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Short-lived and long-lived dust devil tracks in the coastal desert of southern Peru

机译:秘鲁南部沿海沙漠中的短寿命和长寿命尘埃魔鬼足迹

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摘要

In the coastal desert of southern Peru, sequential high-resolution satellite images document the presence of short-lived and long-lived dust devil tracks. Dust devil tracks in the study region remain visible for less than 6 months in one area and for more than 4 years in another area. Short-lived tracks are generally darker than the surrounding ground surface. The brightness of long-lived tracks is often equal to that of their surroundings; they become visible due to a brighter edge along their margins. Different modes of formation related to ground surface properties are suggested to explain the differences in persistence and appearance. Dark, short-lived dust devil tracks are ascribed to the removal of silt-sized material from largely sand-sized surface materials. Long-lived tracks with bright margins are ascribed to coarser surface materials and the fallout of sand-sized particles along the track edges. Locating suitable areas on Earth for the study of dust devil tracks and distinguishing between different types of dust devil tracks is expected to further promote terrestrial analogue studies for Martian dust devil streaks.
机译:在秘鲁南部的沿海沙漠中,连续的高分辨率卫星图像记录了短寿命和长寿命的尘埃魔鬼轨道的存在。在研究区域中,一个地方的尘埃魔鬼轨迹在不到6个月的时间内仍然可见,而在另一个地区则超过4年。短寿命的轨道通常比周围的地面暗。长寿命轨道的亮度通常等于周围环境的亮度;由于边缘的边缘变亮,它们变得可见。建议使用与地面特性有关的不同形成方式来解释持久性和外观的差异。黑暗,寿命短的尘埃魔鬼轨道归因于从较大的沙粒大小的表面材料中清除了淤泥大小的材料。边缘较长的长寿命轨道归因于较粗糙的表面材料以及沿着轨道边缘的沙粒状颗粒的沉降。期望在地球上找到适合研究尘埃魔鬼轨道的区域并区分不同类型的尘埃魔鬼轨道,有望进一步促进火星尘埃魔鬼条纹的地面模拟研究。

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