电解质分析仪校准方法的研究

经过长期的实践摸索,对各种电解质分析仪进行了系统的测试和论证,初步建立了一套可靠的校准电解质分析仪的方法.该方法各项指标评价结果符合仪器的设计性能及实际测试工作要求,对医学临床及法定计量检定机构开展电解质分析仪的校准工作有一定的指导意义.     

酶标分析仪检定用中性滤光片的校准

提出酶标分析仪检定用中性滤光片的校准方法，并用校准实例对校准方法进行了验证。结合校准方法，根据JJF 1059.1—2012《测量不确定度评定与表示》建立了数学模型，不确定度的来源有测量结果的重复性、分光光度计透射比误差、分光光度计杂散辐射、中性滤光片年稳定性、中性滤光片均匀性，按该校准方法校准的中性滤光片，校准结果的不确定度为U=0.005(k=2)，校准结果能够满足JJG 861—2007《酶标分析仪检定规程》对中性滤光片不确定度U≤0.01(k=2)的要求，可用于开展酶标分析仪吸光度值的校准工作。     

液相色谱仪自动进样器样品室温度的校准

液相色谱仪自动进样器样品室的温度对于液相色谱样品的储存与测试有直接影响。为了保证其准确性与溯源性，结合其温控原理和布局结构提出相关的校准项目、校准方法、技术指标及校准设备。同时，针对不同测量方式的校准设备，对有线温度测量方式与无线温度测量方式进行对比。通过分析其结构适应性和实际测量结果得出，有线温度测量方式虽然具备易于获得且成本较低的优势，但其适用范围较小，且可能导致缠绕、牵扯、样品室无法正常闭合、探头位置不易控制等情况，测量结果也显示其会影响样品室温度均匀性的测量。而无线温度测量方式由于其没有线的约束，能适用于各类自动进样器，从实际测量操作和测量结果上看也优于有线测量方式，更适合用于液相色谱仪自动进样器样品室温度的校准。     

实验室从ISO/IEC指南25-1990质量体系向ISO/IEC 17025-1999质量体系的过渡

对ISO/IEC17025-1999和ISO/IEC指南25-1990进行了比较，分析了ISO/IEC17025-1999的显著变化，提出了由ISO/IEC指南25-1990质量体系向ISO/IEC17025-1999质量体系过渡的措施。     

氦离子化气相色谱仪校准用混合物中甲烷气体标准物质研制

介绍氦中甲烷气体标准物质的制备方法.以超纯氦气和高纯甲烷为原料,采用称量法制备特性值为10μmol/mol的氦中甲烷气体标准物质.采用气相色谱法(DID检测器)对制备的标准物质进行均匀性、稳定性检验,并对定值结果的不确定度进行评定.研制的气体标准物质均匀性和稳定性良好,有效期为12个月,相对扩展不确定度为2％(k=2)...     

Twin-image problem in digital holography—a survey(Invited Paper)

Zero-order and twin images are a serious obstacle in achieving a high-quality output in in-line digital holography （DH）. They decrease the useful bandwidth of the off-axis DH. Over the years the twin image removal problem was approached both by instrumental and numerical means. The paper provides an extended survey of the proposed solutions with their pros and cons as a guide for further advance in this field. Processing of a single spatial carrier fringe pattern involves spatial filtering in the frequency domain, spatial phase-shifting （PS） or wavelet transform. A point source digital holographic microscopy （DHM）, introduction of calibration measurements or various modifications of PS technique are instrumental solutions to the twin image problem for in-line DH. Numerical solutions to the same problem include iterative and non-iterative approaches, diffraction-based and inverse problem solutions, reconstruction of purely real or phase objects and of complex objects, reconstruction of plane and volume objects. Elimination only of the zero-order image relies on non-linear filtering or additional calibration measurements.     

Research on calibration method in lab of direct solar channels of Sun photometer

We develop a new calibration method in lab by measuring the absolute spectral irradiance responsivity of Sun photometer sun channel. The absolute power responsivity of Sun photometer is obtained when a white laser double monochromator system serve as a source, and a standard transfer detector calibrated against cryogenic absolute radiometer is assembled to measure the absolute power of laser beam. The effective area of aperture is measured through laser raster scanning method, and the relative spectral irradiance responsivity of the corresponding channel is obtained by using tungsten-halogen lamps double monoehromator system. On the basis of the above results, the top of the atmosphere responsive constants V0 （500, 675, and 870 nm） are obtained by integration with extraterrestrial solar spectral irradiance data. Comparing the calibration results with that of CIMEL, France in November 2011, the relative differences are 4.38%, 2.23%, and 2.45%, respectively. The calibration uncertainty reaches to 2.048×10^-2, which shows a remarkable consistency with the Langley plot method. Further, our scheme can overcome the limits of space and atmospheric conditions which are only available at a high-altitude calibration site in particular date. The advantages lie in not only shortening the experiment period but also being of high precision. This new scheme definitely plays an important role in supporting the current and future sun photometry calibration activities which are significant to earth observation.     

A pressure calibration method for a portable wide-access ＂panoramic＂ cell

A simple and convenient pressure calibration method is developed for a newly designed portable wide-access ＇panoramic＇ cell. This cell is adapted to angle-dispersive-mode high-pressure in situ neutron diffraction of reactor neutron sources. This pressure calibration method has established a relationship between the cell pressure and the anvil displace- ment （gasket compression） based on the fixed-point calibration technique. By employing TiZr gasket with a thickness of 3 mm and WC anvil with a culet of 4 mm diameter, the average anvil displacements are 1.31 mm and 2.22 mm for Bi phase transitions （2.55 GPa and 7.7 GPa）, and 1.85 mm for Ba phase transitions （5.5 GPa）, respectively. In this pressure range, the pressure increases quickly with decreasing gasket thickness, and undergoes a linear increase with the anvil displacement. By extrapolating the calibration curve, the cell pressure will achieve 10 GPa when the anvil displacement is around 2.5 ram.     

Online charge calibration of LHAASO-WCDA——a study with the engineering array

LHAASO-WCDA is a large ground-based water Cherenkov detector array planned to be built at ShangriLa, Yunnan Province, China. As a major component of the LHAASO project, the main purpose of LHAASO-WCDA is to survey the northern sky for very-high-energy（above 100 GeV） gamma ray sources and measure the spectrum. To gain full knowledge of the water Cherenkov technique and to investigate the engineering issues, a 9-cell detector array has been built at the Yang-Ba-Jing site, neighboring the ARGO-YBJ experiment. With the array, charge calibration methods for both low and high ranges of the PMT readout are studied, whose result shows that a precision at several percentages can be reached, which can satisfy the requirement of the detector array. During the long term operation, the charge calibration stability and environmental afection are studied; in this paper, the results are discussed. These calibration methods are proposed to be applied in the future LHAASO-WCDA project.