磁地图和备选导航模型

R. Saltus, P. Alken, Annette Balmes, N. Boneh, S. Califf, A. Chulliat, B. Meyer, M. Nair
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引用次数: 0

摘要

磁导航需要将机载磁传感器测量值与磁地图和磁模型进行比较。磁图和磁模型可用于各种比例尺和范围。在任何给定地点,对环境磁场的测量是各种分量的总和,包括地球内部和外部的源。本文讨论了地核和岩石圈内部成分的图和模型。地球长波长、时变缓慢的地核场由全球卫星模型表示。定常岩石圈磁场的最长波长由基于CHAMP和SWARM卫星任务数据的球谐模型表示,分辨率小于~300 km的分辨率由基于航空、海洋和地面调查处理的网格产品表示。区域到局部磁异常图和网格可用于选定区域,分辨率低至100米。评估给定磁导航场景下可能的地图/模型性能需要考虑磁场变化的幅度和频率,以及磁地图/模型的不确定性。我们给出了磁导航信号作为高度和速度函数的基本分析。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Magnetic Maps and Models for Alternative Navigation
Magnetic navigation requires the comparison of onboard magnetic sensor measurements to reference magnetic maps and models. Magnetic maps and models are available at a wide range of scales and scope. At any given location, measurements of the ambient magnetic field are the sum of various components, including sources internal and external to the Earth. This paper discusses maps and models of the internal components sourced in the core and lithosphere of the Earth. The long-wavelength, slowly-time-varying core field of the Earth is represented by global, satellite-based models. The time-invariant lithospheric magnetic field is represented at its longest wavelengths by spherical harmonic models based on data from the CHAMP and SWARM satellite missions and at resolutions smaller than ~300 km by grid products based on the processing of airborne, marine, and ground surveys. Regional to local magnetic anomaly maps and grids are available for selected areas at resolutions down to 100 m. Evaluation of possible map/model performance for a given magnetic navigation scenario requires consideration of amplitude and frequency of magnetic field variations, and magnetic map/model uncertainty. We present a basic analysis of magnetic navigation signals as a function of altitude and velocity.
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