The Experimental Satellite on Electromagnetism Monitoring
doi: 10.11728/cjss2014.05.558 cstr: 32142.14.cjss2014.05.558
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摘要: The Experimental Satellite on Electromagnetism Monitoring (ESEM) was proposed in 2003 and proved in 2013 after 10-years' scientific demonstration. The ESEM mission was proposed to be the first satellite of space-based geophysical fields observation system in China with a lot of application prospects in earthquake science, geophysics, space sciences and so on. And coincide with the mission objectives, the satellite decides to use the Circular Sun Synchronous Orbit with an altitude of 507km and descending node time at 14:00LT. The payload assemble includes 8 instruments, Search-Coil Magnetometer, Electric Field Detector, High precision Magnetometer, GNSS occupation Receiver, Plasma Analyzer, Langmuir Probe, Energetic Particle Detector, and Three-frequency Transmitter. According to the planned schedule, the satellite is due to be launched in 2016-2017 and will be onboard operated for 5 years.Abstract: The Experimental Satellite on Electromagnetism Monitoring (ESEM) was proposed in 2003 and proved in 2013 after 10-years' scientific demonstration. The ESEM mission was proposed to be the first satellite of space-based geophysical fields observation system in China with a lot of application prospects in earthquake science, geophysics, space sciences and so on. And coincide with the mission objectives, the satellite decides to use the Circular Sun Synchronous Orbit with an altitude of 507km and descending node time at 14:00LT. The payload assemble includes 8 instruments, Search-Coil Magnetometer, Electric Field Detector, High precision Magnetometer, GNSS occupation Receiver, Plasma Analyzer, Langmuir Probe, Energetic Particle Detector, and Three-frequency Transmitter. According to the planned schedule, the satellite is due to be launched in 2016-2017 and will be onboard operated for 5 years.
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[1] HeY, Yang D, Qian J, Parrot M. Response of the ionospheric electron density to different types of seismic events[J]. Nat. Hazards Earth Syst. Sci., 2011, 11:2173-2180 [2] Huang J P, Liu J, Ouyang X Y. Analysis of the energetic particles around the M8.8 Chili earthquake [J]. Seismol.Geology, 2010, 32(3):417-423 (in Chinese) [3] Li L Y, Yang J Y, Cao J B, Lu L, Wu Y, Yang D M. Statistical backgrounds of topside-ionospheric electron density and temperature and their variations during geomagnetic activity[J]. Chin. J. Geophys., 2011, 54(10):2437-2444 (in Chinese) [4] Liu J, Zhang X M, Wan W X, Shen X H, Ouyang X Y, Shan X J. Study on the electronic density perturbation detection by DEMETER satellite before Wenchuan earthquake [C]//Geoscience and Remote Sensing Symposium (IGARSS). Honolulu: IEEE [5] Liu J, Huang J P, Zhang X M. Ionospheric perturbations in plasma parameters before globalstrong earthquakes [J].Adv. Space Res., 2014, 53:776-787 [6] Shen Xuhui, Shan Xinjian, Wu Yun, Zhang Jingfa, Kang Chunli, Ding Jianhai, Qian Jiadong, Yang Dongmei, Du Xuebin, Wang Lanwei.Current status of remote sensing application in earthquake science and the framework of Chinese seismo-related satellite mission[J]. Recent Develop. World Seismol., 2007, 8:38-45 (in Chinese) [7] Shen X H, Wang L W, Wu Y, Shan X J, Zhang j F, Kang C L, Zhang X M, Hong S Y, Jing F, Chen L Z, Yuan S G.The framework and developing progress on the space segment of earthquake observation from space in China[J].Satell. Appl., 2011, 6:9-15 (in Chinese) [8] Shen X H, Zhang X M, Wang L W, Chen H R, Wu Y, Yuan S G, Shen J F, Zhao S F, Qian J D, Ding J H. The earthquake-related disturbancesin ionosphere and project of the first China seismo-electromagnetic satellite[J]. Earthquake Sci., 2011, 24(6):639-650 [9] Shen X H, Zhang X M, Hong S Y, Jing F, Zhao S F.Progress and development on multi-parameters remote sensing application in earthquake monitoring in China[J].Earthquake Sci., 2013, 26(6):427-437 [10] Zeren Z M, Shen X H, Zhang X M,Cao J B, Huang J P,Ouyang X Y, Liu J, Bingqing L. Possible ionospheric electromagnetic perturbations induced by the Ms 7.1 Yushu earthquake [J]. Earth Moon Planet., 2012, 108:231-241 [11] Zhang X M, Shen X H, Liu J, Ouyang X Y, Qian J D,Zhao S F. Analysis of ionosphere plasma perturbations before Wenchuan earthquake [J]. Nat. Hazards Earth Syst.Sci., 2009, 9:1259-1266 [12] Zhang X M, Shen X H, Liu J, Ouyang X Y, Qian J D,Zhao S F. Ionospheric perturbations of electron density before the Wenchuan earthquake [J]. Intern. J. Remote Sens., 2010, 31(13):3559-3569 [13] Zhang X M, Zeren Z M, Parrot M, Battiston R, Qian J D, Shen X H. ULF/ELF ionospheric electric field and plasma perturbations related to Chile earthquakes [J]. Adv. Space Res., 2011, 47:991-1000 [14] Zhang X M, Shen X H, Parrot M, Zeren Z M, Ouyang X Y, Liu J, Qian J D, Zhao S F, Miao Y Q. Phenomena of electrostatic perturbations before strong earthquakes (2005-2010) observed on DEMETER[J]. Nat.Hazards Earth Syst. Sci., 2012, 12:75-83 [15] Zhang X M, Fidani C, Huang J P, Shen X H, Zeren ZM,and Qian J D. Burst increases of precipitating electrons recorded by the DEMETER satellite before strong earthquakes[J]. Nat. Hazards Earth Syst. Sci., 2013, 13:197-209 [16] Zhang X M, Shen X H, Zhao S F, Yao L, Ouyang X Y, Qian J D. The characteristics of quasi-static electric field perturbations observed by DEMETER satellite before large earthquakes[J]. J. Asian Earth Sci., 2013,79:42-52 [17] Zhang X M, Shen X H, Liu J, Zeren Z M, Yao L, Ouyang X Y, Zhao S F, Yuan G P. The solar cycle variation of plasma parameters in equatorial and mid latitudinal areas during 2005-2010 [J]. Adv.Space Res., 2014,doi: 10.1016/j.asr.2013.09.012 [18] Zhao S F, Shen X H, Pan WY, Zhang X M, Liao L. Penetration characteristics of VLF wave from atmosphere into lower ionosphere[J]. Earthquake Sci., 2010, 23:275-281 -
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