Dynamics of the solar granulation - VII. A nonlinear approach

We investigate the attractor underlying the granular phenomenon by applying nonlinear methods to series of spectrograms from 1994 and 1999. In the thr ee-dimensional phase space spanned by intensity, Doppler velocity, and turb ulence (line broadening), the granulation attractor does not fill the entir e phase space, as expected from the high Reynolds and Rayleigh numbers of t he photospheric plasma, but rather shows a highly structured form. This cou ld be due to the correlations between intensity, turbulence, and velocity, which represent also the Reynolds stress. To obtain insight into the dimens ionality of the attractor, we use the time lag method, a nonlinear method t hat enables us to get information about the underlying attractor of a dynam ical system (granulation) from the measurement of one physical quantity onl y. By applying this method to the observed Doppler velocities, we show that the granulation attractor can be described by three independent variables. The dimension of the granulation attractor seems to be independent of the appearance of big granules and shear ow. Furthermore, the power analysis of the Doppler velocity shows power down to the spatial resolution of the ins trument (0.3 arcsec). In order to decide whether the power at the smallest scales is real or noise, we use again the time lag method in combination wi th either a high pass digital or wavelet filter, which filters out the larg e wave numbers. It appears that the power at the smallest scales represents a real signal.