Multiple evolution modes of Aeolian Megaripples and implications for mars
编号:2411 访问权限:私有 更新:2023-04-11 19:12:31 浏览:163次 口头报告

报告开始:2023年05月06日 15:20(Asia/Shanghai)

报告时间:15min

所在会场:[12] 12、地表过程与地貌 [12-1] 12-1 地表过程与地貌

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摘要
The megaripples formed under the condition of multi-modal grain size distribution are considered to be intermediate-scale landforms between normal ripples and dunes. Field investigation shows that the megaripples in the Qaidam Basin are diverse in scale and shape, and a single mechanism seems to be unable to explain their formation. We propose that the formation of megaripples follows three evolution modes, presenting three states: transient, steady, and unstable. Transient megaripples are characterized by small scale, a small range of grain size and a short evolution cycle, which are the result of coarse grains gathering to the crest due to sand sorting; Steady megaripples are characterized by large scale, a wide range of grain size, stratified sedimentary structure and a long evolution cycle. The bimodal sand transport mechanism of the creeping of coarse particles caused by the impact of jumping fine particles shapes the surface armouring and stratified sediment; The scale and grain size range of the unstable megaripple is between the two. The strong wind causes the coarse particles to undergo a brief saltation movement, forming a small-scale secondary ripple. To test this hypothesis, we investigated their wind regime, morphology, grain size, sedimentary structure, and age. We find that the retardation effect of coarse particles relative to fine particles controls the erosion and deposition of megaripples and affects their scale and sedimentary structure. This will help us understand the coexistence of different scale ripples and Transverse Aeolian Ridges on Mars.The megaripples formed under the condition of multi-modal grain size distribution are considered to be intermediate-scale landforms between normal ripples and dunes. Field investigation shows that the megaripples in the Qaidam Basin are diverse in scale and shape, and a single mechanism seems to be unable to explain their formation. We propose that the formation of megaripples follows three evolution modes, presenting three states: transient, steady, and unstable. Transient megaripples are characterized by small scale, a small range of grain size and a short evolution cycle, which are the result of coarse grains gathering to the crest due to sand sorting; Steady megaripples are characterized by large scale, a wide range of grain size, stratified sedimentary structure and a long evolution cycle. The bimodal sand transport mechanism of the creeping of coarse particles caused by the impact of jumping fine particles shapes the surface armouring and stratified sediment; The scale and grain size range of the unstable megaripple is between the two. The strong wind causes the coarse particles to undergo a brief saltation movement, forming a small-scale secondary ripple. To test this hypothesis, we investigated their wind regime, morphology, grain size, sedimentary structure, and age. We find that the retardation effect of coarse particles relative to fine particles controls the erosion and deposition of megaripples and affects their scale and sedimentary structure. This will help us understand the coexistence of different scale ripples and Transverse Aeolian Ridges on Mars.
关键词
Megaripple, Aeolian processes, Qaidam Basin, Mars
报告人
李超
陕西师范大学

稿件作者
李超 陕西师范大学
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重要日期
  • 会议日期

    05月05日

    2023

    05月08日

    2023

  • 03月31日 2023

    初稿截稿日期

  • 05月25日 2023

    注册截止日期

主办单位
青年地学论坛理事会
中国科学院青年创新促进会地学分会
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武汉大学
中国科学院精密测量科学与技术创新研究院
中国地质大学(武汉)
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