Natural image statistics for
Erik Reinhard, Peter Shirley and Tom
School of Computing
University of Utah
Salt Lake City, UT 84112 USA
March 26, 2001
The class of all natural images is an inﬁnitely small fraction of all possible images. The
structure of natural images can be statistically modeled, revealing striking regularities. The
human visual system appears to be optimized to view natural images, as opposed to any
possible image, and therefore expects to interpret images which conform to these statistics.
Research has shown that images that do not statistically behave as natural images are harder
for the human visual system to interpret. This paper reviews the statistics of natural images
and the implications for computer graphics in general are assessed. We argue that these
statistics are important for graphics applications and ﬁnally, we provide a direct application
of these ﬁndings to random subdivision terrain modeling.
Natural image statistics for computer graphics
The class of all natural images is an inﬁnitely small fraction of all
possible images. The structure of natural images can be statisti-
cally modeled, revealing striking regularities. The human visual
system appears to be optimized to view natural images, as opposed
to any possible image, and therefore expects to interpret images
which conform to these statistics. Research has shown that images
that do not statistically behave as natural images are harder for the
human visual system to interpret. This paper reviews the statis-
tics of natural images and the implications for computer graphics in
general are assessed. We argue that these statistics are important for
graphics applications and ﬁnally, we provide a direct application of
these ﬁndings to random subdivision terrain modeling.
CR Categories: G.3 [Mathematics of Computing]: Probabil-
ity and Statistics; I.3.7 [Computing Methodologies]: Computer
Graphics—3D Graphics; I.4.10 [Computing Methodologies]: Im-
age Processing and Computer Vision—Image Representation
Keywords: Natural image statistics, Visual perception, Power
spectra, Fractal terrains
The set of all 1000 by 1000 pixel images occupies a million di-
mensional space. The set of natural images, which are those that
appear in our world, form a sparse subset of all possible images
that can be identiﬁed using statistical approaches. The statistics of
natural images have been studied to understand how their properties
inﬂuence the human visual system (HVS). To assess invariances in
natural images, a large set of calibrated images are collected into an
ensemble and statistics are computed on these ensembles. The en-
semble should be chosen such that it is representative for all natural
images. This cannot generally be achieved with a single image.
Natural image statistics can be characterized by their order.
In particular, ﬁrst, second and higher order statistics are distin-
First order statistics treat each pixel independently, so that for ex-
ample the distribution of intensities encountered in natural im-
ages can be estimated.
University of Utah
University of Utah
University of Sussex
Second order statistics measure the dependencies between pairs
of pixels, which are usually expressed in terms of the power
spectrum (see section 2).
Higher order statistics are used to extract properties of natural
scenes which can not be modeled using ﬁrst and second or-
der statistics. These properties include lines and edges.
First order statistics capture little structure that aids in understand-
ing the HVS, nor does it distinguish natural images from arbitrary
images very well. We therefore choose to largely ignore ﬁrst order
In this paper we review current knowledge of image statistics,
and argue that this knowledge is likely to be useful for some com-
puter graphics applications. We ﬁrst review the basics of image
statistics (Section 2). We thendiscuss the mechanics of power spec-
tra computation and how to analyze their structure (Section 3), This
is followed by experiments on image ensembles (Section 4). Next,
we provide evidence that second order statistics are sensitive to ge-
ometric variations rather than differences between lighting simu-
lations (Sections 5 and 6). The results are then applied to fractal
terrain modeling (Section 7), followed by conclusions (Section 8).
2 Background: second order statistics
The most remarkable and salient natural image statistic that has
been discovered so far is that the slope of the power spectrum tends
to be close to 2. The power spectrum of an M by M image is
|F (u, v)|
where F is the Fourier transform of the image. By represent-
ing the two-dimensional frequencies u and v in polar coordinates
(u = f cos φ and v = f sin φ) and averaging over all directions φ
and all images in the ensemble, it is found that on log-log scale am-
plitude as function of frequency f lies approximately on a straight
line [7, 11,31–33]. This means that spectral power as function of
spatial frequency behavesaccording to a power law function. More-
over, ﬁtting a line through the data points yields a slope α of ap-
proximately 2 for natural images:
Here, A is a constant determining the overall image contrast, α is
the spectral slopeand η isits deviation from 2. This result is true for
ensembles, but may not hold for the lowest few frequencies when
applied to individual images [3,20].
