• 제목/요약/키워드: RINEX observation file

검색결과 2건 처리시간 0.021초

MATLAB GUI 기반 GPS RINEX 관측 파일 생성 소프트웨어의 개발 (Development of MATLAB GUI Based Software for Generating GPS RINEX Observation File)

  • 김동욱;윤호;한덕화;장주영;기창돈;소형민;이기훈;장재규
    • 한국항행학회논문지
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    • 제19권4호
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    • pp.299-304
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    • 2015
  • 본 논문에서는 MATLAB GUI 기반으로 개발된 GPS RINEX 관측 파일 생성 소프트웨어에 대해서 소개한다. 개발된 소프트웨어는 두 가지 데이터 생성 모드를 기반으로 기준국 혹은 동적 사용자의 실제 GPS 측정치와 유사한 L1/L2 의사거리, L1/L2 반송파 위상, 도플러 측정치를 정확하고 효율적으로 생성한다. 생성된 측정치 결과는 최종적으로 RINEX version 3.0 관측 파일로 출력된다. 본 논문에서는 소프트웨어 검증을 위해 기준국의 실측 데이터를 기반으로 측정치 바이어스, 변화율, 잡음 수준을 분석해보았다. 그 결과 개발된 소프트웨어가 실제 GPS 측정치와 RMS 약 0.7 m 수준의 바이어스 오차를 갖는 GPS 측정치를 생성함을 확인하였다.

Generation of Ionospheric Delay in Time Comparison for a Specific GEO Satellite by Using Bernese Software

  • Jeong, Kwang Seob;Lee, Young Kyu;Yang, Sung Hoon;Hwang, Sang-wook;Kim, Sanhae;Song, Kyu-Ha;Lee, Wonjin;Ko, Jae Heon
    • Journal of Positioning, Navigation, and Timing
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    • 제6권3호
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    • pp.125-133
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    • 2017
  • Time comparison is necessary for the verification and synchronization of the clock. Two-way satellite time and frequency (TWSTFT) is a method for time comparison over long distances. This method includes errors such as atmospheric effects, satellite motion, and environmental conditions. Ionospheric delay is one of the significant time comparison error in case of the carrier-phase TWSTFT (TWCP). Global Ionosphere Map (GIM) from Center for Orbit Determination in Europe (CODE) is used to compare with Bernese. Thin shell model of the ionosphere is used for the calculation of the Ionosphere Pierce Point (IPP) between stations and a GEO satellite. Korea Research Institute of Standards and Science (KRISS) and Koganei (KGNI) stations are used, and the analysis is conducted at 29 January 2017. Vertical Total Electron Content (VTEC) which is generated by Bernese at the latitude and longitude of the receiver by processing a Receiver Independent Exchange (RINEX) observation file that is generated from the receiver has demonstrated adequacy by showing similar variation trends with the CODE GIM. Bernese also has showed the capability to produce high resolution IONosphere map EXchange (IONEX) data compared to the CODE GIM. At each station IPP, VTEC difference in two stations showed absolute maximum 3.3 and 2.3 Total Electron Content Unit (TECU) in Bernese and GIM, respectively. The ionospheric delay of the TWCP has showed maximum 5.69 and 2.54 ps from Bernese and CODE GIM, respectively. Bernese could correct up to 6.29 ps in ionospheric delay rather than using CODE GIM. The peak-to-peak value of the ionospheric delay for TWCP in Bernese is about 10 ps, and this has to be eliminated to get high precision TWCP results. The $10^{-16}$ level uncertainty of atomic clock corresponds to 10 ps for 1 day averaging time, so time synchronization performance needs less than 10 ps. Current time synchronization of a satellite and ground station is about 2 ns level, but the smaller required performance, like less than 1 ns, the better. In this perspective, since the ionospheric delay could exceed over 100 ps in a long baseline different from this short baseline case, the elimination of the ionospheric delay is thought to be important for more high precision time synchronization of a satellite and ground station. This paper showed detailed method how to eliminate ionospheric delay for TWCP, and a specific case is applied by using this technique. Anyone could apply this method to establish high precision TWCP capability, and it is possible to use other software such as GIPSYOASIS and GPSTk. This TWCP could be applied in the high precision atomic clocks and used in the ground stations of the future domestic satellite navigation system.