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A permutation test for comparing rotational symmetry in threedimensional rotation data sets
Journal of Statistical Distributions and Applications volume 4, Article number: 19 (2017)
Abstract
Although there have been fairly recent advances regarding inference for threedimensional rotation data, there are still many areas of interest yet to be explored. One such area involves comparing the rotational symmetry of 3D rotations. In this paper, nonparametric inference is used to test if F _{1}=F _{2}, where F _{ i } is the degree of rotational symmetry of distribution i, through a permutation test. The validity of the developed permutation test is examined through a simulation study and the test is applied to a small example in biomechanics.
Introduction
Threedimensional rotation data sets are commonly collected in the study of human motion (Rancourt et al. 2000; Rivest et al. 2008; Haddou et al. 2010; Oualkacha and Rivest 2012) and in materials science (e.g., crystal orientations in metals, Demirel et al. 2000; Wilson and Spanos 2001). Until recently, most developments regarding analysis of 3D rotations used the matrix Fisher distribution as the underlying statistical distribution (Khatri and Mardia 1977; Jupp and Mardia 1979; Prentice 1986; Mardia and Jupp 2000; Rancourt et al. 2000). Recognizing the limitations of existing distributions for 3D rotations, Bingham et al. (2009) developed the Uniform AxisRandom Spin (UARS) class of distributions, Bingham et al. (2012) developed the Preferred AxisRandom Spin (PARS) class of distributions, and Oualkacha and Rivest (2009) developed a new model for symmetric axial directional data. While these recent works provide much more flexibility in modeling 3D rotations, their focus is on fitting the developed distributions to a single data set. Further, there appears to be a disconnect between developments in the statistical literature for 3D rotations and what is easily understood and used by practitioners who collect such data. For example, Pierrynowski and Ball (2009) point out that even standard operations, such as finding mean rotations, are often incorrectly applied by movement scientists.
The need for greater flexibility in modeling 3D rotations, coupled with the need for easily accessible inference procedures, has led to recent works on nonparamteric methods for 3D rotation data. Stanfill et al. (2015) and Will and Bingham (2016) focus on estimating the central rotation through bootstrapping, while Bero and Bingham (2015) explore permutation tests for comparing the central rotations in two data sets. Bingham (2015) uses bootstrapping to quantify the spread in 3D rotations and Eckrote and Bingham (2017) develop a permutation test for comparing the spread in two data sets. These works do provide techniques for analyzing 3D rotation data that are easily implemented by practitioners, but center and spread are not the only features that distinguish 3D distributions. Therefore, this paper aims to fill a gap by developing statistical techniques for comparing the rotational symmetry of the distributions from which two data sets come. This will provide a novel statistical approach for analyzing 3D rotation data while also providing useful tools for practitioners.
In Section 2 further details on the UARS and PARS classes of distributions for 3D rotations are provided. In Section 3 the permutation test for comparing symmetry in two 3D rotation data sets will be developed. In Section 4 a simulation study will be used to investigate the power of the permutation test under various conditions. Finally, in Section 5, the permutation test will be used briefly in an application to compare movement around the calcaneocuboid joint for a human, chimpanzee, and baboon.
Overview of distributions for 3D rotations
In many applications involving 3D rotation data, the rotational distributions used are symmetric (or isotropic) so that they have rotationally invariant densities about a central rotation. Mardia and Jupp (2000, p. 179) give a general definition of rotational symmetry on the (p−1)sphere, \(S^{p1}=\left \{\mathbf {x}\in \mathbb {R}^{p}: \mathbf {x}^{T}\mathbf {x}=1\right \}\), as having density functions of the form f(x)=g(μ ^{T} x). The case of p=4 corresponds to the space SO(3), the set of all 3×3 orthogonal rotation matrices. Qiu et al. (2014) give a thorough overview of rotationally symmetric distributions on SO(3). As the authors show, existing rotationally symmetric distributions that appear in the literature are part of the general class of isotropic distributions on SO(3), the UARS distributions.
We first provide a brief overview of the UARS class of distributions. Although we consider elements of SO(3) as 3×3 matrices throughout this paper, they could equivalently be expressed in terms of quaternions and Bingham et al. (2009) briefly discuss this representation of the UARS class. Let O∈ SO(3) be a random rotation from a UARS distribution with central rotation S. Then O=S P, where P is obtained by rotating the 3×3 identity matrix, I _{3×3}, about an axis \(\mathbf {U} \in \mathbb {R}^{3}\) by a random angle r∈(−π,π]. In this case of the UARS class, r follows some circular distribution that is symmetric about 0 with spread depending on parameter κ>0, and U is uniformly distributed on the unit sphere. (See Mardia and Jupp (2000) for details on spherical distributions.) Since larger values of κ indicate less spread in the rotations, κ is referred to as a concentration parameter. This distribution will be abbreviated as UARS(S,κ). See Bingham et al. (2009) for extensive details on the UARS class, including an expression for the matrix P (page 1388, Eq. 2) and the UARS(S,κ) density (page 1389, Eq. 4).