Although this spectral slope varies subtly between different stud-
ies [7, 10,12,32,40], it appears to be extremely robust against dis-
tortions and transformations and it is therefore concluded that this
spectral behavior is a consequence of the images themselves, rather
than of particular methods of camera calibration or exact computa-
tion of the spectral slope.
However, the precise value of the spectral slope depends some-
what on the type of scenes that make up the ensemble. Most studies
in this ﬁeld use images of natural objects such as trees and shrubs
because it is argued that the HVS evolved when only natural objects
were present. Some studies show that the spectral slope for scenes
containing man-made objects is slightly different . Even if no
manufactured objects are present, the statistics vary dependent on
what is predominantly in the images. The second order statistics
for sky are for example very different from those of trees.
One way in which this becomes apparent is when the power spec-
tra are not circularly averaged, but when the log average power is
plotted against angle. For natural image ensembles all angles show
more or less straight power spectra, although most of the power
is concentrated in horizontal and vertical angles [31,33] (see also
Figure 5). The horizon and the presence of tree-trunks are said to
be factors in this, although this behavior is also likely to occur in
The power spectrum is related to the auto-correlation function
through the Wiener-Khintchine theorem, which states that the auto-
correlation function and the power spectrum form a Fourier trans-
form pair . Hence, power spectral behavior can be equiva-
lently understood in terms of correlations between pairs of pixel-
A related image statistic is contrast, normally deﬁned as the stan-
dard deviation of all pixel intensities divided by the mean intensity
(σ/µ). This measure can either be computed directly from the im-
age data, or through Parceval’s theorem it can be derived from the
power spectrum :
S(u, v). (3)
This particular contrast computation can be modiﬁed to compute
contrast in different frequency bands. Frequency-conscious vari-
ance can then be thresholded, yielding a measure which can detect
blur . This is useful as lack of contrast can also be caused by
the absence of sufﬁcient detail in a sharp image.
The above second order statistics are usually collected for lumi-
nance images only, as luminance is believed to carry the greatest
amount of information. However, chrominance channels are shown
to exhibit similar spectral behavior , and therefore all subse-
quent qualitativearguments are expectedto be true for color as well.
The fact that the spectral behavior of natural images yields a straight
line with a slope of around 2 is important. Recent unrelated stud-
ies have found that in image interpretation tasks, the HVS performs
best when the images conform to this second order statistic. In one
such study, images of acar and a bull were morphed into each other,
with varying distances between the images in the sequence .
Different sequences were generated with modiﬁed spectral slopes.
The minimum distance where participants could still distinguish
consecutive images in each morph sequence was measured. This
distance was found to be smallest when the spectral slope of the
images in the morph sequence was close to 2. Deviation of the
spectral slope in either direction reduced the ability to distinguish
between morphed images.
In a different study the effect of spectral slope on the detection
of mirror symmetry in images was assessed . Here, white noise
patterns with varying degrees of vertical symmetry were created
and subsequently ﬁltered to alter the spectral slope. This experi-
ment, in which participants had to detect if symmetry was present,
revealed that performance was optimal for images with a spectral
slope of 2.
These studies conﬁrm the hypothesis that the HVS is tuned
to natural images. This is consistent with psychophysical mea-
surements, which indicate that the HVS expects to see images
with a 1/f
power spectrum and subsequently whitens them non-
adaptively . Whitening, or ﬂattening the power spectrum, results
in a spectral slope of α =0, which can be obtained by letting
S(f). Hence, it makes sense for computer graphics
applications to anticipate this type of visual processing and ensure
that images have 1/f
power spectra. Investigation of second order
image statistics is therefore the main goal of this paper.
