“…The two characteristic length scales of the SAW, namely its wavelength L and its amplitude H 1 can be extracted from time From the number of observable diraction satellites, the SAW amplitude can be determined [117,118]. c) Relative changes in peak intensity (stars, black), integrated peak intensity (squares, red), and full width at half maximum (FWHM, circles, blue) of the rocking curves shown in (a), as a function of phase φ.…”