{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,2,5]],"date-time":"2026-02-05T11:07:16Z","timestamp":1770289636326,"version":"3.49.0"},"reference-count":33,"publisher":"American Geophysical Union (AGU)","issue":"16","license":[{"start":{"date-parts":[[2016,8,30]],"date-time":"2016-08-30T00:00:00Z","timestamp":1472515200000},"content-version":"vor","delay-in-days":2,"URL":"http:\/\/onlinelibrary.wiley.com\/termsAndConditions#vor"}],"funder":[{"name":"FCT","award":["FRH\/BPD\/72371\/2010"],"award-info":[{"award-number":["FRH\/BPD\/72371\/2010"]}]},{"name":"FCT","award":["UID\/Multi\/00611\/2013"],"award-info":[{"award-number":["UID\/Multi\/00611\/2013"]}]},{"name":"FCT","award":["COMPETE2020\/POCI-01-0145-FEDER-006922"],"award-info":[{"award-number":["COMPETE2020\/POCI-01-0145-FEDER-006922"]}]}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Geophysical Research Letters"],"published-print":{"date-parts":[[2016,8,28]]},"abstract":"<jats:title>Abstract<\/jats:title><jats:p>Martian dunes are sculpted by meter\u2010scale bed forms, which have been interpreted as wind ripples based on orbital data. Because aeolian ripples tend to orient and migrate transversely to the last sand\u2010moving wind, they have been widely used as wind vanes on Earth and Mars. In this report we show that Martian large ripples are dynamically different from Earth's ripples. By remotely monitoring their evolution within the Mars Science Laboratory landing site, we show that these bed forms evolve longitudinally with minimal lateral migration in a time\u2010span of\u2009~\u2009six terrestrial years. Our observations suggest that the large Martian ripples can record more than one wind direction and that in certain cases they are more similar to linear dunes from a dynamic point of view. Consequently, the assumption of the transverse nature of the large Martian ripples must be used with caution when using these features to derive wind directions.<\/jats:p>","DOI":"10.1002\/2016gl070014","type":"journal-article","created":{"date-parts":[[2016,8,9]],"date-time":"2016-08-09T21:42:40Z","timestamp":1470778960000},"page":"8384-8389","source":"Crossref","is-referenced-by-count":60,"title":["Dune\u2010like dynamic of Martian Aeolian large ripples"],"prefix":"10.1029","volume":"43","author":[{"given":"S.","family":"Silvestro","sequence":"first","affiliation":[{"name":"INAF Osservatorio Astronomico di Capodimonte  Naples Italy"},{"name":"SETI Institute, Carl Sagan Center  Mountain View California USA"}]},{"given":"D. A.","family":"Vaz","sequence":"additional","affiliation":[{"name":"CITEUC Centre for Earth and Space Research of the University of Coimbra, Observat\u00f3rio Geof\u00edsico e Astron\u00f3mico da UC  Santa Clara Portugal"},{"name":"CERENA Center for Natural Resources and the Environment Instituto Superior T\u00e9cnico  Lisbon Portugal"}]},{"given":"H.","family":"Yizhaq","sequence":"additional","affiliation":[{"name":"Department of Solar Energy and Environmental Physics Ben\u2010Gurion University of the Negev  Israel"}]},{"given":"F.","family":"Esposito","sequence":"additional","affiliation":[{"name":"INAF Osservatorio Astronomico di Capodimonte  Naples Italy"}]}],"member":"13","published-online":{"date-parts":[[2016,8,30]]},"reference":[{"key":"e_1_2_5_2_1","volume-title":"Current Ripples: Their Relation to Patterns of Water and Sediment Motion","author":"Allen J. R. 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