微型近红外光谱仪测量北极积雪覆盖海冰内部太阳辐照度可行性研究   总被引：1，自引：1，他引：0  

南立文  王晓萍  王杭州  周宏亮  陈鹰 《海洋学报(英文版)》2020,39(9):115-124

The extremely low temperature, high humidity and limited power supply pose considerable challenges when using spectrometers within the Arctic sea ice. The feasibility of using a miniature low-power near-infrared spectrometer module to measure solar radiation in Arctic sea ice environments was investigated in this study.Temperature and integration time dependences of the spectrometer module were examined over the entire target operating range of –50℃ to 30℃, well below the specified operating range of this spectrometer. Using these observations, a dark output prediction model was developed to represent dark output as a function of temperature and integration time. Temperature-induced biases in the saturation output and linear operating range of the spectrometer were also determined. Temperature and integration time dependences of the signal output were evaluated. Two signal output correction models were developed and compared, to convert the signal output at any temperature within the operating temperature range and integration time to that measured at the reference temperature and integration time. The overall performance of the spectrometer was evaluated by integrating it into a refined fiber optic spectrometry system and measuring solar irradiance distribution in the ice cover with thickness of 1.85 m in the Arctic during the 9th Chinese National Arctic Research Expedition. The general shape of the measured solar irradiance above the snow surface agreed well with that measured by other commercial oceanographic spectroradiometers. The measured optical properties of the sea ice were generally comparable to those of similar ice measured using other instruments. This approach provides a general framework for assessing the feasibility of using spectrometers for applications in cold environments.  相似文献   

Reservoir architecture and heterogeneity distribution in floodplain sandstones: Key features in outcrop,core and wireline logs     

Luis Miguel Yeste  Augusto N. Varela  César Viseras  Neil D. Mcdougall  Fernando García-García 《Sedimentology》2020,67(7):3355-3388

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The Review of γ-ray Astronomical Observing Techniques     

《Chinese Astronomy and Astrophysics》2021,45(3):281-300

$\gamma$-ray is a unique probe for extreme events in the universe. Detecting the $\gamma$-ray provides an important opportunity to understand the composition of universe, the evolution of stars, the origin of cosmic rays, etc. $\gamma$-ray astronomy involves in various frontier scientific issues, and the observed energy spectrum spans over a wide range from a few hundreds of keV to a few hundreds of TeV. Different $\gamma$-ray telescopes are in need for different scientific goals and spectral bands. In this work, 5 kinds of space- and ground-based $\gamma$-ray observing techniques were summarized, including the Coded-aperture telescopes, Compton telescopes, Pair-production telescopes, Imaging Atmospheric Cherenkov Telescopes, and Extensive Air Shower Arrays. The progress in $\gamma$-ray astronomy in the past 70 years, motivated by the observation capability, was reviewed. Great achievements have been made in the high-energy domain and very-high-energy domain, while because of the limited missions conducted, as well as a lower sensitivity comparing with other domains, discoveries in low- and medium-energy are few, and due to the high observation difficulty, as well as the late start, relevant scientific yields in ultra- and extremely-high energy are limited. Moreover, the future planned missions and capabilities of the $\gamma$-ray telescopes and their possible scientific outputs were discussed. Among these missions, low- and medium-energy space telescopes e-ASTROGAM (enhanced-ASTROGAM), AMEGO (All-sky Medium Energy Gamma-ray Observatory), and very-high-energy ground-based arrays LHAASO (Large High Altitude Air Shower Observatory) and CTA (Cherenkov Telescope Array) greatly improve sensitivity than their corresponding last generation, thus expect very likely to further expand our knowledge on the $\gamma$-universe.  相似文献   

综合物化探方法在深冲矿区铀多金属矿勘探中的应用     

何友宇  覃金宁  李竹溢  黄绍琼 《国土资源导刊(湖南)》2015,(1):84-89

通过研究深冲铀矿区γ能谱铀异常、氡浓度异常特征和激电异常特征,探索矿区范围岩体、断裂构造和蚀变带与物化探信息显示特征的关系。据此,结合矿区地质特征,总结物化探方法应用效果,矿致异常综合特征。  相似文献   

Data Analysis of Chang’E-1 Gamma-Ray Spectrometer and Global Distribution of U, K, and Th Elemental Abundances     

ZOU Yongliao  ZHANG Liyan  LIU Jianzhong  MU Lingli  REN Xin  ZHANG Guangliang  CHANG Jin  YAN Jun  ZHANG Nan  ZHANG Hongbo  Lü Chang  LIU Jianjun  ZUO Wei  SU Yan  WEN Weibin  BIAN Wei  WANG Min  XU Chun  LI Chunlai  OUYANG Ziyuan 《《地质学报》英文版》2011,85(6):1299-1309

