Research Activity on Synthetic Aperture Radiometry in CSSAR/CAS
Interferometric synthetic aperture radiometry is a relative new technique in the area of microwave earth observation to measure the brightness temperature distribution of the earth. It can enhance the spatial resolution of the passive microwave remote sensing effectively. Steady progress of this technology have been achieved in both one dimensional and two dimensional cases since 1990 s. The typical instruments are ESTAR and MIRAS,developed by NASA (and umass) and ESA respectively. Relative research has also been conducted in China,mainly by National Microwave Remote Sensing Laboratory (NMRS Lab),Center for Space Science and Applied Research (CSSAR),Chinese Academy of Sciences (CAS),since the middle of 1990 s. A C-band and an X-band instrument has been developed. In this paper,research activities on synthetic aperture radiometry in CSSAR/CAS will be reviewed and summarized,including the development of the instruments. Finally,further plans in synthetic aperture radiometry in CSSAR/CAS will also be prospected.
Ji Wu Hao Liu Shouzheng Ban Xiaolong Dong Jingshan Jiang
Center for Space Science and Applied Research,Chinese Academy of Sciences,China
国际会议
Progress in Electromagnetics Research Symposium 2005(2005年电磁学研究新进展学术研讨会)(PIERS 2005)
杭州
英文
538-542
2005-08-22（万方平台首次上网日期，不代表论文的发表时间）