2.2 Higher order statistics
One of the disadvantages of using amplitude information in the fre-
quency domain is that phase information is completely discarded,
thus ignoring the position of edges and objects. For this reason
higher order statistics have been applied to natural image ensem-
bles. The simplestglobal nth-order statistics that may capture phase
structure are the third and fourth moments, commonly referred to
as skew and kurtosis. They are computed as :
These dimensionless measures are by deﬁnition zero for pure Gaus-
sian distributions. Skew can be interpreted as an indicator for the
difference between the mean and the median of a dataset. Kurtosis
is based on the size of a distribution’s tails relative to Gaussian. A
positive value, associated with long tails in the distribution of inten-
sities, is usually associated with natural image ensembles. This is
for example evident when plotting log-contrast histograms, which
plot the probability of a particular contrast value appearing. These
plots are typically non-Gaussian with positive kurtosis .
Thomson  pointed out that for kurtosis to be meaningful
for natural image analysis, the data should be decorrelated, or
whitened, prior to any computation of higher order statistics. This
can be accomplished by ﬂattening the power spectrum, which en-
sures that second order statistics do not also capture higher order
statistics. Thus, skew and kurtosis become measures of variations
in the phase spectra. Regularities are found when these measures
are applied to the pixel histogram of an image ensemble [38,39].
This appears to indicate that the HVS may exploit higher order
phase structure after whitening the image. Understanding the phase
structure is therefore an important avenue of research in the ﬁeld of
natural image statistics.
2.3 Response properties of cortical cells
One of the reasons to study the statistics of natural images is to un-
derstand how the HVS codes these images. Because natural images
are not completely random, there is a signiﬁcant amount of redun-
dancy. The HVS may represent such scenes using a sparse set of
active elements. These elements will then be largely independent.
In this section it is assumed that an image can be represented as a
linear superposition of basis functions. Efﬁciently encoding images
now involves ﬁnding a set of basis functions that spans image space
and ensures that the coefﬁcients across an image ensemble are sta-
tistically as independent as possible . The resulting basis func-
tions (or ﬁlters) can then be compared to the response properties of
cortical cells in order to explain the early stages of human visual
processing. This has resulted in a number of different representa-
tions for basis functions, including Principal Components Analysis
(PCA) [2,15], Independent Components Analysis (ICA) [4,5, 22],
Gabor basis functions [11,12] and wavelets [12,18,23].
The PCA algorithm ﬁnds a set of basis functions which maxi-
mally decorrelates pairs of coefﬁcients, which is achieved by com-
puting the eigenvalues of the covariance matrix (between pairs of
pixel intensities). The corresponding eigenvectors represent a set
of orthogonal coefﬁcients, whereby the eigenvector with the largest
associated eigenvalue accounts for the greatest part of the covari-
ance. By using only the ﬁrst few coefﬁcients, it is possible to en-
code an image with a large reduction in free parameters . If
the image statistics are the same in all regions of an image, i.e. if
stationarity is assumed, then PCA produces coefﬁcients which are
similar to the Fourier transform . Indeed, PCA is strictly a sec-
ond order method assuming Gaussian signals.
Unfortunately, decorrelation does not guarantee independence.
Also, intensities in natural images are do not have a Gaussian dis-
tribution, and therefore PCA yields basis functions which do not
capture higher order structure very well . In particular, the ba-
sis functions tend to be orientationally and frequency sensitive, but
have global extent. This is in contrast to cells in the human primary
cortex which are spatially localized (as well as being localized in
frequency and orientation).
In contrast to PCA, ICA constitutes a transformation resulting in
basis functions which are non-orthogonal, localized in space, fre-
quency and orientation and aims to extract higher order information
from images [4,5]. ICA ﬁnds basis functions which are as indepen-
dent as possible . To avoid second order statistics to inﬂuence
the result of ICA, the data is usually ﬁrst decorrelated (also called
whitened), for example using a PCA algorithm. Filters can then
be found that produce extrema of the kurtosis . A kurtotic am-
plitude distribution is produced by cortical simple cells, leading to
sparse coding. Hence, ICA is believed to be a better model than
PCA for the output of simple cortical cells.
