首页 | 本学科首页   官方微博 | 高级检索  
     检索      


Identification of a debris cloud from the nuclear powered SNAPSHOT satellite with haystack radar measurements
Authors:CL Stokely  EG Stansbery
Institution:1. ESCG/Barrios Technology, Mail Code JE104, 2224 Bay Area Blvd., Houston, TX 77058, USA;2. Orbital Debris Program Office, NASA Johnson Space Center, NASA, 2101 NASA Parkway, Houston, TX 77058, USA
Abstract:Data from the Massachusetts Institute of Technology Lincoln Laboratory Long Range Imaging Radar (known as the Haystack radar) have been used in the past to examine families of objects from individual satellite breakups or families of orbiting objects that can be isolated in altitude and inclination. This is possible because, for some time after a breakup, the debris cloud of particles can remain grouped together in similar orbit planes. This cloud will be visible to the radar, in fixed staring mode, for a short time twice each day, as the orbit plane moves through the field of view. There should be a unique three-dimensional pattern in observation time, range, and range rate which can identify the cloud. Eventually, through slightly differing precession rates of the right ascension of ascending node of the debris cloud, the observation time becomes distributed so that event identification becomes much more difficult.
Keywords:Orbital debris  Space debris  Nuclear  Radar  Haystack  SNAPSHOT
本文献已被 ScienceDirect 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号