  We analyzed TESS photometric data of the flickering-active cataclysmic star
AQ Men in 2018--2019. We processed 7 sectors with 14 light curves (LCs) inside
them, with a time resolution of 2 min. Aiming to study the "macro-flickering",
with quasi periods (QPs) between 10 and 100 hours, we processed LCs after 55
time reduced, with a time resolution of 1.83 hours. The method, developed
earlier by us, includes comparing the LCs by their statistical and fractal
parameters, as well as revealing QPs by minima of structure functions and
relevant maxima of autocorrelation functions.
  We distinguish the known high state of AQ Men, in the sectors ## 01, 05, 08,
12, 13, as well as the low state, in sectors #19, #20. In the low state the LCs
show noticeable eclipses with period 3.4 h, lower average fluxes, higher
scatters, and additional QPs. By its statistical and fractal parameters, the
macro-flickering of AQ Men in the high state is similar to the ordinary
flickering of 3 symbiotic binaries, studied by us earlier (see below).
  We found 92 QPs in the range of 20--70 h. We reveal 3 QP modes, at 20.9 h,
32.5 h and 54.1 h (1.149, 0.738 and 0.434 c/d; Fig. 7) within a standard error
about 10%. The last mode is the most populated one and seems to be a
manifestation of the superorbital period. Other 4 QP modes of AQ Men are added
from the literature. The regularity of these 7 QP modes follows a power
function with a base 1.57 and standard deviation 6.4% (Fig. 8). This power
model prognosticates 5 other QP modes: 3 internal and 2 external (Table 2). The
bases of the power regularity models for the flickering of the symbiotic
binaries RS Oph, T CrB, and MWC 560 (however in the time scale of minutes) are
1.55, 2.0, and 1.34, respectively (Table 1). For unknown reasons in these 4
cases we find (i) regularities with (ii) different bases.
