. The next item is xy. Since it is not in the function, its factor is 0. Likewise the next item, which is xz. And so on. The last item is the scalar term, which is in this case -r².

If we make a proper scene and render it, we get:

camera { location y*4-z*5 look_at 0 angle 35 }
light_source { <100,200,-50> 1 }
background { rgb <0,.25,.5> }

#declare Radius=1;
poly
{ 2,
  <1,0,0,0,1,
   0,0,1,0,-Radius*Radius>
  pigment { rgb <1,.7,.3> } finish { specular .5 }
}

sphere polynomial image

Note: There is a shortcut for 2nd degree polynomials: The quadric primitive. Using a shortcut version, whenever possible, can lead to faster renderings. We can write the sphere code described above in the following way:

quadric
{ <1,1,1>, <0,0,0>, <0,0,0>, -Radius*Radius
  pigment { rgb <1,.7,.3> } finish { specular .5 }
}

2) Now lets try the second one. We do it similarly, but this time we need to look at the column titled 5th in the table.

The polynomial was:

5th order polynomial function

Writing the poly primitive we get:

poly
{ 5,
  <0,0,0,0,0,
   0,0,0,0,0,
   0,0,0,0,0,
   0,0,0,1,0,
   0,0,0,0,0,
   -2,0,0,0,0,
   0,0,0,0,0,
   0,1,0,0,0,
   0,0,0,0,0,
   0,0,0,0,0,
   0,0,0,0,0,0>
}

With the proper scene we get:

camera { location <8,20,-10>*.7 look_at x*.01 angle 35 }
light_source { <100,200,20> 1 }
background { rgb <0,.25,.5> }

poly
{ 5,
  <0,0,0,0,0,
   0,0,0,0,0,
   0,0,0,0,0,
   0,0,0,1,0,
   0,0,0,0,0,
   -2,0,0,0,0,
   0,0,0,0,0,
   0,1,0,0,0,
   0,0,0,0,0,
   0,0,0,0,0,
   0,0,0,0,0,0>
  clipped_by { box { <-4,-4,-1><4,4,1> } }
  bounded_by { clipped_by }
  pigment { rgb <1,.7,.3> } finish { specular .5 }
  rotate <0,90,-90>
}

5th order polynomial image

3) And finally the torus:

The polynomial was:

torus polynomial function

And we get the proper 4th degree poly primitive:

camera { location y*4-z*5 look_at 0 angle 35 }
light_source { <100,200,-50> 1 }
background { rgb <0,.25,.5> }

#declare r1=1;
#declare r2=.5;
poly
{ 4,
  <1,0,0,0,2,
   0,0,2,0,-2*(r1*r1+r2*r2),
   0,0,0,0,0,
   0,0,0,0,0,
   1,0,0,2,0,
   2*(r1*r1-r2*r2),0,0,0,0,
   1,0,-2*(r1*r1+r2*r2),0,pow(r1,4)+pow(r2,4)-2*r1*r1*r2*r2>
  pigment { rgb <1,.7,.3> } finish { specular .5 }
}

When rendered we get:

torus polynomial image

There is a shortcut for 4th order polynomials: The quartic primitive. We can write the torus like this:

quartic
{ <1,0,0,0,2,
   0,0,2,0,-2*(r1*r1+r2*r2),
   0,0,0,0,0,
   0,0,0,0,0,
   1,0,0,2,0,
   2*(r1*r1-r2*r2),0,0,0,0,
   1,0,-2*(r1*r1+r2*r2),0,pow(r1,4)+pow(r2,4)-2*r1*r1*r2*r2>
  pigment { rgb <1,.7,.3> } finish { specular .5 }
}

Polynomial made easy

Since consulting the table in the section Poly, Cubic and Quartic or writing a program to get the right poly vector can be a bit cumbersome, especially when the poly vector is not a write-once-only expression and that you want to get it back, so let's examine how those equations would be rewritten using the simplified syntax.

You should refer to the images in the previous section, as these examples produce exactly the same results.

1) The sphere example can be rewritten as:

#declare Radius=1;
polynomial { 2, 
  xyz(2,0,0):1, 
  xyz(0,2,0):1,
  xyz(0,0,2):1,
  xyz(0,0,0):-Radius*Radius 
}

2) Let's now see the second one:

polynomial { 5,
  xyz(2,0,1):1,
  xyz(0,4,1):1,
  xyz(1,2,0):-2
}

3) And finally the torus example:

polynomial { 4,
  xyz(4,0,0):1,
  xyz(2,2,0):2,
  xyz(2,0,2):2,
  xyz(2,0,0):-2*(r1*r1+r2*r2),
  xyz(0,4,0):1,
  xyz(0,2,2):2,
  xyz(0,2,0):2*(r1*r1-r2*r2),
  xyz(0,0,4):1,
  xyz(0,0,2):-2*(r1*r1+r2*r2),
  xyz(0,0,0):pow((r1*r1-r2*r2),2)
}

Isosurface Object

Superquadric Ellipsoid Object

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