中国实验快堆(China Experimental Fast Reactor,CEFR)采用液态金属钠为冷却剂,一回路冷阱工艺间的放射性钠气溶胶对工作人员的健康和安全有危害,需要对其进行监测以便及时采取相应的防护措施。为保证监测结果的准确性,需要对放射性钠...中国实验快堆(China Experimental Fast Reactor,CEFR)采用液态金属钠为冷却剂,一回路冷阱工艺间的放射性钠气溶胶对工作人员的健康和安全有危害,需要对其进行监测以便及时采取相应的防护措施。为保证监测结果的准确性,需要对放射性钠气溶胶监测仪进行定期校准。通过采用特制的放射性气溶胶滤膜源,对放射性钠气溶胶监测仪进行校准方法研究,分别对监测仪计数率对标准源活度响应、相对误差、重复性等主要校准不确定度来源进行分析及不确定度评定。研究结果表明:放射性钠气溶胶监测仪计数率对活度响应因子的不确定度为5%(k=2),该校准方法适用于放射性钠气溶胶监测仪的校准,满足该监测仪量值溯源的要求。展开更多
The ESA Sentinel-2 mission developed by European Aeronautic Defense and Space Compagny (EADS) Astrium will be devoted to Earth high resolution spectral imagery for the purpose of a global environmental monitoring. A...The ESA Sentinel-2 mission developed by European Aeronautic Defense and Space Compagny (EADS) Astrium will be devoted to Earth high resolution spectral imagery for the purpose of a global environmental monitoring. As a subcontractor of EADS Astrium, AMOS was responsible for the manufacturing of the instrument telescope mirrors and for the validation of the telescope alignment procedure. This paper details the mirror manufacturing sequences from mirror CVD-SiC cladding to surface figuring and coating, outlining the metrology steps and their corresponding accuracy budget. The telescope alignment process is described in connection with the tooling and techniques that helped achieve the required optical performance of less than 90 nm RMS wavefront error within the telescope field of view.Pierre Gloesenet展开更多
文摘中国实验快堆(China Experimental Fast Reactor,CEFR)采用液态金属钠为冷却剂,一回路冷阱工艺间的放射性钠气溶胶对工作人员的健康和安全有危害,需要对其进行监测以便及时采取相应的防护措施。为保证监测结果的准确性,需要对放射性钠气溶胶监测仪进行定期校准。通过采用特制的放射性气溶胶滤膜源,对放射性钠气溶胶监测仪进行校准方法研究,分别对监测仪计数率对标准源活度响应、相对误差、重复性等主要校准不确定度来源进行分析及不确定度评定。研究结果表明:放射性钠气溶胶监测仪计数率对活度响应因子的不确定度为5%(k=2),该校准方法适用于放射性钠气溶胶监测仪的校准,满足该监测仪量值溯源的要求。
文摘The ESA Sentinel-2 mission developed by European Aeronautic Defense and Space Compagny (EADS) Astrium will be devoted to Earth high resolution spectral imagery for the purpose of a global environmental monitoring. As a subcontractor of EADS Astrium, AMOS was responsible for the manufacturing of the instrument telescope mirrors and for the validation of the telescope alignment procedure. This paper details the mirror manufacturing sequences from mirror CVD-SiC cladding to surface figuring and coating, outlining the metrology steps and their corresponding accuracy budget. The telescope alignment process is described in connection with the tooling and techniques that helped achieve the required optical performance of less than 90 nm RMS wavefront error within the telescope field of view.Pierre Gloesenet