Monday, January 25, 2016

Evaluation of Paralympic Basketball Athlete

Protocol of maximum speed in 5 meters starting from the resting state.
Brazilian Paralympic Athlete Paola Klokler (facebook/Paola Klokler 14), Jumper Equipment (facebook/JumperEquipamentos) Athlete.



Wednesday, April 1, 2015

Evaluation in Paralympic Athletics


Angular displacement amplitude of the elbow at the moment of propulsion. Brazilian Paralympic athlete Aline Rocha (facebook/alinerocha), Jumper Equipment (facebook/JumperEquipamentos) athlete.

Saturday, October 4, 2014

Data Normalization - Body-Size-Independent Measures

Muscle strength is strongly influenced by body size and correlated with measures such as Body Mass and Heigth; therefore, utilization of strength body-size-independent measurements for the aforementioned applications is important. The importance of this is especially apparent when comparing persons of different body sizes (ie, athletes vs nonathletes, men vs women, young vs old), or protocols where Body Mass could change between data collection periods (eg, long-term treatment). Normalizing strength measurements to measures of body size has traditionally been used to remove body-size dependence. However, there is no consensus on the method by which strength measurements should be normalized.


While some studies have not normalized strength measures, others have normalized strength to Body Mass or a combination of Body Mass and Heigth (ie, Body Mass X Heigth). Ratio standards (normalizing to Body Mass) assume that muscle strength is directly proportional to Body Mass. These assumptions, however, may result in misleading findings. An alternative to ratio standards is allometric scaling, a normalization technique based on the theory of “geometric similarity”, or that the shapes of human bodies are similar, but variable in size. Allometric scaling is a normalization technique that divides strength by Body Mass raised to a power that removes body-size effects. The equation for normalized strength is Sn=S/mb, where S is the non normalized strength measure, m is Body Mass, b is the allometric b-value (or scaler), and Sn is the body-size-independent strength measurement. 


In literature exists generic theoretical reference values for allometric adjustment of various parameters, but is more appropriate to use the specific exponent generated for your sample.


The normalization procedures included plot a linear regression with a log scale of peak strength parameters of your subjects by your respectives log scale Body Mass values aand then divide its strength parameters by their values of body mass raised to the slope found in linear regression.

Here's a link to download algorithm implemented in Matlab ® to perform the produre to calculate de allometric b-value of your sample. Matlab Code
 
To use the available function,first you must create a spreadsheet in excel with the "A" column containing the body mass in kg of its subjects and the "B" column containing the respective peaks of the strength parameters of the subjects. (ie. figure below)



The output of Allometry_gbiomech.m gives you the allometry b-value, the Confidence Interval of the measure and the R Squared value in a dialog box.

References:
- Lleonart, J.; Salat, J.; Torres, G. J. Removing allometric effects of body size in morphological analysis. Journal of theoretical biology 2000;205:1, p. 85–93.
- Jaric S. Muscle strength testing: use of normalisation for body size. Sports Med 2002;32, p. 615-31.
- Jaric, S.; Mirkov, D.; Markovic, G. Normalizing physical performance tests for body size: a proposal for standardization. Journal of strength and conditioning research / National Strength & Conditioning Association 2005;19:2, p. 467–474.
- Shingleton, A. W. Allometry: The Study of Biological Scaling. Nature Education Knowledge 2010;3:10.

Big Hug!

Tuesday, August 26, 2014

Numerical Integration - Simpson's Rule


In numerical analysis, numerical integration constitutes a broad family of algorithms for calculating the numerical value of a definite integral, and by extension, the term is also sometimes used to describe the numerical solution of differential equations. The term numerical quadrature (often abbreviated to quadrature) is more or less a synonym for numerical integration, especially as applied to one-dimensional integrals.
The basic problem in numerical integration is to compute an approximate solution to a definite integral

 




to a given degree of accuracy. If f(x) is a smooth function integrated over a small number of dimensions, and the domain of integration is bounded, there are many methods for approximating the integral to the desired precision.
An important part of the analysis of any numerical integration method is to study the behavior of the approximation error as a function of the number of integrand evaluations. A method that yields a small error for a small number of evaluations is usually considered superior. Reducing the number of evaluations of the integrand reduces the number of arithmetic operations involved, and therefore reduces the total round-off error. Also, each evaluation takes time, and the integrand may be arbitrarily complicated. 
A 'brute force' kind of numerical integration can be done, if the integrand is reasonably well-behaved, by evaluating the integrand with very small increments. 
A large class of quadrature rules can be derived by constructing interpolating functions that are easy to integrate. 
Typically these interpolating functions are polynomials.

The simplest method of this type is to let the interpolating function be a constant function (a polynomial of degree zero) that passes through the point ((a+b)/2, f((a+b)/2)). This is called the midpoint rule or rectangle rule.

 
 



The interpolating function may be an affine function (a polynomial of degree 1) that passes through the points (a, f(a)) and (b, f(b)). This is called the trapezoidal rule.