Bingham et al. (2012) develop a broad class of distributions that are not rotationally symmetric (referred to here as nonsymmetric) by beginning with the symmetric UARS class. A short overview of the PARS class is provided here, but extensive details can be found in Bingham et al. (2012). Let P∼UARS(S,κ) and let V be some fixed vector. Rotate P around V by a random angle p∈(−π,π], where p follows some circular distribution that is symmetric about 0 with concentration parameter τ>0. If the resulting matrix is T, then S T is said to have PARS distribution with central rotation S, preferred axis of rotation V, and concentration parameters κ and τ. This distribution will be abbreviated as PARS(S,κ,V,τ). As Bingham et al. (2012) show, by introducing the extra rotation around V, rotationally symmetric rotations are “smeared” to create nonsymmetric rotations.
For both the UARS and PARS classes of distributions, a particular distribution is specified by choosing the circular distribution(s) for the random angles r and p. Figure 1 shows data sets that have been generated from (a) the UARS distribution with center at I _{3×3} and κ=50, (b) the PARS distribution with center at I _{3×3}, κ=50, \(\mathbf {V}=(1/\sqrt {3},1/\sqrt {3},1/\sqrt {3})\), and τ=25, and (c) the PARS distribution with center at I _{3×3}, κ=50, \(\mathbf {V}=(1/\sqrt {3},1/\sqrt {3},1/\sqrt {3})\), and τ=10. The von Mises circular distribution (see Bingham et al. 2009) has been used for both r and p. In each figure a 3×3 rotation matrix is displayed as three points on the sphere, one representing each of the three perpendicular axes that correspond to the three columns in the matrix. The center at I _{3×3} is represented by the axes at x, y, and z. We can see that smaller values of τ for the PARS distribution represent data that are more nonsymmetric in nature. The goal of this work is to develop methods for determining if two data sets like the ones displayed in Fig. 1 come from underlying distributions with different degrees of rotational symmetry. In the next section a permutation test is developed to accomplish this.
Development of the permutation test
Suppose O _{1},…,O _{ n } and P _{1},…,P _{ m } are two 3D rotation data sets of sizes n and m. To begin, the mean rotation for each data set will be found. The mean rotation for a set of 3D rotations, M, is a commonly used measure of center which is defined as the rotation that maximizes \(\text {trace}(\mathbf {M}^{T} \bar {\mathbf {O}})\), where \(\bar {\mathbf {O}}=\frac {1}{n}\sum _{i=1}^{n} \mathbf {O}_{i}\) (Khatri and Mardia 1977; Leoń et al. 2006; Bingham et al. 2009a). The mean rotation M can be found by using M=V W, where \(\bar {\mathbf {O}}=\mathbf {V}\boldsymbol {\Sigma }\mathbf {W}\) is the singular value decomposition of \(\bar {\mathbf {O}}\). The mean rotations for the two data sets under consideration will be denoted as M _{ O } and M _{ P }.
For each observation in O _{1},…,O _{ n }, there exists an axis A _{ Oi } such that a rotation by angle \(\arccos [\!(\text {trace}\left (\mathbf {M}_{O}^{T}\mathbf {O}_{i}\right)1)/2]\) about A _{ Oi } will result in the mean M _{ O }. A _{ Oi } can be found by considering the axis part of the axisangle representation of \(\mathbf {M}_{O}^{T}\mathbf {O}_{i}\), i=1,…,n. The axes between P _{1},…,P _{ m } and M _{ P } will also be found and are represented as A _{ Pj }, j=1,…,m. Because rotationally symmetric distributions on SO(3) can be regarded as part of the UARS class (Qui et al. 2014), these axes will be uniform when considering symmetric distributions on SO(3). (See also Bingham et al. (2009); Mardia and Jupp (2000); Watson (1983).)
