首页> 外文期刊>Journal of marine systems: journal of the European Association of Marine Sciences and Techniques >High resolution observations of the Terra Nova Bay polynya using COSMO-SkyMed X-SAR and other satellite imagery
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High resolution observations of the Terra Nova Bay polynya using COSMO-SkyMed X-SAR and other satellite imagery

机译:使用COSMO-SkyMed X-SAR和其他卫星图像对Terra Nova Bay polynya的高分辨率观测

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摘要

In this study we analysed a combination of high and coarse resolution X-band COSMO-SkyMed Synthetic Aperture Radar (SAR) scenes collected during two periods in July and September 2011 over the Terra Nova Bay (Antarctica). High resolution (5m per pixel) and lower resolution SAR (100m) acquired over intervals of the order of minutes provided both, fine details and a full large-scale view of the polynya. The analysis was supported by several Ice Surface Temperature (IST) maps per day obtained from the thermal band of Moderate Resolution Imaging Spectroradiometer (MODIS) and some additional C-band Envisat Advanced SAR (ASAR) scenes available during the July period. The dataset revealed two major openings around 2000km~2 occurred in the July period and one opening around 2500km~2 in the September period. The SAR analysis revealed that the polynya area is clearly distinguished from the sea ice pack offshore during the growing and closing phase. During the opening phase, the open polynya area was characterized by newly formed frazil ice organized as ice streaks parallel to the wind direction and separated by a distance of between 300 and 800m. Waves of length between 30 and 70m were noted on the streaks of frazil ice and on the frazil and grease ice accumulated at the polynya border. The early stage of the growing phase was indicated by the uniform distance of the ice streaks near the border of the polynya, while convergence was an indication that the wind was slowing down and that the growing phase was at a late stage. The closing phase was characterized by the progressive freezing of the open polynya area from the downwind border toward the coast. The results of this analysis suggest that the detection of the polynya area from thermal infrared or microwave temperatures is more effective during the growing phase, when large areas of unfrozen water are present within the polynya, than during the closing phase when large areas of thin sea-ice prevail.
机译:在这项研究中,我们分析了2011年7月和2011年9月在南极Terra Nova湾两个时期收集的高分辨率和粗分辨率X波段COSMO-SkyMed合成孔径雷达(SAR)场景。在几分钟量级的时间间隔内获得高分辨率(每像素5m)和较低分辨率SAR(100m),既提供了细部细节,又提供了完整的多面体全景。这项分析得到了每天从中分辨率成像光谱仪(MODIS)的热带获得的几张冰面温度(IST)图和7月期间可用的一些其他C波段Envisat Advanced SAR(ASAR)场景的支持。数据集显示,在7月期间发生了约2000km〜2的两个主要空洞,在9月期间发生了约2500km〜2的一个空洞。 SAR分析显示,在生长期和封闭期,波利尼亚地区与海上的冰袋区分开来。在开放阶段,开放的多年生植物区域的特征是新形成的巴西冰,其组织为与风向平行且相距300至800m的冰条纹。在f冰的条纹上以及在polynya边界积累的f冰和油脂冰上注意到了长度在30至70m之间的波浪。冰期附近的冰纹距离均匀,表明了生长期的早期,而会聚则表明风在减缓,生长期处于后期。封闭期的特征是开放的多年生植物区域从顺风边界向海岸逐渐冻结。该分析的结果表明,在生长阶段,当polynya中存在大面积的未冻结水时,从热红外或微波温度中检测出polynya区域要比在大面积稀薄海域中的封闭阶段更有效。 -冰为准。

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