dot
Detailansicht
Katalogkarte GBA
Katalogkarte ISBD
Suche präzisieren
Drucken
Download RIS
Hier klicken, um den Treffer aus der Auswahl zu entfernen
Titel Basin-wide sediment interactions between channels, floodplains and dunes in a large, dryland river system, central Australia
VerfasserIn Sarah Eccleshall, John Jansen, Toshiyuki Fujioka, Alexandru Codilean, Charles Mifsud
Konferenz EGU General Assembly 2015
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 17 (2015)
Datensatznummer 250101808
Publikation (Nr.) Volltext-Dokument vorhandenEGU/EGU2015-1040.pdf
 
Zusammenfassung
Low, flat terrain (slope 400 kyr) implied in the ‘storage’ hypothesis. The 26Al/10Be ratio has been used to identify a complex exposure history, such as one including burial, where a lower offset in 26Al/10Be ratio from the expected production-rate ratio of 6.8 can be converted to a burial age. Eleven detrital samples were collected along the full length of the Cooper, plus three surface samples from source-bordering dunes in the lowermost reach. We discuss our preliminary findings with regard to sediment burial and long-term interactions in the river-dune systems of central Australia. References: 1Willenbring, J. K., Codilean, A. T., Ferrier, K. L., McElroy, B., & Kirchner, J. W. (2014). Short Communication: Earth is (mostly) flat, but mountains dominate global denudation: apportionment of the continental mass flux over millennial time scales, revisited.ÂEarth Surface Dynamics Discussions,Â2(1), 1-17. 2Magee, J. W., Miller, G. H., Spooner, N. A., & Questiaux, D. (2004). Continuous 150 ky monsoon record from Lake Eyre, Australia: insolation-forcing implications and unexpected Holocene failure.ÂGeology,Â32(10), 885-888. 3Jansen, J. D., Nanson, G. C., Cohen, T. J., Fujioka, T., Fabel, D., Larsen, J. R., Codilean, A. T., Price, D.M, Bowman, H. H., May, J-H. & Gliganic, L. A. (2013). Lowland river responses to intraplate tectonism and climate forcing quantified with luminescence and cosmogenic 10Be.ÂEarth and Planetary Science Letters,Â366, 49-58.