Observation of the Earth's Magnetic field from KOMPSAT-1

  • Hwang, Jong-Sun (Dept. of Earth System Sciences, Yonsei University) ;
  • Kim, Sung-Yong (Earth Science Education, the Graduate School of Education, Yonsei University) ;
  • Lee, Seon-Ho (Satellite Control System Dept., Korea Aerospace Research Institute) ;
  • Min, Kyung-Duck (Dept. of Earth System Sciences, Yonsei University) ;
  • Kim, Jeong-Woo (Dept. of Geoinformation Engineering, Sejong University) ;
  • Lee, Su-Jin (Dept. of Geoinformation Engineering, Sejong University)
  • 발행 : 2003.11.03

초록

The Earth's total magnetic field was extracted from on board TAM (Three Axis Magnetometer) observations of KOMPSAT-1 satellite between June 19th and 21st, 2000. In the pre-processing, the TAM's telemetry data were transformed from ECI (Earth Centered Inertial frame) to ECEF (Earth Centered Earth Fixed frame) and then to spherical coordination, and self-induced magnetic field by satellite bus itself were removed by using an on-orbit magnetometer data correction method. The 2-D wavenumber correlation filtering and quadrant-swapping method were applied to the pre-processed data in order to eliminate dynamic components and track-line noise, respectively. Then, the spherical harmonic coefficients are calculated from KOMPSAT-1 data. To test the validity of the TAM's geomagnetic field, Danish/NASA/French ${\phi}$rsted satellite's magnetic model and IGRF2000 model were used for statistical comparison. The correlation coefficient between ${\phi}$rsted and TAM is 0.97 and IGRF and TAM is 0.96. It was found that the data from on board magnetometer observations for attitude control of Earth-observing satellites can be used to determinate the Earth's total magnetic field and that they can be efficiently used to upgrade the global geomagnetic field coefficients, such as IGRF by providing new information at various altitudes with better temporal and spatial coverage.

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