In order to determine if the resulting axes are uniformly distributed, the quantity
proposed by Mardia and Jupp (2000, p. 232) will be calculated for each set of axes A _{ O1},…,A _{ On } and A _{ P1},…,A _{ Pm }. Smaller values of R in (1) indicate uniform axes, translating to rotational symmetry on SO(3). We note that although the main focus of this paper is to compare two data sets in terms of rotational symmetry using a permutation test, the quantity R can be used to determine whether or not a single data set comes from a distribution with rotational symmetry as well. Under uniformity of the axes, R has approximately a \(\chi ^{2}_{5}\) distribution (Mardia and Jupp 2000). Thus we can test for rotational symmetry of a single 3D rotation data set by using R as a test statistic. A small simulation study for this onesample test is provided in Section 4.
To compare the rotational symmetry in two independent 3D rotation data sets, the absolute difference in R values can be calculated to serve as the test statistic for the permutation test of H _{0}:F _{1}=F _{2} versus H _{ a }:F _{1}≠F _{2}, where F _{ i } is the degree of rotational symmetry of distribution i. The steps of the permutation are listed below.

1.
Calculate the statistic in Eq. (1) for each data set, giving R _{ O } and R _{ P }, respectively. Calculate θ _{ obs }=R _{ O }−R _{ P }, which will serve as the observed test statistic.

2.
Permute the data by combining the two data sets and randomly reassigning n observations to the first set and m to the second. Calculate θ _{ perm }=R _{ O }−R _{ P }, the permuted test statistic, based on the permuted data.

3.
Repeat step 2. a large number (say 10,000) of times.

4.
Let the pvalue be the fraction of times that the permuted test statistic is greater than the observed test statistic; pvalue \(= \frac {\text {\# of times }\theta _{perm} > \theta _{obs}}{\text {\# of permutations}}\).
The permutation test developed above is demonstrated here for two cases. In Fig. 2 a, the two simulated data sets (in white and black) appear to have similar degrees of rotational symmetry. When applying the permutation test above, these data sets resulted in a test statistic of 0.325 and a pvalue of 0.844. In Fig. 2 b, the simulated data sets have symmetries that differ by a greater amount, with the points in white being more symmetric than the points in black. These data sets gave a test statistic of 5.798 and a pvalue of 0.005, indicating a significant difference in the distributional symmetry. From these two examples, it can be seen that the pvalue decreases as expected when the data sets have symmetries that appear to differ more. In the next section the adequacy of the 3D permutation test for rotational symmetry is examined further by performing a simulation study.
Exploring power through simulations
First, a small set of simulations were done to test for rotational symmetry in the onesample case. 3D rotation data sets were simulated from PARS distributions using sample sizes of n=20 and 100 and concentration parameters of κ=5 and 100. The central rotation was fixed at the identity matrix and the preferred axis of rotation V was generated from the uniform distribution on the sphere for each simulation. The second concentration parameter τ was set at either 1, 5, 10, or 50. Smaller values of τ indicate a higher degree of nonsymmetry in the PARS class. The quantity R from (1) was used as the test statistic for testing a null hypothesis of rotational symmetry. Under rotational symmetry, \(R \sim \chi ^{2}_{5}\) (Mardia and Jupp 2000, p. 232). For each combination of n, κ, and τ, 1000 PARS data sets were simulated and used in the test. The proportion of times the test correctly rejected the null of rotationally symmetry was found, with results in Table 1. As expected, power increases as τ decreases and the underlying distribution becomes less symmetric. Power is also higher for the distribution with less spread (κ=100) and the larger sample size.
A more extensive simulation study was done to examine the effectiveness of the permutation test developed in the last section by considering the power of the test to correctly reject a null of equal degree of rotational symmetry for two distributions. A first 3D rotation data set was simulated from the nonsymmetric Preferred AxisRandom Spin (PARS) distribution (Bingham et al. 2012) with rotations r and p from the von Mises distribution. The central rotation was fixed at the identity matrix, since choice of center does not have a bearing on the rotational symmetry. For this PARS(I _{3×3},κ,V,τ) data set, V was generated from the uniform distribution on the sphere, κ was chosen to be 5, 20, 50, or, 100, and τ was varied from very small (0.01) to very large (500), with this range reflecting less symmetric to more symmetric, respectively. Sample sizes of n=20,50, or 100 were used. Using the same values of κ and n, a second data set was simulated from the rotationally symmetric von Mises version of the Uniform AxisRandom Spin distributions, vMUARS(I _{3×3}, κ) (Bingham et al. 2009).
