Larsen-C A-68冰山监测用多频多极化合成孔径雷达

F. Nunziata, A. Buono, M. Migliaccio, M. Moctezuma, F. Parmiggiani, G. Aulicino
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引用次数: 3

摘要

自2016年以来,在东威德尔海(南极洲68°S, 61°W)经常观察到拉森- c冰架的断裂。这一过程导致了2017年7月的最终崩塌,当时约6000平方公里的面积(即约占整个冰架的9-12%)消失。在这项研究中,由此产生的冰山被称为“A-68”,来自美国国家冰中心,使用多频率和多极化合成孔径雷达(SAR)卫星平台进行观测,包括l波段Alos PaISAR-2, c波段sentinel - 1和x波段cosmos - skymed。我们考虑了在ScanSAR成像模式下收集的大约1年的大量SAR场景,以分析冰山的性质及其融化过程和漂移。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Multi-Frequency and Multi-Polarization Synthetic Aperture Radar for the Larsen-C A-68 Iceberg Monitoring
Since 2016 the fracture of the Larsen-C ice shelf has been regularly observed in the Eastern Weddell Sea (68°S, 61°W, Antarctica). This process led to the final collapse in July 2017, when an area of about 6000 km2 (i. e., about 9-12% of the whole shelf) was lost. In this study the resulting calved iceberg, termed as “A-68” from the U. S. National Ice Center, is observed using multi-frequency and multi-polarization Synthetic Aperture Radar (SAR) satellite platforms that include L-band Alos PaISAR-2, C-band Sentinel-l and X-band COSMO-SkyMed. A large set of SAR scenes were considered, collected in ScanSAR imaging modes over a time span of about 1 year, to analyze the iceberg properties and its melting process and drifting.
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