The receptive ﬁelds of simple cells in the mammalian striate cor-
tex are localized in space, oriented and bandpass. They are there-
fore similar to the basis functions of wavelet transforms [12, 23].
For natural images, strong correlations between wavelet coefﬁ-
cients at neighboring spatial locations, orientations and scales have
been shown using conditional histograms of the coefﬁcients’ log
magnitudes . These results were successfully used to synthe-
size textures [27,36] and to denoise images .
For statistical approaches to be useful in computer graphics appli-
cations, it is important to be able to attach a physical meaning to
the statistics that are found. For the higher order methods in the
previous sections, we would be interested in the statistics of the
coefﬁcients, rather than the appearance of the basis functions. In
the absence of sufﬁcient data on these statistics, we choose to ig-
nore these results for the moment and instead focus on the widely
accepted second order statistics as discussed in section 2. In this
paper we study which aspects of rendering and modeling inﬂuence
second order statistics.
3 Calculation of image statistics
To verify our approach, three different image ensembles were used.
Two of these ensembles consist of synthetic images, while the
third ensemble consists of natural images from the van Hateren
database . This last ensemble consists of just over 4000 cali-
brated images of outdoor scenes, 133 of which were randomly cho-
sen to form our natural image ensemble. Below, we will refer to
this as ensemble “A”.
For the artiﬁcial image ensembles, research images from vari-
ous internet sites were collected. Images that had obvious copy-
Figure 1: Example images drawn from ensemble “A”.
Figure 2: Example images drawn from ensemble “B”.
Figure 3: Example images drawn from ensemble “C”.
right notices were rejected, as well as images that were smaller
than 512x512 pixels. Further, both the rendering and the model-
ing had to be of high subjective quality. Images which had obvious
markings of post-processing, as well as camera speciﬁc artifacts
(depth of ﬁeld), were also rejected. The images thus collected were
subdivided into two groups, where the classiﬁcation was based on
the subjective quality of the modeling. The high quality modeling
ensemble (ensemble “B”) consists of 30 images and the ensemble
with slightly simpler modeling has 18 images (ensemble “C”). Ex-
ample images of all three ensembles can be found in Figures 1 to 3.
The images in the natural image ensemble are available as lumi-
nance images. The synthetic images are usually given in someRGB
format. Where appropriate, these wereconverted to a 24 bit uncom-
pressed ﬁle format (theinﬂuence oflossy compressionon thepower
spectra is assessed in Section 5). All subsequent computations were
performed on the Y (luminance) channel, after conversion to YUV.
For these image ensembles (as well as for individual images), the
power spectra were computed and the spectral slope was estimated.
The power spectrum computation proceeds as follows (after ):
For images that are larger than 512x512 pixels, a window of this
size was cut out of the middle of the image upon which further
processing was applied. Then, the weighted mean intensity µ was
subtracted to avoid leakage from the DC-component of the image,
with µ deﬁned as:
L(x, y)w(x, y)
Next, the images were preﬁltered to avoid boundary effects. This
is accomplished by applying a circular Kaiser-Bessel window func-
tion (with parameter α =2) to the image :
1.0 − (
is the modiﬁed zero-order Bessel function of the ﬁrst kind
and N is the window size (512 pixels). In addition, this weight
function was normalized by letting:
This windowing function was chosen for its near-optimal trade-off
between side-lobe level, main-lobe width and computability .
The resulting images were then Fourier transformed:
F (u, v)=
L(x, y) − µ
Finally, thepower spectrum wascomputed as per equation1 and the
resulting data points plotted. Although frequencies up to 256 cycles
per image are computed, only the 127 lowest frequencies were used
to estimate the spectral slope. Higher frequencies may suffer from
aliasing, noise and low modulation transfer . The estimation of
the spectral slope was performed by ﬁtting a straight line through
the logarithm of these data points as function of the logarithm of
1/f. This method was chosen over other slope estimation tech-
niques such as the Hill estimator  and the scaling method 
to maintain compatibility with . In addition, the number of
data points (127 frequencies) is insufﬁcient for the scaling method,
which requires at least 1,000 data points to yield reliable estimates.
