2021
DOI: 10.1016/j.geomorph.2020.107481
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New type of sand wedge polygons in the salt cemented soils of the hyper-arid Atacama Desert

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Cited by 13 publications
(20 citation statements)
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“…Temperatures as high as that have been recorded in 10 cm depth close to our study site, after a rain experiment when the soil moisture still reached 100%, indicating the presence of liquid water (Sager et al, 2021). Considering that these temperatures can be reached at shallow depth and that rainwater can dampen the soil at 10-30 cm depth for months (Schulze-Makuch et al, 2018;Sager et al, 2021;Jordan et al, 2020), we assume that the formation of anhydrite in the chusca horizon can occur through precipitation out of solarheated water after a rain event with retention time of several months. At depths below 50 cm the temperatures remain too low for this process to occur.…”
Section: Gypsum Vs Anhydritesupporting
confidence: 53%
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“…Temperatures as high as that have been recorded in 10 cm depth close to our study site, after a rain experiment when the soil moisture still reached 100%, indicating the presence of liquid water (Sager et al, 2021). Considering that these temperatures can be reached at shallow depth and that rainwater can dampen the soil at 10-30 cm depth for months (Schulze-Makuch et al, 2018;Sager et al, 2021;Jordan et al, 2020), we assume that the formation of anhydrite in the chusca horizon can occur through precipitation out of solarheated water after a rain event with retention time of several months. At depths below 50 cm the temperatures remain too low for this process to occur.…”
Section: Gypsum Vs Anhydritesupporting
confidence: 53%
“…The porous and permeable chusca horizon is most frequently exposed to meteoric water and therefore is the most dynamic horizon, which could explain why measured isotopic fractionation is stronger than seen in the modeled data. This upper soil horizon is also affected by salt efflorescence after rain events and through artificial rain experiments (Sager et al, 2021, Pfeiffer et al, 2021, which indicates more complex water pathways at the surface than dominant downward migration, influencing potentially also the isotopic fractionation. Furthermore, rainwater infiltration is not homogeneous and is most intense along the sand wedges (Owen et al, 2013), presumably affecting the lateral isotope pattern.…”
Section: Water-soil Interactionsmentioning
confidence: 99%
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“…PNs occurring on these soils in the Atacama Desert (Fig. 1 ) exhibit ~ 1 m deep and salt-poor sand wedges outlining salt-rich polygons of a uniform flat-center morphology 25 . They exhibit an orthogonal to hexagonal pattern geometry, and elongated polygons have either one or two dominant orientations, preferably parallel or perpendicular to the slope.…”
Section: Introductionmentioning
confidence: 97%
“…However, the details on the formation of PNs remain under debate, such as the driving forces behind the crack formation. The proposed processes range from thermal contraction, where cementation by salts results in cohesive soils and makes them susceptible to thermal stress 25 and/or salt dehydration 12 , 14 , both being cyclic processes. The details on the importance of rain events for PN formation remain unclear, although, its involvement is certain as rainwater infiltration, which is insufficient to fully wash out the salts, creates the vertical salt sequence of these indurated soils 12 , 22 .…”
Section: Introductionmentioning
confidence: 99%