墨西哥奇瓦瓦州北部萨马拉尤卡沙丘的形态测量学

Miguel Domínguez Acosta, Richard P. Langford, Thomas E. Gill
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摘要

墨西哥奇瓦瓦州的萨马拉尤卡沙丘(Samalayuca Dunes)(Médanos de Samalayuca)是墨西哥最大的沙丘地之一,也是研究最少的沙丘地之一。我们基于遥感和实地研究,对沙丘地的形态特征进行了分析,以加深对其物理环境的了解。SMD 的沙粒一般较细,源自帕洛马斯古湖的海岸线沉积物,沿风化走廊向东(下风向)迁移,主要在萨马拉尤卡和普雷西迪奥山脉的上风向堆积成回音沙丘。北风和南风与区域内盛行的西南风相辅相成,形成了复杂的风系,并受到地形的影响,塑造了 SMD 的形态。沙海面积约为 139.7 平方公里,其中约 113.8 平方公里位于东部主体,约 25.9 平方公里位于西北部分区。我们描述了六种主要沙丘形态:南北向直顶沙丘、东西向直顶沙丘、星形沙丘、植被抛物线沙丘、残留横向沙丘和 "巨星"(德拉)沙丘。沙丘中心点之间的平均间距为 76.5 米。活动沙丘以前曾被描述为 "aklé "模式,主要是近乎垂直的直顶沙丘,大致呈南北和东西走向,高 4-5 米,南北走向的沙丘顶间距约为 67 米,东西走向的沙丘顶间距约为 53 米,在某些位置呈现近乎垂直的干扰模式。活动沙丘叠加在更大的北北西向横向沙丘脊的残余物上,形成复杂的复合排列,沙丘脊由南向北呈扇形延伸,间距约为 1 公里,高约 50 米。最东边的沙丘脊包含一组活跃的沙丘,至少有 15 个活跃的巨型沙丘和反转沙丘,高达 120 米,沙丘的大小和复杂程度由南向北递增。作为一个具有历史和生态价值的保护区,应在 SMD 进行更多的地质调查,以帮助保护这一显著的地质特征。
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Morphometry of the Samalayuca dunes, northern Chihuahua, Mexico
The Samalayuca Dunes (SMD) (Médanos de Samalayuca), Chihuahua, México, are one of México’s largest and least studied dune fields, now managed as a Protected Area for their ecological characteristics. We present a morphometric characterization of the dune field based on remote sensing and field studies, to advance understanding of its physical environment. SMD’s generally-fine sands originate from shoreline deposits of Paleolake Palomas, transported eastward (downwind) along an aeolian corridor, accumulating primarily as echo dunes upwind of the sierras of Samalayuca and Presidio. A complex wind regime, with northerly and southerly winds complementing regionally-prevailing southwesterlies, modified by topographic effects, shapes the SMD’s morphology. The sand sea covers ~139.7 km2, with ~113.8 km2 in the main eastern body and ~25.9 km2 in a northwestern subfield. We describe six major dune forms: north to south straight-crested dunes, east to west straight-crested dunes, star dunes, vegetated parabolic dunes, relict transverse dunes, and “megastar” (draa) dunes. Mean interdune centroid spacing is 76.5 m. The active dunes, previously described as an “aklé” pattern, are predominantly straight-crested dune sets oriented near-perpendicular to each other with general north-south and east-west crest orientations, 4-5 m high, spaced ~67 m apart for north-south trending crests and ~53 m for east-west trending crests, representing a nearly perpendicular interference pattern in some locations. The active dunes are superimposed in a compound and complex arrangement on relict remnants of much larger north-northwest trending transverse dune ridges fanning out from south to north-northwest, spaced approximately ~1 km apart and ~50 m high. The easternmost dune ridge contains an active set of at least 15 active megastar and reversing dunes up to 120 m tall, increasing in size and complexity from south to north. As a protected area with historical and ecological value, additional geologic investigations should be performed at the SMD, to help conserve this remarkable geologic feature.
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