4 Image ensembles
For the three image ensembles, second order statistics were ex-
tracted as detailed above. The 1.87 (±0.43 standard deviation)
spectral slope for the van Hateren database was conﬁrmed: we
found 1.88 ± 0.42 s.d. for our subset of 133 images. The devia-
tions from this value for the artiﬁcial image ensembles are depicted
in Figure 4. These results show that our synthetic image ensembles
produce straight power spectra, although the total amount of con-
trast and the value of the slope vary. It is also interesting to note that
the subjective classiﬁcation into two separate synthetic image en-
sembles using quality of modeling as criterion, has produced power
spectra that are markedly different.
Especially the area under the data points, which can be inter-
preted as a measure for contrast, is an order of magnitude higher for
the high quality syntheticensemble. It is possible that the subjective
selection criterion was subconsciously guided by the human visual
system’s tendency to prefer viewing areas with high contrast .
The angular distribution of power tends to show peaks near hor-
izontal and vertical angles. Both the natural image ensemble “A”
and the high quality synthetic image ensemble “B” show this (Fig-
ure 5). The lower quality synthetic ensemble “C” shows a distinct
lack of power in horizontal directions, but has peaks present in ver-
Power vs. spatial frequency
Spatial frequency (cycles/image)
A: Slope 1.88
B: Slope 1.92
C: Slope 1.97
Figure 4: Spectral slopes for the three image ensembles: A natural
image ensemble, B high quality synthetic ensemble and C lower
quality synthetic ensemble. The double lines indicate ±2 standard
deviations for each ensemble.
0 30 60 90 120 150 180 210 240 270 300 330 360
Average power per direction
log average power
Figure 5: Log average power as function of angle.
Differences between the artiﬁcial image ensembles and the nat-
ural ensemble may be partially explained by the fact that rendered
imagery predominantly depicts indoor scenes, whereas ensemble
“A” is exclusively outdoors.
While the two synthetic ensembles produce straight lines with
spectral slopes that fall well within the range of slopes observed
in natural images, individual images tend to deviate fairly strongly
from the average. In the following sections, we assess which parts
of the rendering pipeline affect second order statistics, which goes
towards establishing these statistics as a tool for graphics applica-
5 Image manipulation
In this and the following sections we empirically evaluate which
aspects of rendering and modeling affect the spectral slope. Start-
ing with issues relating to image space, possible artifacts may arise
from lossy compression for ﬁle formats, such as gif and jpeg,
gamma correction and aliasing. Each of these is discussed in turn,
using a high quality rendering created using Radiance . The
Figure 6: Test scene, modeled to a spatial resolution of 1 mm.
modeling for this image (depicted in Figure 6) was done by hand to
a resolution of 1 mm. This provides a detailed scene as encountered
in many graphics applications.
The lighting simulation included diffuse inter-reﬂection and soft
shadows. An image was created at 512x512 pixels with 64 super-
samples per pixel, which was subsequently converted to PPM. The
tests in the following subsections all pertain to this rendered image,
which has a measured spectral slope of α =2.36.
5.1 File formats
Lossy compression, as employed by various different ﬁle formats,
may cause the frequency content of images to change. To see
whether substantial modiﬁcations occur, the above PPM image was
converted to GIF and JPEG (the latter using different levels of qual-
ity and smoothing) using XV. With the exception of smoothing,
which destroys high frequency content, the effect of ﬁle conver-
sion on the spectral slope is generally benign with deviations less
than 1%. For different levels of smoothing, the spectral slope varies
linearly with the amount of smoothing applied during ﬁle conver-
Hence, moderate levels of compression do not have an apprecia-
ble effect on the measured spectral slope. We therefore conclude
that the different ﬁle formats used in image ensembles B and C
above, did not signiﬁcantly affect our results.
