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High-resolution digital elevation model from tri-stereo Pleiades-1 satellite imagery for lava flow volume estimates at Fogo Volcano

机译:来自三立体声Pleiades-1卫星影像的高分辨率数字高程模型,用于估算Fogo火山的熔岩流量

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摘要

Resolving changes in topography through time using accurate high-resolution digital elevation models (DEMs) is key to understanding active volcanic processes. For the first time in a volcanic environment, we utilize very high-resolution tri-stereo optical imagery acquired by the Pleiades-1 satellite constellation and generate a 1mresolution DEM of Fogo Volcano, Cape Verde-the most active volcano in the Eastern Atlantic region. Point cloud density is increased by a factor of 6.5 compared to conventional stereo imagery, and the number of 1m(2) pixels with no height measurements is reduced by 43%. We use the DEM to quantify topographic changes associated with the 2014-2015 eruption at Fogo. Height differences between the posteruptive Pleiades-1 DEM and the preeruptive topography from TanDEM-X give a lava flow volume of 45.83 +/- 0.02 x 10(6)m(3), emplaced over an area of 4.8km(2) at a mean rate of 6.8m(3) s(-1).
机译:使用精确的高分辨率数字高程模型(DEM)解决随时间变化的地形变化是了解活动火山过程的关键。首次在火山环境中,我们利用由Pleiades-1卫星星座获取的超高分辨率三立体光学图像,并生成了1m分辨率的佛得角佛戈火山DEM,这是东大西洋地区最活跃的火山。与传统的立体图像相比,点云密度增加了6.5倍,并且没有高度测量的1m(2)像素数量减少了43%。我们使用DEM量化与2014-2015年Fogo火山爆发相关的地形变化。后喷的Pleiades-1 DEM和弹前的地形之间的高度差使熔岩流体积为45.83 +/- 0.02 x 10(6)m(3),位于4.8 km(2)平均速率为6.8m(3)s(-1)。

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