Ring of attraction: overlapping directions of the dipole modulation of
  the CMB, the parity asymmetry, and kinematic dipole percolation zone
  The largest anisotropy in the cosmic microwave background (CMB) is the 3 mK
kinematic dipole reflecting our motion with respect to the CMB frame and
pointed in the direction $(l, b) = (264^\circ, +48^\circ)$ in Galactic
coordinates. We introduce the concept of the ring of attraction (RA), which is
orthogonal to the axis of the kinematic dipole. These directions overlap with
the zone of percolation for the kinematic dipole, where its amplitude almost
vanishes. We show that along this ring are oriented the directions of the
dipole modulation of the CMB, and positions of the peaks responsible for
generation of parity asymmetry. This coincidence is peculiar at around the 3
sigma level. We analyzed the "interaction" of low multipoles of the CMB with RA
and showed that for odd modes there is a sequence of peaks in the RA direction.
These peaks correlate with each other for different multipoles and result in
mutual amplification of the odd $\ell$ signal for the first 30 multipoles. Our
method sheds new light on the nature of parity asymmetry. It consists of the
deficit of symmetrically located and equal in amplitude peaks in the CMB map in
comparison with asymmetric peaks.
