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In this study we report about the first in-situ analysis of terrestrial dust devil tracks (DDTs) observed in the Turpan depression desert in northwestern China. Passages of active dust devils remove a thin layer of fine grained material (< similar to 63 mu m), cleaning the upper surface of coarse sands (0.5-1 mm). This erosional process changes the photometric properties of the upper surface causing the albedo differences within the track to the surroundings. Measurements imply that a removal of an equivalent layer thickness of similar to 2 mu m is sufficient to form the dark dust devil tracks. Our terrestrial results are in agreement with the mechanism proposed by Greeley et al. (2005) for the formation of DDTs on Mars. Citation: Reiss, D., J. Raack, A. P. Rossi, G. Di Achille, and H. Hiesinger (2010), First in-situ analysis of dust devil tracks on Earth and their comparison with tracks on Mars, Geophys. Res. Lett., 37, L14203, doi:10.1029/2010GL044016.