測地学会誌
Online ISSN : 2185-517X
Print ISSN : 0038-0830
ISSN-L : 0038-0830
62 巻, 1 号
選択された号の論文の5件中1~5を表示しています
坪井賞受賞記念論文
  • 太田 雄策
    2016 年 62 巻 1 号 p. 1-19
    発行日: 2016/07/29
    公開日: 2017/04/30
    ジャーナル フリー

    GNSS is strong and common observation tool for understanding the spatial and temporal development of crustal deformation. The one of the advantage of GNSS is the high dynamic range with broadband characteristic. Based on these characteristics, various studies developed the quasi realtime coseismic fault determination method deduced from the real-time GNSS data. Crustal deformation due to coseismic slips at an earthquake fault detected by real-time GNSS analysis is quite useful in estimating fault expansion and the amount of its slip. It in turn contributes to rapid tsunami warning for near field coast, even though the huge interplate earthquakes such as larger than the magnitude 9 event. This paper summarizes the author’s past research on improvement and its comprehensive noise assessment of real-time kinematic GNSS analysis and development of rapid coseismic fault determination technique based on those data. The author also reviews recent development status on crustal deformation monitoring system in Japan, which have been jointly developed by Geospatial Information Authority of Japan and Tohoku University. Furthermore, the author also discusses a future direction of the real-time crustal deformation monitoring and near field tsunami early warning system based on the GNSS data.

寄書
テクニカルレポート
  • 河野 宣之
    2016 年 62 巻 1 号 p. 29-44
    発行日: 2016/07/29
    公開日: 2017/04/30
    ジャーナル フリー

    A Doppler frequency has been used to track a spacecraft and to know the orbit. FFT (Fast Fourier Transforms) gives a mean spectrum for a period of Fourier transforms so that it is a useful tool to estimate a Doppler frequency from a received signal. Phase variations of the signal in the period would be derived if we need to know the frequency variation of the signal in the period. FFT enables us to estimate phase variations of the signal in the period, when the signal is frequency-converted by software. The software for phase estimation of S- and X-band carrier signals with very narrow bandwidth (e.g. several ten Hz) has been developed, using time series data sampled at two hundred ksps (kilo-sample per second) after frequency conversions by hardware. This software can be applied to detect the lunar ionosphere with very small TEC variations by tracking phases of two frequency signals from a lunar orbiter. It can be widely used to measure phases of a carrier signal from a satellite, for example, GNSS or others with high accuracy.

訂正
報告
feedback
Top