用单色亮度比较法确定高温黑体的温度

高温黑体温度的测量水平将直接影响光谱辐射度量值的不确定度。我国的高温温标截止于 2 2 0 0℃。确定2 2 0 0℃以上范围内的温度必须进行温度延伸。从Planck公式的定义出发 ,推导出用单色亮度比较法进行温度延伸的原理和方法。在国家光谱辐射度基准改造中 ,该方法被用来确定高温黑体的温度。实验证明 :使用参考灯替代法能够有效消除探测器灵敏度漂移带来的误差。此外 ,旁证实验用来验证该方案的可行性。     

一种基于控温黑体的红外实时校正技术

二代扫描型热像仪的非均匀性校正(NUC)通常采用定点两点温度校正法或定点多点温度校正法,采用定点校正无法适应时间或环境的变化对探测器带来的影响,造成校正偏离,空间噪声增大。通过在成像光路中设置2个可控温的黑体完成探测器的实时校正,保证在不同时刻以及不同应用环境下,黑体的温度始终实时地跟随场景温度,校正系数实时更新,使非均匀性校正的输出误差有效降低。通过实际多个场景对比试验,采用传统定点校正,非均匀性噪声约为4.0,而该方法的噪声不大于2,有效降低50%。     

A method to retrieve blackbody temperature errors in the two points radiometric calibration

Measurements of the atmospheric thermal emission using an infrared Fourier transform spectrometer need to be radiometrically calibrated. As for several existing instruments (IASI-MetOp, IASI-balloon, NAST-I, AERI, etc.), the two points radiometric calibration is generally performed using two well-characterized blackbodies at two different temperatures (or one blackbody and the cold space), which allow to determine the response and the self-emission of the instrument. To perform an accurate radiometric calibration, the emissivity and the temperature of each blackbody should be known accurately. The blackbody temperatures are chosen to fit the characteristics of the instrument. The measurement of these temperatures is essential. This paper proposes a method to perform an accurate radiometric calibration even when one of the two blackbodies temperatures is not perfectly measured, by numerically retrieving this erroneous temperature.     

目标辐射特性现场校准用大面积黑体辐射源技术研究

红外成像技术在空间探测、对地观测、安防监控等领域的应用越来越广,为了确保红外目标识别的准确性,必须掌握目标的辐射特性。目标辐射特性需要在外场实际条件下测量得到,需要利用大面积黑体辐射源对目标特性测量设备进行现场辐射参数校准。设计了一种大面积黑体辐射源,辐射体采用铝材质并发黑处理,大面积黑体辐射源温度控制采用PID控制算法。在外场实际环境温度为26.8 ℃,湿度为60%时对目标特性测量设备辐射参数进行了校准。试验数据表明:辐射温度测量不确定度为0.4 ℃（k=2）,取得了较好的应用效果。     

一种可溯源的光谱椭偏仪标定方法

提出了一种用X射线反射术标定光谱椭偏仪的方法.作为一种间接测量方法,光谱椭偏术测得的薄膜厚度依赖于其光学常数,不具有可溯源性.在掠入射条件下,X射线反射术能测得薄膜的物理厚度,测量结果具有亚纳米量级的精密度且与薄膜光学常数无关.在单晶硅基底上制备了厚度分别为2nm,18nm,34nm,61nm及170nm的SiO2薄膜标样,并用强制过零点的直线拟合了两种方法的标样测量结果,拟合直线的斜率为1.013±0.013,表明该方法可在薄膜厚度测量中标定光谱椭偏仪.     