 




For either one of these rules, we can make a more accurate approximation by breaking up the interval [a, b] into some number n of subintervals, computing an approximation for each subinterval, then adding up all the results. This is called a composite rule, extended rule, or iterated rule. For example, the composite trapezoidal rule can be stated as



where the subintervals have the form [k h, (k+1) h], with h = (b−a)/n and k = 0, 1, 2, ..., n−1.
Interpolation with polynomials evaluated at equally spaced points in [a, b] yields the Newton–Cotes formulas, of which the rectangle rule and the trapezoidal rule are examples. Simpson's rule is a Newton-Cotes formula for approximating the integral of a function f using quadratic polynomials (i.e., parabolic arcs instead of the straight line segments used in the trapezoidal rule).
Quadrature rules with equally spaced points have the very convenient property of nesting. The corresponding rule with each interval subdivided includes all the current points, so those integrand values can be re-used.
 
 
 

In sport and exercise biomechanics the data are most commonly available for wich the process of integration is appropiate are data from force platforms and accelerometers. The force data from force plataforms can be used to compute acceleration following Newton's second law (F = m * a). In this example, the process of integration enables the velocity to be obtained, and the process can be repeated in this velocity data in order to obtain displacement. This method can be applied in other type of biomechanics data, for example in EMG, like contractile impulse of activation. Integration of this type of data is best done using numerical integration.
The numerical integration method most commonly found in the literature in the area of ​​biomechanics is the Trapezoidal. However, studies such as Won (2000) shows that we must have concern for the error produced by the choice of the integration method to be used and the method of Simpson is the one with the lowest error. 


Simpson's rule can be derived by integrating a third-order Lagrange interpolating polynomial fit to the function at three equally spaced points. In particular, let the function f be tabulated at points x_0, x_1, and x_2 equally spaced by distance h, and denote f_n=f(x_n). Then Simpson's rule states that







Since it uses quadratic polynomials to approximate functions, Simpson's rule actually gives exact results when approximating integrals of polynomials up to cubic degree. For example, consider f(x)=sinx (black curve) on the interval [0,pi/2], so that f(x_0=0)=0, f(x_1=pi/4)=1/sqrt(2), and f(x_2=pi/2)=1.




Then Simpson's rule (which corresponds to the area under the blue curve obtained from the third-order interpolating polynomial) gives

 





whereas the trapezoidal rule (area under the red curve) gives pi/4 approx 0.785398 and the actual answer is 1. In exact form,



where the remainder term can be written as

 



with x^* being some value of x in the interval [x_0,x_2].
An extended version of the rule can be written for f(x) tabulated at x_0, x_1, ..., x_(2n) as






where the remainder term is 





for some x^* in [x_0,x_(2n)]. 

Here's a link to download Matlab Code with a sub-program implemented in environment Matlab© to get the integration value of your signal with Simpson's Rule.
To use the function provided just save the file "simpson_gbiomech.m" in the same folder as the data to be analyzed. Then just call in your Matlab routine sub-program as follows in the example below:

Z=simpson_gbiomech(Y);      - computes an approximation of the integral of Y via the Simpson's method (with unit spacing). To compute the integral for spacing different from one, multiply Z by the spacing increment.

Z=simpson_gbiomech(X,Y);   - computes the integral of Y with respect to X using the Simpson's rule. X and Y must be vectors of the same length, or X must be a column vector and Y an array whose first non-singleton dimension is length(X). SIMPS operates along this dimension.


Note: you can specify the window which will be modified by inserting an index on the input variables.

References:
- Abramowitz, M. and Stegun, I. A. (Eds.). Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables, 9th printing. New York: Dover, p. 886, 1972.
- Davis, P. J.; Rabinowitz, P.. Methods of Numerical Integration. 
- Horwitz, A. "A Version of Simpson's Rule for Multiple Integrals." J. Comput. Appl. Math. 134, 1-11, 2001.
- Jeffreys, H. and Jeffreys, B. S. Methods of Mathematical Physics, 3rd ed. Cambridge, England: Cambridge University Press, p. 286, 1988.
- Stoer J.; Bulirsch R.. Introduction to Numerical Analysis. New York: Springer-Verlag, 1980. (See Chapter 3.)
- Trott, M. The Mathematica GuideBook for Programming. New York: Springer-Verlag, p. 105, 2004. http://www.mathematicaguidebooks.org/.
- Whittaker, E. T. and Robinson, G. "The Trapezoidal and Parabolic Rules." The Calculus of Observations: A Treatise on Numerical Mathematics, 4th ed. New York: Dover, pp. 156-158, 1967.
- Won, T. The comparison of among different numerical integration methods on the biomechanics of sport countermovement jump. 18º International Symposium on Biomechanics in Sports. Hong Kong, China: 2000. Available: <https://ojs.ub.uni-konstanz.de/cpa/article/view/2270/2123>

Big Hug!