禹城地区光合有效辐射的计算方法

利用2005年7月-2006年10月在山东禹城对太阳辐射（包括光合有效辐射PAR、可见光辐射VIS、总辐射Q等）、气象要素等进行的4次综合观测资料,初步得到了朋R,VIS的日、季节变化特征并对其进行了分析,结果表明：各辐射的小时累计之比vIS／Q,PAR／Q,PAR／VIS相对稳定,其平均值分别为0．39,1．95（mol／MJ）,4．97（mol／MJ）,但它们均有明显的日、逐日、季节变化,并受水汽、气溶胶、云等因素的影响。同时建立了实际天气PAR,VIS的小时累计经验公式及其转换关系,计算值与观测值均比较接近。当考虑水汽和散射因子时,PAR,VIS的计算值与观测值的相对偏差分别为11．1％,10．6％。限于实际情况,可以只考虑水汽因子的作用来计算PAR和VIS的小时累计值,它们的相对偏差分别为13．3％,12．6％。水汽因子对于PAR,VIS的传输和计算具有重要作用。     

The Solar Optical Telescope of Solar-B (Hinode): The Optical Telescope Assembly

The Solar Optical Telescope (SOT) aboard the Solar-B satellite (Hinode) is designed to perform high-precision photometric and polarimetric observations of the Sun in visible light spectra (388 – 668 nm) with a spatial resolution of 0.2 – 0.3 arcsec. The SOT consists of two optically separable components: the Optical Telescope Assembly (OTA), consisting of a 50-cm aperture Gregorian with a collimating lens unit and an active tip-tilt mirror, and an accompanying Focal Plane Package (FPP), housing two filtergraphs and a spectro-polarimeter. The optomechanical and optothermal performance of the OTA is crucial to attain unprecedented high-quality solar observations. We describe in detail the instrument design and expected stable diffraction-limited on-orbit performance of the OTA, the largest state-of-the-art solar telescope yet flown in space.     

俄罗斯高温高压处理钻石特征

采用显微观察、红外光谱、可见吸收光谱和低温光致发光谱等分析方法,对9颗俄罗斯高温高压处理钻石样品进行了研究。结果表明,该类钻石样品的内部多见石墨化现象,尤以彩色钻石样品更明显;金黄色、紫红色、黄绿色样品为ⅠaAB型,浅黄色样品为ⅠaB型,近无色样品为Ⅱa型;样品的可见吸收光谱因颜色不同而差异显著,其中金黄色样品可见475 nm处的吸收宽带,紫红色样品可见638,614,595 nm处的吸收峰,黄绿色和浅黄色样品可见415,475,503 nm处的吸收峰,近无色样品则为较光滑的平直曲线。此外,该类样品在低温光致发光谱中可见575 nm与637 nm处强发光峰。这些特征为探讨该类钻石的晶格缺陷与呈色机理提供了一定的科学依据。     

基于遗传自组织神经元网络的可见光与热红外遥感数据融合方法

提出了一种融合方法,充分发掘可见光数据高空间分辨率和热红外数据高时间分辨率的特点,在由可见光数据估算的地表参量与热红外数据间,通过遗传自组织神经元网络建立非线性融合方法,最终获得高空间、高时间分辨率的地表温度数据,并利用ASTER卫星产品数据对该方法进行了验证。结果表明,该方法简便易行,精度较高,为快速获取高分辨率地表温度分布提供了一条新途径。     

具有图像内容保持特性的小波域可见水印

根据图像的噪声掩蔽性设计了一种小波域可见水印算法，并根据水印图像的纹理特征对算法作了进一步改进。在此基础上，提出了具有内容保持的嵌入策略及改进算法。实验结果表明，该算法在保证水印具有较好可见性的同时，载体图像内容得到了保持。     

内蒙古白乃庙金矿床石英脉中绢云母可见光光谱特征及其地质意义

以简单、经济的可见光吸收光谱方法研究了绢云母可见光光谱特征,结果表明含矿石英脉中绢云母可见光光谱在650~700nm之间透射率高,并总结了透射率与Fe含量和寄主脉金品位之间的关系。·     

Double-camera measurements of plumes, applied to wind field characterization and dispersion studies

A stereophotogrammetric technique based on standard equipment to measure plume trajectories in sheared wind fields and/or complex terrain is shown here. The approach is to use existing visible plumes as tracers of opportunity of air flow. This technique was first developed as part of a multi-instrument field program intended for the experimental characterization of atmospheric dispersion in the complex coastal area of Bilbao in northern Spain. Emphasis is placed on the calibration method and the experimental procedures as well as on sources and margins of error. Finally, applications and joint usage with other techniques during several field programs are also presented.     

The NO2 absorption spectrum. II. Absorption cross-sections at low temperatures in the 400–500 nm region

With improved experimental conditions already used for measurements at ambient temperature (Mérienneet al., 1994), new values have been found for the absorption cross-sections of NO₂ at 240 and 220 K in the 400–500 nm spectral region. Using a better resolution than in previous studies we show that the temperature effect is not negligible and should be taken into account for the optical measurements of atmospheric NO₂ amounts by differential absorption methods.Unité de Recherche Associée au CNRS.     

基于月球反射的遥感器定标跟踪监测

月亮辐照度是可见近红外波段一种稳定的辐射参考基准,对月观测已成为星载遥感仪器辐射定标和验证的一种新方法。风云三号03星(FY-3C)中分辨率光谱成像仪(Moderate Resolution Spectral Imager,MERSI)增加了对月观测功能,改进了太阳反射波段的在轨辐射定标。本文收集分析了MERSI在轨工作以来的全部11组对月观测数据,利用通道间辐照度比值方法移除月相角,日—月—星相对距离等因素对月亮辐照度观测值的影响,开展了可见光近红外波段的辐射定标工作,实现了MERSI太阳反射通道的辐射定标系数动态跟踪和评估。通过线性回归及统计发现,通道8辐射响应的年衰减率达到了14.55%,通道9达到了8.42%,通道1、6、10、11、16和19的年衰减率为1.15%—4.72%,其余通道未检测到衰减。研究结果可以用于订正MERSI数据的辐射定标系统性偏差,提高MERSI全寿命期的辐射定标精度。     

HyLogger-3, a visible to shortwave and thermal infrared reflectance spectrometer system for drill core logging: functional description

Australian Geological Surveys are the custodians of a major national asset in the form of historically drilled and archived drill cores of the top few kilometres of the continent acquired by government agencies and companies over many decades. The AuScope National Virtual Core Library (NVCL) component of the AuScope Earth Model comprises geological/rock samples, technology, people and database/delivery infrastructure located in six nationally distributed nodes and is aimed at extracting additional value from this asset. The technology components of the NVCL comprise an integrated suite of hardware (HyLogger-3) and software (TSG-Core) systems for the imaging and hyperspectral characterisation of drill cores in their original core trays and the interpretation of their contained oxide, carbonate, hydrous and anhydrous silicate mineralogy. The HyLogger-3 includes state-of-the-art Fourier Transform Spectrometers that continuously measure calibrated spectral reflectance from nominal 10 by 18 mm fields of view. These spectra are in turn passed through a series of automatic and semi-automatic pre-processing and mineralogical unmixing algorithms. These, along with numerous other tools in TSG-Core, output a variety of mineralogical and image products for use by scientists in many branches of the earth sciences. This paper provides a functional overview of the HyLogging hardware and software tools available in each of Australia's Geological Surveys.