5.2 Gamma correction
Gamma correction is a non-linear transformation to adapt the ap-
pearance of an image to a particular display device. As such, the
spectral information present in the image may be affected due to
the non-linear nature of the transformation. However, our measure-
ments using the gamma correction option in XV show that the spec-
tral slope is only weakly dependent on gamma correction value, as
can be seen in Figure 7. The largest deviations occur for extreme
gamma correction values that strongly darken the image
It is therefore concluded that gamma correction does not consti-
tute a signiﬁcant factor in the determination of spectral slopes and
therefore does not substantially inﬂuence our results of Section 4.
Aliasing is another factor which may affect the spectral slope by
projecting frequencies above the Nyquist limit to lower frequen-
0.4 0.8 1.2 1.6 2 2.4 2.8
Spectral slope vs. gamma correction
Figure 7: Spectral slope vs. gamma correction value.
1x1 2.23 0.15
2x2 2.32 0.19
4x4 2.35 0.20
8x8 2.36 0.20
Table 1: Spectral slope α and standard deviation σ as function of
super-sampling. Slope α changes less than 1% if 16 or more super-
samples are computed per pixel.
cies. Despite careful consideration of this issue by using only
the 127 lowest frequencies in the spectral computations, as ex-
plained in Section 3, the rendering process itself may still cause
aliasing at lower frequencies. Images with different numbers of
super-samples were computed, suppressing aliasing by different
amounts. Table 1 shows how the spectral slope depends on the
number of super-samples. In order to minimize aliasing artifacts
in the Fourier domain, it appears that at least 16 super-samples per
pixel are needed. All the renderings in this and following section
use 64 super-samples, eliminating aliasing as a possible factor.
6 Modeling or rendering?
From the previous section it is clear that most of the distortions
regularly applied to synthetic images do not unduly affect our spec-
tral analysis. In this section we extend our analysis to the spatial
domain and answer the question whether second order statistics ap-
ply to lighting simulation or modeling. The scene as described in
the previous section was used for rendering images using differ-
ent lighting simulations: with and without diffuse inter-reﬂection
as well as with and without shadow rays.
Depending on the nature of the scene rendered, shadows can make
an important contribution to the overall appearance of a scene.
Hence, the accuracy with which shadows are rendered may affect
the statistics of the resulting image. By varying the size of the light
sources and adjusting their emission to maintain constant light lev-
els, the effect of varying soft shadows on second order statistics
was measured. Table 2 shows that for our room scene, shadows do
not appear to be an overly important factor for computing image
statistics. However, it should be noted that special cases could be
constructed which prove the contrary.
6.2 Diffuse inter-reﬂection
We have also assessed the inﬂuence of diffuse inter-reﬂection on
second order statistics. As diffusely reﬂecting surfaces are unlikely
Size Energy ασ
1/8 64 2.35 0.20
1/4 16 2.35 0.20
1/2 4 2.35 0.20
1 1 2.36 0.20
2 1/4 2.36 0.20
4 1/16 2.37 0.21
Table 2: Spectral slope α and its standard deviation σ as function
of light source size and energy (both multiplication factors).
to produce high spatial frequencies due to their illumination, we ex-
pect an even smaller effect than for the light source tests above. The
largest difference occurs when switching from lighting simulations
without diffuse inter-reﬂection to those with diffuse inter-reﬂection.
This changed the spectral slope by 5.5%.
As adding diffuse inter-reﬂection to the lighting computations
produced a marked effect, we were wondering whether this is due
to an overall increase in energy in the environment. Ray tracing al-
lows a constant ambient to be added to each shading result, which
increases image intensities. It was found that this produced the
same effect. Hence, we conclude that absolute energy levels are
more important than the low-frequency distribution associated with
It appears that the particular details of the lighting simulation,
whether it be soft or hard shadows, diffuse inter-reﬂection etc. do
not signiﬁcantly inﬂuence second order image statistics. Differ-
ences between renderers, suchas ray tracing and OpenGL rendering
with Phong shading, also did not prove essential (data not shown).
We therefore conclude that these statistics are invariant to rendering
details. Although second order statistics can not be used to differ-
entiate between lighting simulations, this makes them ideal tools
for assessing quality of modeling. We provide evidence for this
hypothesis through the example of fractal terrain modeling.
