We investigate the interlayer magnetoresistance (MR) along the chiral crystallographic axis in the hexagonal chiral magnet CrNb 3 S 6 . In a region below the incommensurate-commensurate phase transition between the chiral soliton lattice and the forced ferromagnetic state, a negative MR is obtained in a wide range of temperature, while a small positive MR is found very close to the Curie temperature. Normalized data of the negative MR almost falls into a single curve and is well fitted by a theoretical equation of the soliton density, meaning that the origin of the MR is ascribed to the magnetic scattering of conduction electrons by a nonlinear, periodic, and countable array of magnetic soliton kinks. , belong to chiral space groups and are frequently referred to as chiral magnets. In chiral magnets, the combined effect of the symmetric Heisenberg exchange and the antisymmetric Dzyaloshinskii-Moriya (DM) interactions caused by the relativistic spin-orbit interaction [5,6] gives rise to a nontrivial spin texture and various interesting functions unique to chiral magnets. A coupling of conduction electrons with nontrivial spin textures has recently attracted great attention because of the ability to manipulate magnetotransport properties such as the topological Hall effect [7]. One promising candidate to realize this coupling is the chiral soliton lattice (CSL), which is formed in a chiral magnet under magnetic fields perpendicular to the chiral axis. The CSL is a nonlinear array of magnetic soliton kinks. It is naturally expected that each magnetic soliton kink works as a strong scattering potential for itinerant spins. Therefore, decreasing the number of magnetic soliton kinks may reduce the magnetoresistance (MR) and thus the CSL will present a nontrivial MR.In this Letter, we report the MR along the chiral axis in a hexagonal chiral magnetic crystal of CrNb 3 S 6 . We find that the normalized data of the negative MR almost falls into a single curve, and the revealed behavior indicates that the origin of the MR can be attributed to the magnetic scattering of conduction electrons by a nonlinear, periodic, and countable array of magnetic soliton kinks. Namely, we clarify the direct correlation between the experimentally measured MR and the analytically obtained soliton density as a function of the magnetic field.CrNb 3 S 6 is a typical monoaxial chiral magnet, which belongs to the space group of P6 3 22 [8]. It has a layered hexagonal structure of 2H-type NbS 2 intercalated by Cr atoms, so often expressed as Cr 1=3 NbS 2 . The size of the unit cell is 0.57 nm in the ab plane and 1.21 nm along the c axis [9,10]. Cr atoms are in the trivalent state and have localized electrons with spins of S ¼ 3=2, whereas conduction electrons are in an unfilled hybridized band of Nb and S. As a consequence of the chiral space group, the monoaxial DM interaction is allowed along the chiral c axis in CrNb 3 S 6 , which is given in the form of ÀD Á S 1 Â S 2 between localized neighboring spins S 1 and S 2 at Cr atoms. Here, D repres...