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Ocean-generated magnetic field study based on satellite geomagnetic measurements: 2. Signal inference

机译:基于卫星地磁测量的海洋磁场研究:2.信号推断

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The work presented here is the second part of an ocean-generated magnetic field study and provides a procedure for inferring the ocean-generated magnetic field from satellite geomagnetic measurements. The procedure was first tested on synthetic data. The simulation employed a hypothetical satellite measuring the magnetic field at an altitude of 400km. The "measurements" (generated by the CM4 and CHAOS models) included the core field, the lithospheric field, the ionospheric and magnetospheric fields, the secular variation, and the ocean-generated magnetic field. The search algorithm, as proposed in part 1, converts irregular measurements into fields on a regular grid. The filtration procedure is based on the Savitzky-Golay algorithm. The procedure includes four steps providing seven unknown filter parameters. Parameter values were obtained by solving the problem of minimizing the spatially averaged squared residuals between the inferred field and the model field. Then, the parameters were used in the filter to infer the ocean-generated magnetic field that was initially added to the "measurements." The inferred signal, although spatially corrupted and having a smaller magnitude (60% of the magnitude of the initial signal), indicated the presence of magnetic anomalies within the Southern Ocean. The technique was then applied to CHAMP geomagnetic measurements. The result of filtering was clear magnetic anomalies within the Southern Ocean with a spatial character that were close to what models of the ocean-generated magnetic field provided. The magnitude of the inferring signal was 5 nT, the corrected values were 7-8 nT, 1-2 nT larger than the modeled field magnitude. To compare the temporal variability of the inferred field with the variability of sea surface height, ten 10° by 10° areas were selected within the Southern Ocean and the root-mean-square of both SSH and the magnetic field were computed for each area. A comparison of the results indicated a close similarity between SSH and the magnetic field temporal variability, which allowed the identification of the inferred field as the ocean-generated magnetic field.
机译:本文介绍的工作是海洋磁场研究的第二部分,并提供了一种从卫星地磁测量推论海洋磁场的程序。该程序首先在综合数据上进行了测试。该模拟使用了一个假设卫星,该卫星在400 km的高度测量磁场。 “测量”(由CM4和CHAOS模型生成)包括核心场,岩石圈场,电离层和磁层场,长期变化以及海洋产生的磁场。如第1部分所述,搜索算法将不规则的测量值转换为规则网格上的字段。过滤过程基于Savitzky-Golay算法。该过程包括四个步骤,提供七个未知的过滤器参数。通过解决最小化推断字段和模型字段之间的空间平均平方残差的问题来获得参数值。然后,在滤波器中使用这些参数来推断最初添加到“测量”中的海洋磁场。推断的信号尽管在空间上受到破坏并且幅度较小(占初始信号幅度的60%),但它表明南大洋内部存在磁异常。然后将该技术应用于CHAMP地磁测量。过滤的结果是南大洋内部明显的磁异常,其空间特征与海洋产生的磁场所提供的模型接近。推断信号的大小为5 nT,校正后的值为7-8 nT,比建模的场大小大1-2 nT。为了比较推断场的时间变化性与海面高度的变化性,在南大洋中选择了10个10°乘10°的区域,并计算了每个区域的SSH和磁场的均方根。结果的比较表明SSH与磁场的时间变异性非常相似,从而可以将推断出的磁场识别为海洋产生的磁场。

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