Determination of the Earths Magnetic Field Gradients from SatellitesMeasurements and Their Inversion over the Kursk Magnetic Anomaly

K. Kis, P. Taylor, G. Wittmann
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Abstract

We computed magnetic field gradients at satellite altitude, over Europe with emphasis on the Kursk Magnetic Anomaly (KMA). They were calculated using the CHAMP satellite total magnetic anomalies. Our computations were done to determine how the magnetic field observations data from the new ESA/Swarm satellites could be utilized to determine the structure of the magnetization of the Earth’s crust, especially in the region of the KMA. Ten years of CHAMP data were used to simulate the Swarm data. An initial east magnetic anomaly gradient map of Europe was computed and subsequently the North, East and Vertical magnetic gradients for the KMA region were calculated. The vertical gradient of the KMA was also determined using Hilbert transforms. Inversion of the total KMA was derived using Simplex and Simulated Annealing algorithms. The depths of the upper and lower boundaries are calculated downward from the 324 km elevation of the satellite. Our resulting inversion depth model is a horizontal quadrangle. The maximum errors are determined by the model parameter errors.
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卫星测量地球磁场梯度的测定及其在库尔斯克磁异常上的反演
我们计算了欧洲上空卫星高度的磁场梯度,重点是库尔斯克磁异常(KMA)。它们是用CHAMP卫星的总磁异常计算出来的。我们的计算是为了确定如何利用新的ESA/Swarm卫星的磁场观测数据来确定地壳的磁化结构,特别是在KMA区域。10年的CHAMP数据被用来模拟Swarm数据。首先计算了欧洲东部的初始磁异常梯度图,然后计算了KMA地区的北、东和垂直磁异常梯度。利用希尔伯特变换确定了KMA的垂直梯度。利用单纯形和模拟退火算法推导了总KMA的反演。上下边界的深度是从卫星324公里高度向下计算的。我们得到的反演深度模型是一个水平四边形。最大误差由模型参数误差决定。
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