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First in‐situ analysis of dust devil tracks on Earth and their comparison with tracks on Mars
Author(s) -
Reiss D.,
Raack J.,
Rossi A. P.,
Di Achille G.,
Hiesinger H.
Publication year - 2010
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2010gl044016
Subject(s) - mars exploration program , albedo (alchemy) , geology , astrobiology , earth (classical element) , atmospheric sciences , physics , astronomy , art , performance art , art history
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 (< ∼63 μ 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 ∼2 μ 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.