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The largest anisotropy in the cosmic microwave background (CMB) is the 3 mKkinematic dipole reflecting our motion with respect to the CMB frame andpointed in the direction $(l, b) = (264^\circ, +48^\circ)$ in Galacticcoordinates. We introduce the concept of the ring of attraction (RA), which isorthogonal to the axis of the kinematic dipole. These directions overlap withthe zone of percolation for the kinematic dipole, where its amplitude almostvanishes. We show that along this ring are oriented the directions of thedipole modulation of the CMB, and positions of the peaks responsible forgeneration of parity asymmetry. This coincidence is peculiar at around the 3sigma level. We analyzed the "interaction" of low multipoles of the CMB with RAand 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 inmutual amplification of the odd $\ell$ signal for the first 30 multipoles. Ourmethod sheds new light on the nature of parity asymmetry. It consists of thedeficit of symmetrically located and equal in amplitude peaks in the CMB map incomparison with asymmetric peaks.

Ring of attraction: overlapping directions of the dipole modulation of the CMB, the parity asymmetry, and kinematic dipole percolation zone