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The parameters of Earth free core nutation (FCN) are two relatively significant geophysical parameters. Sasao et al. (1980)
and Wahr and Bergen (1986) provided the theoretical estimation values of FCN parameters. Gwinn, Herring and Shapiro (1987)
first obtained the observational values of FCN parameters by very long base Interference (VLBI) at Cambridge University. In
the same year, Neuberg and Zürn in former West Germany and Hinderer in France began to retrieve FCN parameters by the observation
of gravity tides and introduced the stacking method. The other scholars who researched into the same geophysical problems
by applying the data of gravity tides basically followed the stacking method. The results they reached were similar to the
observational result of FCN parameters given by Neuberg et al. in 1987. But the observational results of FCN parameters gained
from gravity tides were not identical with those from VLBI, mainly because of the large difference of quality of FCN. So there
was not an affirmative observational result of FCN parameters since then. In this paper, The authors firstly introduce the
tri-frequency spectrum method with clearly geometrical and geophysical meaning for the resolution of FCN parameters, and the
observational results of FCN parameters obtained from tide data at three superconducting gravity stations were accordant with
those from VLBI, which will be relatively important to arriving at a certain observational result of FCN parameters. 相似文献
174.
The parameters of Earth free core nutation (FCN) are two relatively significant geophysical parameters. Sasao et al. (1980) and Wahr and Bergen (1986) provided the theoretical estimation values of FCN parameters. Gwinn, Herring and Shapiro (1987) first obtained the observational values of FCN parameters by very long base Interference (VLBI) at Cambridge University. In the same year, Neuberg and Zürn in former West Germany and Hinderer in France began to retrieve FCN parameters by the observation of gravity tides and introduced the stacking method. The other scholars who researched into the same geophysical problems by applying the data of gravity tides basically followed the stacking method. The results they reached were similar to the observational result of FCN parameters given by Neuberg et al. in 1987. But the observational results of FCN parameters gained from gravity tides were not identical with those from VLBI, mainly because of the large difference of quality of FCN. So there was not an affirmative observational result of FCN parameters since then. In this paper, The authors firstly introduce the tri-frequency spectrum method with clearly geometrical and geophysical meaning for the resolution of FCN parameters, and the observational results of FCN parameters obtained from tide data at three superconducting gravity stations were accordant with those from VLBI, which will be relatively important to arriving at a certain observational result of FCN parameters. 相似文献
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分析2015年8月—2018年7月满洲里地震台FHDZ-M15地磁总场与分量组合观测系统记录的地磁秒采样观测数据(剔除磁暴与磁扰时间段),发现台站地磁秒采样数据资料所受干扰主要呈阶跃和尖峰形态,通过测量测区地磁场水平梯度,排查周边环境,并对设备和线路进行漏电检测,认为:阶跃形态干扰主要由高压直流输电和车辆停放引起;经逐项排查对UPS加热及输电线路漏电检测,仪器室温度过低和输电线路漏电均造成高频毛刺尖峰形态干扰,对UPS加热处理,干扰状态得到改善,但Z、F分量干扰仍在.受满洲里气候条件等因素限制,未能在2019年完成输电线路更换,当前无法确定干扰是否为输电线路漏电所致,后续将采取相应措施予以确认. 相似文献