Application of Synthetic Aperture Radiometer Technology in Solar Wind Remote Sensing
Synthetic aperture radiometer technology used nowadays in earth remote sensing is an extended development from ground-based radio astronomy used for stellar observation. However,once the technology is further developed in the Earth remote sensing area,it can certainly be applied back in its original field or other fields. In this paper,we discuss a rotational phased array of time-shared synthetic aperture technology application in solar wind remote sensing. The main idea is to send a spacecraft into solar polar orbit. From this orbit,one can look down to the ecliptic plane. In and around the ecliptic plane, the most interested and useful information of the interplanetary solar wind is the Corona Material Ejection (CME) of the Sun since it can cause sever geo-space storms and result man made technical system failure such as navigation positioning errors and communication break down or even satellite failures. The main scientific initiatives and technical system conceptual design of this application will be presented in this paper.
Ji Wu Hao Liu Weiying Sun Chi Wang Shui Wang Chingsheng Wu
Center for Space Science and Applied Research,Chinese Academy of Sciences,China Chinese University of Science and Technology,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
515-519
2005-08-22（万方平台首次上网日期，不代表论文的发表时间）