7 Sample application: fractal terrains
We would expect natural image statistics to be useful in any real-
istic rendering application that normally involves parameter tuning
such as solid texture creation , procedural plant modeling 
or displacement mapping [8, 37]. We have chosen procedural ter-
rain modeling as our test for whether natural image statistics can be
useful for automatic parameter selection.
We implemented the midpoint subdivision algorithm of Fournier
et al. . That algorithm iteratively adds smaller and smaller ran-
dom displacements to smaller and smaller spatial scales. As the
scale decreases by a factor of 2, the magnitude of displacement de-
creases by a factor k. Smaller values of k result in rougher ter-
rain, and larger values result in smoother terrain. Figure 10 shows
twelve terrain models using k =1.5 to k =2.6 after applying 10
iterations. The terrains, each consisting of 524, 288 triangles, were
rendered in Radiance with diffuse inter-reﬂection and an 11 o’clock
sky model . The resulting images have an approximately linear
relationship between spatial frequency and spectral slope. Figure 8
demonstrates this behavior, along with the observation that for all
values of parameter k, the spectral slope decreases predictably with
each iteration of the algorithm. The relationship between division
parameter k and spectral slope shows after 10 iterations a minimum
of 1.40 for parameter k =2.1. The value of the spectral slope in-
creases slightly for rougher terrains, which we believe to be caused
by self-shadowing. However, this effect is small and does not inter-
fere with our results.
Figure 8: The spectral slope for each iteration of the terrain gener-
ation process and for each of the 12 resulting terrains of Figure 10.
k = 1.5 1.6 1.7 1.8 1.9 2.0 2.1 2.2 2.3 2.4 2.5 2.6
Number of responses
Figure 9: Responses from 52 participants using prints and 31 par-
ticipants who performed the web based experiment. The histogram
shows both the spectral slope and the division parameter k associ-
ated with the images in Figure 10.
If we wereto set k automatically to produce an image withstatis-
tics tuned to the human visual system, we would use a k which pro-
duces images with spectral slopes near 1.88, as this was the value
found for the natural image ensemble “A” (Section 4). This corre-
sponds to a value of k close to 2.2. To evaluate this selection of
k we asked 30 people to pick the most realistic image from Fig-
ure 10. The images, rendered at a resolution of 1024
each printed on a single sheet at a resolution of 300dpi, yielding
cm. prints. These prints were then presented to the partici-
pants in a randomly ordered pile. We asked the subjects to select
the image that looked most realistic. To make sure that geographic
location did not bias the participants, the experiment was repeated
using participants from both North America and Europe. This lat-
ter experiment was conducted using aweb page toshow the images.
Again, the question asked was to selected the most realistic image.
The results of both experiments are shown in Figure 9. This
histogram shows the number of responses obtained for each terrain.
The peaks of the histograms lie close to k =2.1 and k =2.2.
This corresponds to a spectral slope of between 1.70 and 1.86. The
selection that ourparticipants made correlates to theselection based
on spectral analysis of the terrain images (which would be k =
2.2). Additionally, the mean value lies well within one standard
deviation of the natural image ensemble “A” (α =1.88±0.42 s.d.),
suggesting that people would select images with “natural” statistics
if they were given the choice.
We therefore conclude that this analysis can be successfully used
for parameter selection in fractal terrains. The agreement between
user and algorithmic image selection suggests that this statistical
approach lends itself to wider usage in graphics applications, espe-
cially those applications where computer generated imagery needs
to be evaluated for realism or parameters need to be tuned.
Because computer graphics applications should produce cues ap-
propriate for the HVS, it is important to understand what kind of
images the HVS expects. We have surveyed natural image statis-
tics and the most salient one, 1/f
power spectra, was investigated
further. We established that this image statistic is sensitive to geom-
etry, while the entire rendering pipeline seems to not signiﬁcantly
affect this statistic. Hence, modeling applications can beneﬁt from
applying second order statistics, as shown by an example appli-
cation in the form of fractal terrain modeling. We envisage these
statistical tools to be able to provide criteria for a wide range of
graphics applications, as argued in the previous section.
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