Simplex noise

Simplex noise is a method for constructing an n-dimensional noise function comparable to Perlin noise ("classic" noise) but with fewer directional artifacts and, in higher dimensions, a lower computational overhead. Ken Perlin designed the algorithm in 2001^[1] to address the limitations of his classic noise function, especially in higher dimensions.

The advantages of simplex noise over Perlin noise:

Simplex noise has a lower computational complexity and requires fewer multiplications.
Simplex noise scales to higher dimensions (4D, 5D) with much less computational cost: the complexity is $O(n^{2})$ for $n$ dimensions instead of the $O(2^{n})$ of classic noise.^[2]
Simplex noise has no noticeable directional artifacts (is visually isotropic), though noise generated for different dimensions are visually distinct (e.g. 2D noise has a different look than slices of 3D noise, and it looks increasingly worse for higher dimensions).
Simplex noise has a well-defined and continuous gradient (almost) everywhere that can be computed quite cheaply.
Simplex noise is easy to implement in hardware.

Whereas classical noise interpolates between the gradients at the surrounding hypergrid end points (i.e., northeast, northwest, southeast and southwest in 2D), simplex noise divides the space into simplices (i.e., $n$ -dimensional triangles). This reduces the number of data points. While a hypercube in $n$ dimensions has $2^{n}$ corners, a simplex in $n$ dimensions has only $n+1$ corners. The triangles are equilateral in 2D, but in higher dimensions the simplices are only approximately regular. For example, the tiling in the 3D case of the function is an orientation of the tetragonal disphenoid honeycomb.

Simplex noise is useful for computer graphics applications, where noise is usually computed over 2, 3, 4 or possibly 5 dimensions. For higher dimensions, n-spheres around n-simplex corners are not densely enough packed, reducing the support of the function and making it zero in large portions of space.

Algorithm detail

Simplex noise is most commonly implemented as a two-, three-, or four-dimensional function, but can be defined for any number of dimensions. An implementation typically involves four steps: coordinate skewing, simplical subdivision, gradient selection, and kernel summation.

Coordinate skewing

An input coordinate is transformed using the formula

x'=x+(x+y+...)*F

y'=y+(x+y+...)*F

...

where

F={\frac {{\sqrt {n+1}}-1}{n}}

This has the effect of placing the coordinate on an A*
n lattice, which is essentially the vertex arrangement of a hypercubic honeycomb that has been squashed along its main diagonal until the distance between the points (0, 0, ..., 0) and (1, 1, ..., 1) becomes equal to the distance between the points (0, 0, ..., 0) and (1, 0, ..., 0).

The resulting coordinate (x', y', ...) is then used in order to determine which skewed unit hypercube cell the input point lies in, (xb'=floor(x'), yb'=floor(y'), ...), and its internal coordinates (xi'=x'-xb', yi'=y'-yb', ...).

Simplical subdivision

Once the above is determined, the values of the internal coordinate (xi', yi', ...) are sorted in decreasing order, to determine which skewed Schläfli orthoscheme simplex the point lies in. Then the resulting simplex is composed of the vertices corresponding to an ordered edge traversal from (0, 0, ..., 0) to (1, 1, ..., 1), of which there are n! possibilities each of which correspond to a single permutation of the coordinate. In other words, start with the zero coordinate, and successively add ones starting in the value corresponding to the largest internal coordinate's value, and ending with the smallest.

For example, the point (0.4, 0.5, 0.3) would lie inside the simplex with vertices (0, 0, 0), (0, 1, 0), (1, 1, 0), (1, 1, 1). The yi' coordinate is the largest so it is added first. It is then followed by the xi' coordinate, and finally zi'.

Gradient selection

Each simplex vertex is added back to the skewed hypercube's base coordinate, and hashed into a pseudo-random gradient direction. The hash can be implemented in numerous ways, though most often uses a permutation table or a bit manipulation scheme.

Care should be taken in the selection of the set of gradients to include, in order to keep directional artifacts to a minimum.

Kernel summation

The contribution from each of the n+1 vertices of the simplex is factored in via a summation of radially-symmetric kernels centered around each vertex. First, the unskewed coordinate of each of the vertices is determined using the inverse formula

x=x'+(x'+y'+...)*G

y=y'+(x'+y'+...)*G

...

where

G={\frac {1-1/{\sqrt {n+1}}}{n}}

This point is subtracted from the input coordinate in order to obtain the unskewed displacement vector. This unskewed displacement vector is used for two purposes:

To compute the extrapolated gradient value using a dot product
To determine d², the squared distance to the point.

From there, each vertex's summed kernel contribution is determined using the equation

(max(0,r^{2}-d^{2}))^{4}*(<\Delta x,\Delta y,...>\cdot <grad.x,grad.y,...>)

where r² is usually set to either 0.5 or 0.6. 0.5 ensures no discontinuities, whereas 0.6 may increase visual quality in applications for which the discontinuities are not noticeable. 0.6 was used in Ken Perlin's original reference implementation.

Legal status

Uses of implementations in 3D and higher for textured image synthesis are covered by U.S. Patent 6,867,776, if the algorithm is implemented using the specific techniques described in any of the patent claims.

References

↑ Ken Perlin, Noise hardware. In Real-Time Shading SIGGRAPH Course Notes (2001), Olano M., (Ed.). (pdf)
↑ Ken Perlin, Making noise. Based on a talk presented at GDCHardcore (Dec 9, 1999). (url)

External links

Procedural Coherent noise

Approach

Lattice based

Gradient noise	Simplex noise OpenSimplex noise Perlin noise Wavelet noise

Value noise	Value noise

Point based

Worley noise (Voronoi/Cellular noise)

Applications

Noise (physics and telecommunications)

General	Acoustic quieting Distortion Noise cancellation Noise control Noise measurement Noise power Noise reduction Noise temperature Phase distortion

Noise in...	Audio Buildings Electronics Environment Government regulation Human health Images Radio Rooms Ships Sound masking Transportation Video

Class of noise	Additive white Gaussian noise (AWGN) Atmospheric noise Background noise Brownian noise Burst noise Cosmic noise Flicker noise Gaussian noise Grey noise Jitter Johnson–Nyquist noise (thermal noise) Pink noise Quantization error (or q. noise) Shot noise White noise Coherent noise Value noise Gradient noise Worley noise

Engineering terms	Channel noise level Circuit noise level Effective input noise temperature Equivalent noise resistance Equivalent pulse code modulation noise Impulse noise (audio) Noise figure Noise floor Noise shaping Noise spectral density Noise, vibration, and harshness (NVH) Phase noise Pseudorandom noise Statistical noise

Ratios	Carrier-to-noise ratio (C/N) Carrier-to-receiver noise density (C/kT) dBrnC E_b/N₀ (energy per bit to noise density) E_s/N₀ (energy per symbol to noise density) Modulation error ratio (MER) Signal, noise and distortion (SINAD) Signal-to-interference ratio (S/I) Signal-to-noise ratio (S/N, SNR) Signal-to-noise ratio (imaging) Signal to noise plus interference (SNIR) Signal-to-quantization-noise ratio (SQNR)

Related topics	List of noise topics Acoustics Colors of noise Interference (communication) Noise generator Radio noise source Spectrum analyzer Thermal radiation

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