Gamma-ray spectrometer (GRS) is one of the main payloads on the Chang’E-1 (CE-1) lunar probe, mainly aimed to detect the elemental abundances and distributions on the lunar surface. At 03:58 on 28 November 2007, it performed the first observation of the lunar gamma rays. As of 24 October 2008, 2105?h of effective gamma rays spectra had been acquired by CE-1 GRS, which covers the whole surface of the moon. This paper mainly describes the data processing procedures and methods of deriving the elemental abundances by using the CE-1 GRS time series corrected spectra: first, to bin data into pixels for mapping; then, to perform a background deduction of the cumulative spectra and obtain a peak area of the elements; and finally, to use the elemental abundances inversion model to produce the elemental abundances. Based on these processing methods, the global abundance maps of U, K, and Th at a 5°×5° equal-area pixel are acquired by CE-1 GRS data. The paper gives a preliminary analysis of the uncertainties of the elemental abundances  相似文献   

原子荧光光谱仪在黄金矿山金测定中的应用     

李洪芳  高树林 《吉林地质》2011,30(4):89-92

本文着重介绍了原子荧光光谱仪在黄金矿山中的应用。该仪器与化学法和其它类型的仪器相比较,具有灵敏度高（DL：〈1×10-9）、重现性好（RSD：〈2.0%）、分析速度快等优点。同时简单介绍了目前测定金的一些其它方法,包括原子吸收和发射光谱、化学分析等方法在应用过程中的优缺点和所遇到的情况,论证了原子荧光光谱仪在黄金矿山金...  相似文献   

翡翠与相似玉石及仿制品的仪器鉴定     

李晨 《山东地质》2011,(7):14-16

翡翠和相似玉石及仿制品肉眼下真假难辨,需借助仪器进行鉴定。常规仪器下的鉴定是根据其相关数据和结构特征判定;用红外光谱仪则是根据光谱图特征识别。通过常规仪器和红外光谱仪两种鉴定方式进行比较,得出红外光谱仪能更完全正确地对各类型玉石进行正确判断。  相似文献   

张掖市平山湖地区煤岩层物性规律研究与测井方法应用     

张元基 《中国煤炭地质》2011,(6):59-64

通过对平山湖地区11口井的测井资料进行分析,初步掌握了该区含煤岩层的地球物理特性及其在视电阻率、密度、自然伽马、声波时差、自然电位等测井曲线上的响应特征。总结出一套适合该地区的测井方法,如各种测井参数的数据计算方法与曲线处理技巧,为该类地区使用TYSC-3Q测井仪器进行测井提供了参考依据。针对该地区煤层具有中高阻、低密度、低放射性、高时差、弱自然电位的物性特征,以多个实例介绍了煤层在不同测井参数曲线上的识别方法及定量解释原则。  相似文献   

A Comparison of Four Precipitation Distribution Models Used in Daily Stochastic Models     

LIU Yonghe  ZHANG Wanchang  SHAO Yuehong  ZHANG Kexin 《大气科学进展》2011,28(4):809-820

Stochastic weather generators are statistical models that produce random numbers that resemble the observed weather data on which they have been fitted; they are widely used in meteorological and hydrologi- cal simulations. For modeling daily precipitation in weather generators, first-order Markov chain-dependent exponential, gamma, mixed-exponential, and lognormal distributions can be used. To examine the perfor- mance of these four distributions for precipitation simulation, they were fitted to observed data collected at 10 stations in the watershed of Yishu River. The parameters of these models were estimated using a maximum-likelihood technique performed using genetic algorithms. Parameters for each calendar month and the Fourier series describing parameters for the whole year were estimated separately. Bayesian infor- mation criterion, simulated monthly mean, maximum daily value, and variance were tested and compared to evaluate the fitness and performance of these models. The results indicate that the lognormal and mixed-exponential distributions give smaller BICs, but their stochastic simulations have overestimation and underestimation respectively, while the gamma and exponential distributions give larger BICs, but their stochastic simulations produced monthly mean precipitation very well. When these distributions were fitted using Fourier series, they all underestimated the above statistics for the months of June, July and August.  相似文献   

雨滴谱的变化对降水估计的影响     

吴亚昊  周筠珺  刘黎平 《成都信息工程学院学报》2015,30(2)

针对雨滴谱的变化对降水估计的影响,提出根据激光雨滴谱仪上方雷达回波的结构特征将降水过程划分为对流云降水和层状云降水交替分布5个部分,通过基于2种降水类型的第1种分类Z-R关系、基于5个部分的第Ⅱ种分类Z-R关系和基于整个降水过程的总体Z-R关系分析雨滴谱的变化对降水估计的影响.结果表明:当对流云降水向层状云降水过渡时,指数谱从无到有、多峰谱比例减小,Nw减小、μ增大、Dm变化不大;Mw与R变化相似,当Z增大时μ和Dm分别是递减和递增的;Z-R关系(Z=aRb)中a值变化范围较大、系数b在1～2波动且与层状云阶段相比,对流云阶段的a和b值较小;利用第Ⅱ种分类Z-R关系反演的雨强与基于雨滴谱仪观测数据计算的雨强最接近;雨滴谱仪在层状云阶段的反演效果明显强于对流云阶段,这与对流云降水中雨滴谱信息变化大且快等因素有关.  相似文献