用电报设备估计低频视电阻率和相位

Q4 Earth and Planetary Sciences Papers in Meteorology and Geophysics Pub Date : 2003-08-29 DOI:10.2467/MRIPAPERS.54.47
H. Takayama
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引用次数: 0

摘要

我们提出了一种时域估计视电阻率和相位的方法。该方法利用多元回归模型,其中通过最小化AIC(赤池信息准则)来确定顺序。该方法比传统的基于谱分析的频域方法在估计相同低频视电阻率时所需的数据长度要长几倍。因此,将该方法应用于磁暴中波长较长的短长度数据,可以估计低频时的视电阻率和相位,而感应地磁场有限波长的影响很小。将该方法应用于地电场观测网中日本标准观测站Kakioka地磁观测站利用电报设施观测到的地电场数据和地磁场数据。地电场数据在很长一段时间内非常稳定,因为电极埋在5米以上的深度,接触电阻小于2欧姆。此外,由于18.8 ~ 27.4 km的观测线长度比普通观测线长得多,且大部分地电变化是由地磁变化引起的,因此地电数据具有较高的信噪比(信号为诱发变化)。在3.3 × 10-5 ~ 10 × 1.0-3 Hz的低频范围内(对应512 ~ 16 min周期)估计了视电阻率和相位。由于分析中使用的数据的时间跨度是在大规模磁暴期间,因此估计不太可能受到诱导地磁场有限波长的影响。
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Estimating apparent resistivity and phase at low frequencies using telegraphic facilities
We propose a time-domain method for estimating the apparent resistivity and phase. The method utilizes a multiple regression model where the order is determined by minimizing the AIC (Akaike Information Criterion). The method is superior to conventional frequency-domain methods based on spectral analysis, since the data length necessary for the latter methods is several times longer than that for the former in estimating the apparent resistivity at the same low frequency. Therefore, applying this method to shorter length data having long wavelengths like those in a magnetic storm, we can estimate apparent resistivities and phases at low frequencies with little effect of the finite wavelength of the inducing geomagnetic field. This method was applied to geoelectric field data observed by means of telegraphic facilities and geomagnetic field data at the Kakioka Magnetic Observatory, which is the standard observatory in Japan, located in the observation network of the geoelectric field. The geoelectric field data are very stable over a long time period because the electrodes are buried to a depth of more than 5 meters and have a contact resistance of less than 2 ohms. Furthermore, the geoelectric data had a high signal-to-noise ratio (signal is induced variations), because the lengths of observation lines ranging from 18.8 to 27.4 km were much longer than that of ordinary observations and the greater part of geoelectric variations were induced by geomagnetic variations. Apparent resistivity and phase in the low-frequency range from 3.3 × 10-5 to 10 × 1.0-3 Hz (corresponding to periods of 512 to 16 minutes) were estimated. Since the time span of the data used in the analysis was within the period of a large-scale magnetic storm, the estimates were unlikely to be affected by the finite wavelength of the inducing geomagnetic field.
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Papers in Meteorology and Geophysics
Papers in Meteorology and Geophysics Earth and Planetary Sciences-Geophysics
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