Stereology Spheres Other shapes Wicksell’s Corpuscle Problem Markus Kiderlen, CSGB Kolloquium at Osnabrück University June 18, 2014 Local Wicksell pb. Stereology Spheres Other shapes 0. Stereology at the CSGB. Local Wicksell pb. Stereology Spheres Other shapes Local Wicksell pb. Prologue: What is stereology? Stereology is ‘spatial sampling theory’: estimation of geometric charcteristics from section or projection samples of an object. Typical problem: estimate the volume of the hippocampus. Possible solutions: Stereology Spheres Other shapes Local Wicksell pb. Prologue: What is stereology? Stereology is ‘spatial sampling theory’: estimation of geometric charcteristics from section or projection samples of an object. Typical problem: estimate the volume of the hippocampus. Possible solutions: 1. Archimedes: Stereology Spheres Other shapes Local Wicksell pb. Prologue: What is stereology? Stereology is ‘spatial sampling theory’: estimation of geometric charcteristics from section or projection samples of an object. Typical problem: estimate the volume of the hippocampus. Possible solutions: 1. Archimedes: 2. Stereology. Stereology Spheres Other shapes Local Wicksell pb. Volume estimation with stereology Let X ⊂ R3 be an (smooth) object in the unit cube [0, 1]3 . Choose a randomized plane P parallel to the x-y -plane. Mean value stereology: We have E λ2 (X ∩ P) = λ3 (X ), where λn is Lebesgue measure in Rn and E is usual expectation. Intuitive reason: The section is Resentative as the position of P is randomized. Stereology Spheres Other shapes Local Wicksell pb. Volume estimation with stereology Let X ⊂ R3 be an (smooth) object in the unit cube [0, 1]3 . Choose a randomized plane P parallel to the x-y -plane. Mean value stereology: We have E λ2 (X ∩ P) = λ3 (X ), where λn is Lebesgue measure in Rn and E is usual expectation. Intuitive reason: The section is Resentative as the position of P is randomized. Classical stereology: position and orientation of P are randomized. ‘kinematic averages’. Stereology Spheres Other shapes Local Wicksell pb. Volume estimation with stereology Let X ⊂ R3 be an (smooth) object in the unit cube [0, 1]3 . Choose a randomized plane P parallel to the x-y -plane. Mean value stereology: We have E λ2 (X ∩ P) = λ3 (X ), where λn is Lebesgue measure in Rn and E is usual expectation. Intuitive reason: The section is Resentative as the position of P is randomized. Classical stereology: position and orientation of P are randomized. ‘kinematic averages’. Local stereology: only orientation of P is randomized. ‘rotational averages’. Stereology Spheres Other shapes Local Wicksell pb. What is needed for stereology? If we want the section to be representative: One of the two assumptions needed: • X is deterministic and the plane is suitably randomized. Design-based approach • the section plane is deterministic and fixed, but the the set is random and statistically homogeneous: Model-based approach Stereology Spheres Other shapes I. The classical Wicksell problem for spheres Local Wicksell pb. Stereology Spheres Other shapes The size distribution of particles Wicksell’s corpuscle problem: Determine the size-distribution of spherical particles from planar sections. Assume a model-based setting: • P is deterministic and • X a random collection of spheres; statistically translation invariant. ‘stationary marked point process with radii as marks’. • Wanted: ‘mark distribution’ FR = distribution function of spheres’ radii R in R3 . • We can estimate: Fr = distribution function of profiles’ radii r in E . Densities: fR and fr . Local Wicksell pb. Stereology Spheres Other shapes Local Wicksell pb. Why is this interesting? The Swedish statistician S.D. Wicksell was the first to formulate and solve this problem in the 1920ies. His research was motivated by two applications: Estimate size of ball-shaped cells in planar microscopy. Here: Hassal corpuscles in the thymus (’im lymphatischen System’). Stereology Spheres Other shapes Local Wicksell pb. Why is this interesting? The Swedish statistician S.D. Wicksell was the first to formulate and solve this problem in the 1920ies. His research was motivated by two applications: Estimate size of ball-shaped cells in planar microscopy. Here: Hassal corpuscles in the thymus (’im lymphatischen System’). Estimate the density of stars in a globular cluster from telescope observations. Stereology Spheres Other shapes Relations between R and r Two effects: 1. Given a sphere hits P, its radius Rw has 1 size weighted distribution: fRw (y ) = 2ER 2yfR (y ). Local Wicksell pb. Stereology Spheres Other shapes Local Wicksell pb. Relations between R and r Two effects: 1. Given a sphere hits P, its radius Rw has 1 size weighted distribution: fRw (y ) = 2ER 2yfR (y ). 