Summary of the filtered RHESSI flare list showing a histogram of the latitudes per Cycle (left panel), frequency distribution of the flare GOES 1–8 Å flux (middle panel) and number of flares and sunspots versus time (right panel). Note that the power-law fitted to the frequency distribution (red line, middle panel) was found using a Maximum Likelihood Estimator method (Crawford et al. 1970; Wheatland 2004), over the range indicated by the dashed vertical lines, and is not a direct fit to the histogram. The times during which RHESSI was not pointing at the Sun or the detectors were off is indicated by the red bars (right panels).