A new irradiated quartz for beta source calibration

For luminescence dating to be an accurate absolute dating technique it is very important that we are able to deliver absolutely known radiation doses in the laboratory. This is normally done using a radiation source (alpha, beta, X-ray) calibrated against an absolutely known reference source. Many laboratories have used the various different batches of Risø calibration quartz for the calibration of beta and X-ray sources, but these have been largely undescribed. Here we describe in detail the preparation and luminescence characteristics of a new quartz standard, based on a North Sea beach sand collected from south-western Denmark (Rømø). Two grain sizes (4–11 μm and 180–250 μm) have been examined in detail. These were pre-treated (annealed, dosed and annealed again) to sensitise and stabilise the luminescence signals before being given an absolutely known gamma dose from a point ¹³⁷Cs source in scatter-free geometry. The luminescence characteristics are described; the very intense blue-light stimulated signal is dominated by the fast OSL component and the IR-stimulated signal is negligible. The material is shown to be suitable for measurement using SAR, and the dose recovery ratio is indistinguishable from unity with a standard deviation of <2% for multi-grain aliquots. The material is also shown to be suitable for single-grain calibration, with >80% of the grains giving a useful signal. Although there is an unexplained dispersion in our calibration data of ∼3% (which we cannot attribute to instrument variability), we nevertheless conclude that this material is very suitable for transferring absolute known doses from a standardised gamma source to in-built irradiation sources.     

A three-step system calibration procedure with error compensation for 3D shape measurement

System calibration, which usually involves complicated and time-consuming procedures, is crucial for any three-dimensional （3D） shape measurement system based on vision. A novel improved method is proposed for accurate calibration of such a measurement system. The system accuracy is improved with considering the nonlinear measurement error created by the difference between the system model and real measurement environment. We use Levenberg-Marquardt optimization algorithm to compensate the error and get a good result. The improved method has a 50% improvement of re-projection accuracy compared with our previous method. The measurement accuracy is maintained well within 1.5% of the overall measurement depth range.     

A general procedure for thermomechanical calibration of nano/micro-mechanical resonators

We describe a general procedure to calibrate the detection of a nano/micro-mechanical resonator’s displacement as it undergoes thermal Brownian motion. A brief introduction to the equations of motion for such a resonator is presented, followed by a detailed derivation of the corresponding power spectral density (PSD) function, which is identical in all situations aside from a system-dependent effective mass value. The effective masses for a number of different resonator geometries are determined using both finite element method (FEM) modeling and analytical calculations.     

高温物体比辐射率及温度测量系统

本文介绍了一种利用激光作为光源,利用遮蔽板作为标准噪声辐射源,并以８０３１ 单片机为核心实现测量静止及慢速运动的高温物体的比辐射率及温度系统。该系统主要由光学发射与接收系统、信号放大与处理系统及显示系统三部分组成。文中还详细介绍了该系统的工作原理与基本结构,讨论了其中的技术难点及其相应的解决方法,分析了各量的测量精度对比辐射率及温度测量精度的影响     

具有温度自校准功能的光纤折射率传感器

提出一种具有温度自校准功能的光纤折射率（RI）传感器,传感头结构由2段很短的多模光纤（MMF）之间夹熔一段对折射率不敏感的光纤布拉格光栅（FBG）构成,传感头总长度为14 mm,FBG可以为折射率测量提供良好的温度校准功能。实验结果证明,该传感器的折射率灵敏度为126 nm。其干涉光谱共振波长的温度灵敏度为35.09 pm/℃,用于温度校准的FBG的温度灵敏度为11.14 pm/℃。相比于普通的折射率传感器,这种具有温度自校准功能的折射率传感器具有良好的实用前景。     

A novel radiant source for infrared calibration by using a grooved surface

A radiant source with a large aperture at 5-95 ℃ in the wavelength bands of 8-12μm for calibrating infrared imaging systems has been designed. The effective emissivity of its flat bottom with concentric V-grooves was evaluated by the Monte-Carlo method whose correctness was tested and accuracy was discussed. The structure of the source was completed by incorporating the simulation results with the blackbody cavity effect. The source was certificated via an optical measurement system. The source can provide a consistent radiant flux with temperature uniformity of ±0.1 ℃ over an area of diameter of φ80 mm.     

