1. Ground Calibration and In-Flight Performance of the Low Energy Particle Analyzer on FY-4B.
- Author
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Su, Bin, Chen, Anqin, Liu, Mohan, Kong, Linggao, Zhang, Aibing, Tian, Zheng, Liu, Bin, Wang, Xinyue, Wang, Wenjing, Zhang, Xiaoxin, Zong, Weiguo, Zheng, Xiangzhi, and Wang, Jinsong
- Subjects
NUMERICAL weather forecasting ,GEOSTATIONARY satellites ,ELECTRON distribution ,SPACE environment ,METEOROLOGICAL satellites ,SURFACE charges - Abstract
The FY-4B satellite is one of the second generation of China's geosynchronous meteorological satellites aiming at numerical weather forecasts. The space environment monitoring package (SEMP) onboard the FY-4B is a comprehensive instrument package for plasma, high-energy particle, and energetic neutral particle measurements. The low-energy particle analyzer (LEPA) is one of the instruments of the SEMP and consists of two top hat electrostatic analyzers designed for plasma detection. The electron and ion sensors are back-to-back assembled and are integrated to a shared electronic box. It measures the three-dimensional velocity distribution of low-energy electrons and ions on the geosynchronous orbit. In this paper, we present the ground calibration and in-flight performance of the instrument. With the electrostatic deflectors and the cylindrically symmetric structure, the instrument provides high-cadence measurements of electron and ion velocity distributions with a wide field of view (FOV) of 180° by 100°, an angular resolution of 16.7° × 20°, and a broad energy range for both the electrons and ions from tens of eV to above 30 keV, with a 1 s time resolution. The geometric factors of the electron and ion analyzers are 1.1 × 10
−3 cm2 ·sr·eV/eV and 1.4 × 10−3 cm2 ·sr·eV/eV, respectively, which fulfills the requirements of the low-energy plasma measurement. The LEPA monitored typical space environment disturbance such as geomagnetic storms and successfully recorded the responses of plasma energy fluxes. Satellite surface charging events were measured, with the highest potentials of −2000 V in the shadow period and −500 V in the nonshadow period. [ABSTRACT FROM AUTHOR]- Published
- 2023
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