南极和格陵兰冰损对极地运动的影响:基于GRACE和多任务卫星测高的评估

F. Göttl, A. Groh, M. Kappelsberger, Undine Strößenreuther, L. Schröder, V. Helm, M. Schmidt, F. Seitz
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引用次数: 0

摘要

由于全球气候变化,南极和格陵兰冰盖(AIS, GrIS)的冰损失增加,影响了地球自转轴相对于地球固定参考系(极运动)的方向。由卫星雷达和激光高度计任务(如ENVISAT、CryoSat-2和ICESat)测量的地表高程变化,通过重力恢复和气候实验(GRACE)观测到南极洲和格陵兰岛的冰质量变化。除了有限的空间分辨率外,GRACE估算冰质量变化的精度还受到信号噪声(经向误差条纹)、泄漏效应和冰川均衡调整(GIA)模式的不确定性的限制,而卫星测高估算冰质量变化的精度则受到波形重跟踪、坡度相关的重新定位误差、在本研究中,我们使用不同的GRACE重力场模型(CSR RL06M, JPL RL06M, ITSG-Grace2018)和卫星测高数据(来自德累斯顿工业大学,利兹大学,阿尔弗雷德韦格纳研究所)来评估重力和测高导出的极运动激励函数的准确性。结果表明,由于单个解的组合,可以减少数据处理的系统和随机误差,并且可以增加大地测量导出的AIS和GrIS极运动激励函数的鲁棒性。基于这些研究,我们发现AIS质量的变化导致极点位置矢量沿60°在2003-2015年研究期间,东子午线的变化幅度为2 mas/年,而GrIS质量变化导致极矢量沿45°漂移;西经偏移3马/年。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The influence of Antarctic and Greenland ice loss on polar motion: an assessment based on GRACE and multi-mission satellite altimetry

Increasing ice loss of the Antarctic and Greenland Ice Sheets (AIS, GrIS) due to global climate change affects the orientation of the Earth’s spin axis with respect to an Earth-fixed reference system (polar motion). Ice mass changes in Antarctica and Greenland are observed by the Gravity Recovery and Climate Experiment (GRACE) in terms of time variable gravity field changes and derived from surface elevation changes measured by satellite radar and laser altimeter missions such as ENVISAT, CryoSat-2 and ICESat. Beside the limited spatial resolution, the accuracy of GRACE ice mass change estimates is limited by signal noise (meridional error stripes), leakage effects and uncertainties of the glacial isostatic adjustment (GIA) models, whereas the accuracy of satellite altimetry derived ice mass changes is limited by waveform retracking, slope related relocation errors, firn compaction and the density assumption used in the volume-to-mass conversion.

 

In this study we use different GRACE gravity field models (CSR RL06M, JPL RL06M, ITSG-Grace2018) and satellite altimetry data (from TU Dresden, University of Leeds, Alfred Wegener Institute) to assess the accuracy of the gravimetry and altimetry derived polar motion excitation functions. We show that due to the combination of individual solutions, systematic and random errors of the data processing can be reduced and the robustness of the geodetic derived AIS and GrIS polar motion excitation functions can be increased. Based on these investigations we found that AIS mass changes induce the pole position vector to drift along the 60° East meridian by 2 mas/yr during the study period 2003-2015, whereas GrIS mass changes cause the pole vector to drift along the 45° West meridian by 3 mas/yr.

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