For each combination of n, κ, and τ, 1000 different samples were simulated from each of the vMUARS(I _{3×3}, κ) and PARS(I _{3×3},κ,V,τ) distributions. For each of the 1000 cases, the rotational symmetries of the two data sets were compared using the permutation test with 1000 permutations per test, and the power was calculated as the fraction of times that the permutation test correctly rejected the null hypothesis of similar symmetries (using a significance level of 0.05). It is expected that smaller values of τ should result in higher power, because a PARS data set with less symmetry is being compared to a symmetric vMUARS data set. Thus, power was plotted against 1/τ and Fig. 3 shows the results for each choice of κ and n.
Each plot shows that the power of the test increases as 1/τ increases and as n increases. By comparing the four plots, it can also be seen that power increases as the data are less spread (i.e. larger values of κ). These relationships between power and the varied quantities are all as to be expected. As 1/τ increases the rotational symmetry of the simulated data sets are less alike, making the test more powerful. As both sample size increases and as the data become less spread, the test becomes more powerful. In the cases of n=20 with smaller values of κ, power of only approximately 0.5 is achieved. This is because in small data sets exhibiting a high degree of spread, it is much harder to identify the distribution as being either symmetric or nonsymmetric, resulting in the test detecting a difference in symmetries less often. Since all of the features of power seen through the simulation study match what is expected, the permutation test for rotational symmetry is performing as desired in terms of power.
Additionally, simulations were conducted to investigate the Type I error rate for the permutation test. For these simulations, the two data sets were generated from the same distribution, so that we would expect the test to not result in rejection of the null hypothesis. The permutation test was done with 1000 permutations and repeated 100 times for each scenario. The simulated Type I error rate was then calculated as the proportion of the times (out of 100) that the pvalue was less than or equal to 0.05. Results for both the UARS and PARS (with τ=0.01,10, and 500) distributions are provided in Table 2 for various choices of n and κ. All values are close to the desired 0.05, showing that the permutation test also behaves as expected when the two distributions under consideration are the same.
Brief Application to Calcaneocubiod joint rotation data
Since it has been verified that the 3D permutation test performs as desired when it comes to both power and Type I error rate, the test will be applied to calcaneocuboid joint data. The data used here were collected by Professor Thomas Greiner, Physical Therapy, at the University of WisconsinLa Crosse. Infrared emitting diodes were attached to the calcaneous and cuboid bones of the foot in a human, baboon, and chimpanzee. Load was applied to the knee while the subjects had their foot flat on the floor. The rotation of the calcaneocuboid joint between the two bones was recorded. Although 125 measurements were collected over time as the load was applied, these observations will be assumed to be independent and identically distributed for the purposes of illustration.
The data were collected with the goal of comparing the species’ movement around the joint with respect to its variability and rotational symmetry, with it being hypothesized that there would be differences appearing among all species. Eckrote and Bingham (2017) found significant differences in variability for the baboon and chimp and for the human and baboon. We test for differences in degree of rotationally symmetry here. The permutation test for comparing rotational symmetry was conducted pairwise for human versus chimpanzee, human versus baboon, and chimpanzee versus baboon, with 1000 permutations used per test. All three of the permutation tests resulted in a pvalue of approximately 0, suggesting that there is a difference in the rotational symmetry for all three comparisons, as hypothesized. This also matches the result of Bingham et al. (2012) where confidence intervals for the parameter τ in the PARS distribution were investigated for overlap. While the inference of Bingham et al. (2012) only applied to a single sample at a time, the permutation test considered here allows for direct comparison of two data sets through a single test, making it preferred for this type of application.
Conclusion
Although applied to a small example in biomechanics, the permutation test developed here has applications reaching beyond just the study of movement in skeletal mammals. Data in the form of 3D rotations are found in multiple disciplines, making techniques for comparing symmetry in these data sets important. Since the test developed here is nonparametric, it can be used in situations where one of the few 3D rotation distributions does not provide an adequate fit to the data. Its nonparametric nature also allows it to be easily implemented, making it accessible to practitioners who collect 3D rotation data. Thus, the 3D permutation test for rotational symmetry is valuable not only for statisticians, but also for those who work with 3D rotation data in practice.
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Acknowledgments
Thank you to Dr. Thomas Greiner, University of WisconsinLa Crosse, for providing the data used in the application. Thank you to the reviewers for their detailed comments and suggestions that greatly improved the quality of the manuscript.
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Bingham, M.A., Scray, M.L. A permutation test for comparing rotational symmetry in threedimensional rotation data sets. J Stat Distrib App 4, 19 (2017). https://doi.org/10.1186/s4048801700752
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Keywords
 Directional data
 Threedimensional rotations
 Permutation test
 Rotational symmetry
Mathematics Subject Classification:
 62H11
 62G09
 62G10