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《Chinese Journal of Space Science》 2004-04
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THE DEVELOPMENT AND STATUS OF SPACE X-RAY IMAGING TELESCOPE

LI Baoquan~(1,2) ZHU Guangwu~1 LIN Huaan~1 WANG Shijin~1 PENG Jilong~1 1 Center for Space Science and Applied Research, The Chinese Academy of Sciences, Beijing 100080 2 Graduate School, The Chinese Academy of Sciences  
With the development of space technique, the space systems are becoming more and more complicated, but they are more and more susceptible to space weather. Consequently, space weather forecast is being widely researched in the world. The great impacts on the normal life of human made by space weather are presented in this paper. The importance about solar X-ray imaging in space weather forecast is expatiated on. The fundamental principle, the principal design and the instrument characteristics of celestial and solar X-ray grazing imager operating successfully in space are introduced. The principal technical indices of solar X-ray imaging telescope (SXIT) which is being developed in China are presented. The SXIT integrates the gracing incident telescope and the normal incident telescope and operates in the 0.4--10 nm X-ray band interval and the 19.5 nm EUV band. It can provide the high resolution solar disk imaging for its 45 arcmin field of view and 5 arcsec spatial resolutions. The SXIT is the newest solar storm monitor at present. The SXIT extends the temperature response to the coronal plasma and enhances the sensitivity to the coronal plasma with lower temperature, so more signatures and precursors of the solar eruption can be observed by the SXIT. The SXIT is dedicated to domestic space weather forecast. It will firstly fly on the FY-4 serial meteorological satellites that operates on a geostationary orbit, so real-time data for space weather forecast can be obtained 24 hours per day. The SXIT will greatly enhance the ability of the domestic space weather forecast and the research of solar physics if it operates successfully on orbit.
【CateGory Index】: P111
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【References】
Chinese Journal Full-text Database 2 Hits
1 LI Bao-Quan 1 ,ZHU Guang-Wu 1 ,WANG Shi-Jin 1 ,LIN Hua-An 1 ,PENG Ji-Long 1 , LIU Jie 1 ,WEI Fei 1 ,KONG Ling-Gao 1 ,CHEN Bo 2 ,GONG Yan 2 ,SHAO Jing-Hong 2 , MA Chang-Sheng 2 ,TANG Yu-Hua 3 ,QIU Ke-Ping 3 1 The Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100080, China 2 Changchun Institute of Optics,Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130022, China 3 Department of Astrophysics, Nanjing University, Nanjing 210093, China;The solar X-EUV imaging telescope[J];Chinese Journal of Geophysics;2005-02
2 LIU Xin~(1,2) LI Baoquan~1 ~1(Center for Space Science and Applied Research,Chinese Academy of Sciences,Beijing 100190) ~2(Graduate University of Chinese Academy of Sciences);Optimizing Process of the Images Captured by the Solar X-EUV Imaging Telescope[J];Chinese Journal of Space Science;2008-04
【Co-references】
Chinese Journal Full-text Database 7 Hits
1 LI Bao-Quan 1, 2 ZHU Guang-Wu 1 WANG Shi-Jin 1 LIANG Jin-Bao 1 WANG Chun-Qin 1 1 Center for Space Science and Applied Research,Chinese Academy of Sciences, Beijing 100080, China 2 Graduate School, Chinese Academy of Sciences, Beijing 100039, China;THE SPACE PARTICLE COMPOSITION DETECTOR ABOARD FY-1C SATELLITE AND ANALYSIS OF PARTICLE RADIATION IN SOUTH ATLANTIC ANOMALY[J];Chinese Journal of Geophysics;2004-06
2 LI Bao-Quan 1 ,ZHU Guang-Wu 1 ,WANG Shi-Jin 1 ,LIN Hua-An 1 ,PENG Ji-Long 1 , LIU Jie 1 ,WEI Fei 1 ,KONG Ling-Gao 1 ,CHEN Bo 2 ,GONG Yan 2 ,SHAO Jing-Hong 2 , MA Chang-Sheng 2 ,TANG Yu-Hua 3 ,QIU Ke-Ping 3 1 The Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100080, China 2 Changchun Institute of Optics,Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130022, China 3 Department of Astrophysics, Nanjing University, Nanjing 210093, China;The solar X-EUV imaging telescope[J];Chinese Journal of Geophysics;2005-02
3 CAO Mao-yong 1,2 , YU Dao-yin 1 (1. College of Precision Instrument and Opto-electronic Engineering, Tianjin Un iversity, Tianjin 300072, China) (2. Information and Electrical Engineering School, Shandong University of Scienc e and Technology, Jin;Pseudocolor coding of gray image based on perceptual color space[J];Optical Technology;2002-04
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5 Hu Jiasheng; Zhang Jinghe;Wang Baolin (Changchun Institute of Optics and Fine Mechanics, Academia Sinica,Changchun 130022)Sun Kexu; Ma Hongliang; Xu Heping (Southwest Institute of Nuclear of Nuclear Physics and Chemistry,Chengdu 610003);Manufacturing Technology of an X-ray Grazing Mirror System[J];CHINESE JOURNAL OF LASERS;1995-04
6 PAN Ning-ning,WANG Zhan-shan,GU Chun-shi,QIN Shu-ji(Department of Physics,Tongji University,Shanghai 200092,China);Image quality with Kirkpatrick-Baez microscope in hard X-ray[J];High Power Laser and Particle Beams;2006-01
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【Secondary References】
Chinese Journal Full-text Database 4 Hits
1 Zhang Xin Su Donglin(School of Electronics and Information Engineering,Beijing University of Aeronautics and Astronautics,Beijing 100083,China)Li Baoquan Peng Jilong(Center for Space Science and Applied Research,Chinese Academy of Sciences,Beijing 100080,China);Jitter compensation system in solar X-EUV imaging telescope[J];Journal of Beijing University of Aeronautics and Astronautics;2007-03
2 LIU Xin~(1,2) LI Baoquan~1 ~1(Center for Space Science and Applied Research,Chinese Academy of Sciences,Beijing 100190) ~2(Graduate University of Chinese Academy of Sciences);Optimizing Process of the Images Captured by the Solar X-EUV Imaging Telescope[J];Chinese Journal of Space Science;2008-04
3 PENG Jilong~(1,2) ZHU Guangwu~1 WEI Fei~(1,2) LI Baoquan~1 1(Center for Space Science and Applied Research,Chinese Academy of Sciences,Beijing 100190) 2(Graduate University of Chinese Academy of Sciences);Solar Extreme Ultraviolet Multichannel Imager[J];Chinese Journal of Space Science;2009-04
4 ZENG Zhi-rong,LI Bao-quan,PENG Ji-long,ZHANG Xin,ZHOU Hong-jun1,HUO Tong-lin(Center for Space Science and Applied Research,CAS,Beijing 100190,P.R.China;National Synchrotron Radiation Laboratory1,USTC,Hefei 230026,P.R.China);EUV Response Calibration of Astronomic CCD[J];Science Technology and Engineering;2009-08
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