2. Given sphere with radius Rw = y hits P, x fr (x|Rw = y ) = p , y y2 − x2 0 6 x 6 y. Stereology Spheres Other shapes Local Wicksell pb. Relations between R and r Two effects: 1. Given a sphere hits P, its radius Rw has 1 size weighted distribution: fRw (y ) = 2ER 2yfR (y ). 2. Given sphere with radius Rw = y hits P, x fr (x|Rw = y ) = p , y y2 − x2 =⇒ fr (x) = x ER R∞ x √fR (y ) dy 2 2 y −x 0 6 x 6 y. Stereology Spheres Other shapes The influence of the two effects • There are populations for which Er > ER (!) Local Wicksell pb. Stereology Spheres Other shapes The influence of the two effects • There are populations for which Er > ER (!) • Z is Rayleigh(σ)-distributed ⇐⇒ Z = √ X 2 + Y 2 , where (X , Y ) ∼ N(o, σ 2 ) Density: fZ (t) = t2 t − 2σ 2 e , σ2 t > 0. Reproducing property of the Rayleigh distribution R ∼ Rayleigh(σ) ⇐⇒ r ∼ Rayleigh(σ) • It is the only distribution with this property. • simple parametric models. [Wicksell 1925], [Keiding et al. 1972], mixture of χ-distributions, [Bach 1959] related distributions. Local Wicksell pb. Stereology Spheres Other shapes Local Wicksell pb. The integral equation and analytical unfolding fr (x) = x ER R∞ x √fR (y ) dy 2 2 y −x • First derived by [Wicksell 1925], • Proof by [Kendall & Moran 1963] (independence assumpt.) • General proof [Mecke & Stoyan 1980] . Stereology Spheres Other shapes Local Wicksell pb. The integral equation and analytical unfolding fr (x) = x ER R∞ x √fR (y ) dy 2 2 y −x • First derived by [Wicksell 1925], • Proof by [Kendall & Moran 1963] (independence assumpt.) • General proof [Mecke & Stoyan 1980] . This is an Abel integral equation with solution R∞ 1 − FR (y ) = π2 (2ER) y √fr 2(x) 2 dx. x −y • the Abel integral is smoothing, (corresponds to “1/2 integration”) • the unfolding problem is (moderately) ill posed Stereology Spheres Other shapes Numerical unfolding: a simple algorithm Discretization of the direct integral equation e.g. Scheil-Schwartz-Saltykov method r - q q q q q R Local Wicksell pb. Stereology Spheres Other shapes Local Wicksell pb. Numerical unfolding: a simple algorithm Discretization of the direct integral equation e.g. Scheil-Schwartz-Saltykov method q q q q q - r R Scheil−Schwartz−Saltikov, 8 bins 0.00 0.00 0.05 0.05 0.10 0.10 0.15 0.15 0.20 0.20 0.25 0.25 0.30 0.30 0.35 0.35 Scheil−Schwartz−Saltikov, 20 bins 0 2 4 R 6 8 0 2 4 6 8 R R, r ∼ Rayleigh(2), n = 1000 with 20 (left) and 8 (right) bins. Stereology Spheres Other shapes Local Wicksell pb. Conclusion: Numerical unfolding • subtle interplay of numerical and statistical problems, • the lower tail of FR is not accessible, • no method appears to be generally best, • large samples required, n ∼ 1000, in binning methods: low number of bins ∼ 7 − 10 or smoothing • Suggestion: pilot study as input for a non-parametric method proper study with a fitted parametric model (max. likelihood) Stereology Spheres Other shapes Local Wicksell pb. Variants • Thin sections of opaque spheres: “tomato salad problem” [Bach 1959, 1967,. . .]: Fr FR ; (ER + δ)Er k = ck ER k+1 + δER k , where 2δ = thickness of the slab. • Thin sections of transparent spheres “swiss cheese” [Coleman 1981,1982,1983] • Truncated Fr and measurement errors e.g. small sphere radii unobservable or inexact due to preparation [Cruz-Orive 1983], [Coleman 1980], . . . • Sections with lines: [Spektor 1950, Lord & Willis 1951] (more unstable than 2D sections) Stereology Spheres Other shapes Local Wicksell pb. II. Wicksell’s problem for other shapes Stereology Spheres Other shapes Local Wicksell pb. Ellipsoids General Wicksell problem for ellipsoids: Determine the joint distribution of the three principal axis in R3 from the joint distribution of two principal axis in the profiles. Stereology Spheres Other shapes Local Wicksell pb. Ellipsoids General Wicksell problem for ellipsoids: Determine the joint distribution of the three principal axis in R3 from the joint distribution of two principal axis in the profiles. • restrict attention to spheroids (= ellipsoids of revolution) Stereology Spheres Other shapes Local Wicksell pb. Ellipsoids General Wicksell problem for ellipsoids: Determine the joint distribution of the three principal axis in R3 from the joint distribution of two principal axis in the profiles. • restrict attention to spheroids (= ellipsoids of revolution) • In a population of prolate spheroids (“cigars”) we have uniqueness. Stereology Spheres Other shapes Local Wicksell pb. Ellipsoids General Wicksell problem for ellipsoids: Determine the joint distribution of the three principal axis in R3 from the joint distribution of two principal axis in the profiles. • restrict