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Figure 12: Short time scale part (t < 16 s) of the time scale spectrum of the X-ray pulsar 1E2259+586, ROR 400314. Vertical lines indicate position of different time scale components shown in Table 1. The logarithm of the time scale is displayed on the x-axis |
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Figure 13: An amplitude distribution graph for the ampligram in Fig. 8. (ROR 701246). The horizontal scale shows the normalized amplitude, vertical scale shows fraction of the maximum wavelet coefficient magnitude and the color scale shows the logarithm of the relative occurrence frequency |
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Figure 14: The distribution entropy as a of the fraction of the maximum wavelet coefficient magnitude for the distribution graph of Fig. 13 |
A complementary information may be obtained from the ampligram constructing a set of amplitude distributions of yl(ti), one for each level l of wavelet coefficient magnitude. For levels with pure stochastic component, Gaussian amplitude distributions will be obtained. For levels with deterministic components, broader amplitude distributions, often revealing structures, will be found. An example of distribution plot for ROSAT, ROR 701246 is shown in Fig. 13. In order to enhance sides of the distributions a logarithmic probability density scale is used. The amplitudes used to construct the graph in Fig. 13 are normalized to the maximum value of yl(ti) for each l. It may be seen that for wavelet coefficient magnitudes between 0.02 and 0.16 the distribution is broadened, which is in agreement with the part of ampligram where deterministic structures may be seen.
A useful method to quantify the above observation is to calculate the
distribution entropy for each level of wavelet coefficient magnitude.
The distribution entropy, El, is calculated as:
The distribution entropy will be used in the present study as a measure of occurrence of deterministic structures.
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