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Estimating external magnetic field differences at high geomagnetic latitudes from a single station

机译:估算单个站点在高地磁纬度上的外部磁场差异

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Providing an accurate estimate of the magnetic field on the Earth's surface at a location distant from an observatory has useful scientific and commercial applications, such as in repeat station data reduction, space weather nowcasting or aeromagnetic surveying. While the correlation of measurements between nearby magnetic observatories at low and mid-latitudes is good, at high geomagnetic latitudes (58-75 degrees) the external field differences between observatories increase rapidly with distance, even during relatively low magnetic activity. Thus, it is of interest to describe how the differences (or errors) in external magnetic field extrapolation from a single observatory grow with distance from its location. These differences are modulated by local time, seasonal and solar cycle variations, as well as geomagnetic activity, giving a complex temporal and spatial relationship. A straightforward way to describe the differences are via confidence intervals for the extrapolated values with respect to distance. To compute the confidence intervals associated with extrapolation of the external field at varying distances from an observatory, we used 695 station-years of overlapping minute-mean data from 37 observatories and variometers at high latitudes from which we removed the main and crustal fields to isolate unmodelled signals. From this data set, the pairwise differences were analysed to quantify the variation during a range of time epochs and separation distances. We estimate the 68.3%, 95.4% and 99.7% confidence levels (equivalent to the 1 sigma, 2 sigma and 3 sigma Gaussian error bounds) from these differences for all components. We find that there is always a small non-zero bias that we ascribe to instrumentation and local crustal field induction effects. The computed confidence intervals are typically twice as large in the north-south direction compared to the east-west direction and smaller during the solstice months compared to the equinoxes.
机译:在远离天文台的位置提供对地球表面磁场的准确估算,具有有用的科学和商业应用,例如在重复站数据缩减,太空天气预报和航空磁测量中。尽管在低纬度和中纬度附近的电磁观测站之间的测量相关性很好,但是在高地磁纬度(58-75度)下,即使在相对低的磁活动期间,观测站之间的外场差异也会随着距离而迅速增加。因此,有趣的是描述来自单个观测站的外部磁场外推的差异(或误差)如何随距其位置的距离而增长。这些差异受到当地时间,季节和太阳周期变化以及地磁活动的调节,从而形成了复杂的时空关系。描述差异的一种直接方法是通过针对距离的外推值的置信区间。为了计算与从天文台到不同距离的外场外推相关的置信区间,我们使用了来自高纬度37个天文台和变径仪的695站年的重叠分钟平均值数据,从中删除了主场和地壳以隔离未建模的信号。从该数据集中,分析成对差异以量化在一段时间和间隔距离范围内的变化。从所有组件的这些差异中,我们估计出68.3%,95.4%和99.7%的置信度(相当于1 sigma,2 sigma和3 sigma高斯误差范围)。我们发现总是存在一个小的非零偏差,这归因于仪器和局部地壳场的感应效应。计算得出的置信区间通常在东西向方向上在南北方向上是两倍,而在冬至月间则比春分时小。

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