Distributed sound source localization algorithm with sound velocity calibration in windy environments

A new sound source localization method with sound speed compensation is proposed to reduce the wind influence on the performance of conventional TDOA(Time Difference of Arrival) algorithms. First, the sound speed is described as a set of functions of the unknown source location, to approximate the acoustic velocity field distribution in the wind field. Then,they are introduced into the TDOA algorithm, to construct nonlinear equations. Finally, the particle swarm optimization algorithm is used to estimate the source location. The simulation results show that the proposed algorithm can significantly improve the localization accuracy for different wind velocities, source locations and test area sizes. The experimental results show that the proposed method can reduce localization errors to about 40% of the original error in a four nodes localization system.     

A novel spectroscopic filter used in rotational Raman lidar for the temperature profiling

We perform the rotational Raman temperature measurements in the troposphere and lower stratosphere with high performance. Depending on the aerosol content and presence of clouds in the lower troposphere, the rotational Raman lidar (RRL) is the lidar technique of choice for temperature measurements. However, the Raman filter design is a technical difficulty in RRL systems. Considering the higher spectral resolution and compactness, we select several photonic crystals to construct a novel spectroscopic filter for extracting the required rotational Raman spectrum (RRS) signals of atmospheric molecules. We describe in detail the principle to design the photonic-crystal filter. To verify the feasibility of the novel spectroscopic filter, we carry out some numerical calculations, and our results show that the novel spectroscopic filter has the capability to fine draw the required RRS signal and suppress sufficiently elastic signals. For the RRL system which uses the novel spectroscopic filter, we obtain that a statistical temperature error is less than 1 K up to a height of 3.2 and 5.6 km for daytime and nighttime measurements, respectively. Our simulation conditions are as follows: 532 nm laser with 500 mJ energy, and 10 Hz pulse repeating rate, a 300 mm diameter Cassegrain reflecting telescope with 1000 mm focus length, 0.2 mm diameter multimode optical fiber which sets the field of view (FOV) of receiving system to 0.2 mrad, 45 m range resolution, 9 min observation time, overall optical-system efficiency of 0.6, and a special atmospheric model which integrates the US standard model of 1976 with an actual Mie scattering profile obtained from practical observations.     

A general protocol for temperature calibration of MAS NMR probes at arbitrary spinning speeds

A protocol using (207)Pb NMR of solid lead nitrate was developed to determine the temperature of magic-angle spinning (MAS) NMR probes over a range of nominal set temperatures and spinning speeds. Using BioMAS and FastMAS probes with typical sample spinning rates of 8 and 35 kHz, respectively, empirical equations were devised to predict the respective sample temperatures. These procedures provide a straightforward recipe for temperature calibration of any MAS probe.     

A comparison among optical emission spectroscopic methods of determining electron temperature in low pressure argon plasmas

In this article, four kinds of optical emission spectroscopic methods of determining electron temperature are used to investigate the relationship between electron temperature and pressure in the cylindrical plasmas of dc glow discharges at low pressures in laboratory by measuring the relative intensities of ArI lines at various pressures. These methods are developed respectively on the basis of the Fermi--Dirac model, corona model, and two kinds of electron collision cross section models according to the kinetic analysis. Their theoretical bases and the conditions to which they are applicable are reviewed, and their calculation results and fitting errors are compared with each other. The investigation has indicated that the electron temperatures obtained by the four methods become consistent with each other when the pressure increases in the low pressure argon plasmas.     

Interaction of BSA with proflavin: A spectroscopic approach

The interaction of bovine serum albumin (BSA) with proflavin was investigated by spectroscopic tools like absorption and fluorescence spectroscopy as well as laser flash photolysis. Absorption spectroscopy proved the formation of ground-state BSA-proflavin complex. Proflavin was found to quench the intrinsic fluorescence of BSA via static quenching. High value of quenching constant suggested that energy transfer occurred from BSA to proflavin. Distance between the fluorophore in the protein and the ligand (proflavin) was evaluated. Binding constant and number of binding site were determined for proflavin-BSA interaction both in phosphate buffer (pH∼6.8) and in sodium dodecylsulphate media. The values of the thermodynamic parameters suggested that the key interacting forces are van der Waal's interaction and hydrogen bonding. Laser flash photolysis study reconfirmed the formation of complex between BSA and proflavin.