“…To avoid these problems, we have visualized the spatial distribution of the ILMs, using SnXRD from the bulk to the atomically thin limit. In the previous X-ray diffraction (XRD) study of BSCCO 6,8,[13][14][15] , the 1D ILM has been reported to have both diffuse Short-range order (SRO) satellites at 𝒒 s = (0,0.21,2𝑛) and Long-range order (LRO) satellites at 𝒒 𝐿 = (0,0.21,2𝑛 + 1) (where 𝒒 𝑠 and 𝒒 𝐿 are the reciprocal lattice units (r.l.u.) and n is an integer number) around Bragg peaks.…”