Sand dune movement in the Victoria Valley, Antarctica

被引:60
作者
Bourke, Mary C. [1 ,2 ]
Ewing, Ryan C. [3 ]
Finnegan, David [4 ]
McGowan, Hamish A. [5 ]
机构
[1] Planetary Sci Inst, Tucson, AZ USA
[2] Univ Oxford, Sch Geog, OUCE, Oxford OX1 3QY, England
[3] Univ Texas Austin, Jackson Sch Geosci, Dept Geol Sci, Austin, TX 78712 USA
[4] USA, Cold Reg Res & Engn Lab, Hanover, NH 03755 USA
[5] Univ Queensland, Sch Geog Planning & Architecture, St Lucia, Qld 4072, Australia
关键词
Antarctica; Dune; Niveo-aeolian; Migration; BARCHAN DUNES; SPATIALLY DIVERSE; EOLIAN SEDIMENT; IMPERIAL-VALLEY; FIELD; TRANSPORT; WIND; DEPOSITS; COMPLEX; ORGANIZATION;
D O I
10.1016/j.geomorph.2009.02.028
中图分类号
P9 [自然地理学];
学科分类号
0705 ; 070501 ;
摘要
We use vertical aerial photographs and LiDAR topographic survey data to estimate dune migration rates in the Victoria Valley dunefield, Antarctica, between 1961 and 2001. Results confirm that the dunes migrated an average of 1.5 m/year. These values are consistent with other estimates of dune migration from cold climate deserts and are significantly lower than estimates from warm deserts. Dune migration rates are retarded by the presence of entrained ice, soil moisture and a reversing wind regime. Dune absorption, merging and limb extension are apparent from the time-series images and account for significant changes in dune form and the field-scale dune pattern. Dune-field pattern analysis shows an overall increase in dune-field organization with an increase in mean dune spacing and a reduction in total crest length and defect density. These data suggest that dunes in other cold desert environments on Earth, Mars or Titan, that may also have interbedded frozen laminae, still have the potential to migrate and organize, albeit at lower rates than dunes in warm deserts. (C) 2009 Elsevier B.V. All rights reserved.
引用
收藏
页码:148 / 160
页数:13
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