attention to spheroids (= ellipsoids of revolution) • In a population of prolate spheroids (“cigars”) we have uniqueness. • In a population of oblate spheroids (“flying saucers”) we have uniqueness. Stereology Spheres Other shapes Local Wicksell pb. Ellipsoids General Wicksell problem for ellipsoids: Determine the joint distribution of the three principal axis in R3 from the joint distribution of two principal axis in the profiles. • restrict attention to spheroids (= ellipsoids of revolution) • In a population of prolate spheroids (“cigars”) we have uniqueness. • In a population of oblate spheroids (“flying saucers”) we have uniqueness. • In a mixed population, we do not have uniqueness. Stereology Spheres Other shapes Local Wicksell pb. III. Wicksell’s problem with central sections for balls (joint with Ólöf Thórisdóttir) Stereology Spheres Other shapes Local Wicksell pb. Wicksell’s corpuscle problem in local stereology Local stereology: Particle properties from sections through a reference point P. For spherical particles: • In R3 : R = radius of the sphere (“size”) Q = relative distance of P from particle center (“shape”) Stereology Spheres Other shapes Local Wicksell pb. Wicksell’s corpuscle problem in local stereology Local stereology: Particle properties from sections through a reference point P. For spherical particles: • In R3 : R = radius of the sphere (“size”) Q = relative distance of P from particle center (“shape”) • In the isotropic section plane: r = radius of the section profile q = relative distance of P from profile circle center Problem: Find distributions of R and Q from those of r and q. Stereology Spheres Other shapes Local Wicksell pb. Integral relations Assume that Q and R are independent, P(Q = 0) = 0 1 − Fq (x) = Z fr (y ) = y y √ 1 1−x 2 ∞ √ 1 t 2 −y 2 Z 1 √ x R1 1 √ t s 2 −x 2 dFQ (s), s 1−(y /t)2 dFQ (s) s dFR (t). Hence: • q is independent of R • Fq determines FQ uniquely (analytic solution FQ = . . .) • The second integral is a generalized Abel integral. Stereology Spheres Other shapes Local Wicksell pb. Uniqueness in the local Wicksell problem Assume that Q and R are independent, P(Q = 0) = 0 The distributions of r and q determine those of R and Q. • There is no reproducing distribution like the Rayleigh-distribution before. • There are moment and extreme value relations for the radii. • It is open if the distribution of (q, r ) determines the distribution of (Q, R). • There is a two-step algorithm that resonstructs fQ and fR . Stereology Spheres Other shapes Local Wicksell pb. 1 1 0.9 0.9 0.8 0.8 0.7 0.7 0.6 0.6 FR(u) FQ(u) Unfolding example for the local Wicksell problem 0.5 0.5 0.4 0.4 0.3 0.3 0.2 0.2 0.1 0 0.1 0 0.1 0.2 0.3 0.4 0.5 u 0.6 0.7 0.8 0.9 1 0 0 1 2 3 4 5 u 6 7 True cumulative distribution functions for R (dashed) and step the functions from the unfolding. Left: Q ∼ unif[0, 1] (not shown) and R ∼ exp(1). Right: Q ∼ Beta(5, 2) (not shown) and R ∼ unif[0, 10]. 8 9 10 Stereology Spheres Other shapes Local Wicksell pb. References. R.S. Anderssen and A.J. Jakeman. Abel type integral equations in stereology. ii. computational methods of solution and the random spheres approximation. Journal of Microscopy, 105(2):135–153, 1975. G. Bach. Über die Grössenverteilung von Kugelschnitten in durchsichtigen Schnitten endlicher Dicke. Zeitschrift wiss. Mikroskopie, 57:265–270, 1959. G. Bach. 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Abel type integral equations in stereology: I. general discussion. Stereology Spheres Other shapes Local Wicksell pb. Journal of Microscopy, 105(2):121–133, 1975. M.G. Kendall and P.A.P. Moran. Geometrical probability. Hafner Pub. Co, 1st edition, 1963. S. Kötzer and I. Molchanov. On the domain of attraction for the lower tail in wicksell’s on the domain of attraction for the lower tail in wicksell’s corpuscle problem. In R.Lechnerova, I.Saxl, and V.Benes, editors, Proceedings S4G. International Conference on Stereology, Spatial Statistics and Stochastic Geometry. Prague, June 26-29, 2006., pages 91–96, 2006. J. Mecke and D. Stoyan. Stereological problems for spherical particles. Math. Nachr., 96:311–317, 1980. G.M. Tallis. Stereology Spheres Other shapes Local Wicksell pb. Estimating the distribution of spherical and elliptical bodies in conglomerates from plane sections. Biometrics, 26:87–103, 1970. R. Takahashi and M. Sibuya. Prediction of the maximum size in wicksell’s corpuscle problem. Annals of the Institute of Statistical Mathematics, 50:361–377, 1998. 10.1023/A:1003451417655. S.D. Wicksell. The corpuscle problem I. Biometrika, 17:84–99, 1925. S.D. Wicksell. The corpuscle problem II. Biometrika, 18:152–172, 1926.
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