More interesting perhaps is the discovery that visual search RTs, when considered as a time series, have a 1/
f power spectrum (Farrell, Wagenmakers, & Ratcliff,
2006; Gilden,
2001; Gilden, Thornton, & Mallon,
1995). The power spectrum of a time series is calculated by treating the sequence of RTs as an evenly spaced set of signal values, and taking the Fourier transform of them. A 1/
f power spectrum has power at frequency f proportional to 1/
f. The finding of a 1/
f spectrum is interesting for two reasons. First, 1/
f power spectra are found in many diverse phenomena, such as the fluctuation of light intensity from quasars, current noise in resistors, semiconductors, and thermionic tubes, sea level fluctuations, music, intervals between heartbeats, and errors in time interval estimation, among others (Dutta & Horn,
1981; Milotti,
2002; Press,
1978; Voss & Clarke,
1975). The widespread occurrence of 1/
f power spectra, and power spectra close to 1/
f, suggests that there may be a universal mechanism behind all these phenomena. The second reason 1/
f spectra are interesting is because, despite many attempts, no one has so far convincingly put forward any such universal mechanism.