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Long-range correlations in human standing

Long-range correlations in human standing

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126 M. Duarte, V.M. Zatsiorsky / Physics Letters A 283 (2001) 124–128Fig. 1. Position of the subjects on the force plate and axes convention (a). Two examples of stabilograms dur<strong>in</strong>g a 30 m<strong>in</strong> PUS: multi-region (b)and s<strong>in</strong>gle-region stand<strong>in</strong>g (c). Exemplary COP time series (d).ear least-squares fit, ŷ, and the curve is subsequentlydetrended. The variance of each w<strong>in</strong>dow’s detrendedsample path is calculated. The root of the mean variancesof all w<strong>in</strong>dows of length l is the detrended fluctuation,F ,ofthewalker:√F(l)=√ l/sNN/(l/s)∑n=11ll∑ [ ] 2.y(k)−ŷ(k)k=1The root-mean square fluctuations <strong>in</strong>crease with l,andif there is a l<strong>in</strong>ear relationship <strong>in</strong> a log–log scale of Fwith l, the data obey a power-law function, F(l)∼ l α ,where α is the scal<strong>in</strong>g exponent quantify<strong>in</strong>g the long<strong>range</strong><strong>correlations</strong>. For white noise, the exponent αis 0.5, for 1/f noise it is 1, and 1.5 for Brownian noise.For data with <strong>in</strong>f<strong>in</strong>ite length, the exponents α and β arerelated by the expression β = 1 − 2α [16].3. Results and discussion<strong>Long</strong>-<strong>range</strong> <strong>correlations</strong> for the COP data wereanalyzed for lags/w<strong>in</strong>dow lengths greater than 10 sand up to one-third (10 m<strong>in</strong>) of the 30 m<strong>in</strong> data. Thelower limit was selected to ignore the already reportedshort-<strong>range</strong> <strong>correlations</strong> for quiet stance <strong>in</strong> the <strong>range</strong>of 1 s [3]. The upper limit was chosen to obta<strong>in</strong>three <strong>in</strong>dependent sets of data, <strong>in</strong> order to <strong>in</strong>crease thestatistical power of the results. The fitted l<strong>in</strong>e for eachtrial <strong>in</strong> the region of 10 s to 10 m<strong>in</strong> represent<strong>in</strong>g thescal<strong>in</strong>g exponent (slopes) obta<strong>in</strong>ed by the DFA andPSA methods are shown <strong>in</strong> Fig. 2. The α exponentswere 0.98 ± 0.17 and 1.01 ± 0.26 for the a–p andm–l directions, respectively. The β exponents were−1.00 ± 0.42 and −1.27 ± 0.63 for the a–p andm–l directions, respectively. These results satisfiedthe relation β = 1 − 2α and <strong>in</strong>dicated the presenceof nontrivial long-<strong>range</strong> <strong>correlations</strong>. Because thereported values were less than the values for Brownianmotion, the <strong>correlations</strong> were <strong>in</strong> fact anti-<strong>correlations</strong>(negative <strong>correlations</strong>).The variability of α (expressed by the mean standarddeviations) was about 2.5 times lower than thevariability of β. As expected, this <strong>in</strong>dicated that theDFA method yielded more robust results that were lesssensitive to nonstationarities. The average value of αfor the COP data <strong>in</strong> the a–p and m–l directions was1.00 ± 0.22 (<strong>range</strong>: 0.68–1.47), which is equivalent to

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