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With this paper we present the mathematical background for a novel method for the deconvolution of longer exposed double star images, merged by seeing and other effects. This method, which was recently presentcd in a short paper (Müller and Geyer 1993) makes use of the autocorrelation of the odd function of the merged, and thus asymmetric two dimensional double star image profile. We give the mathematical evidence that digital filtering during the image processing does not influence the angular distance of the binary components, and that it can be determined independently of the brightness difference of the components. The brightness difference itself can be obtained without ambiguity, if it does not exceed 3 mag, and then the distance has been derived before. We further show that the information content of stellar images is generally less degraded by seeing effects as was previously supposed. Thus closer double stars can be resolved and photometrically deconvoluted by the method. By atmospheric disturbances, telescope guiding errors, optical distortions and silhouetting generally the stellar images on astrometric photographs of modern opto—electronic detectors are asymmetrically deformed. Therefore, the method yields also better accuracy and more adequate results for astrometry, photometry, and also astropspectroscopy.     

基于对象诊断的空间检验方法（MODE）

基于对象诊断的空间检验方法 MODE(Method for Object-Based Diagnostic Evaluation),通过在空间场中识别对象,计算对象的相似度,并最终形成两个场的综合相似度来实现对两个空间场的检验。相对于传统的点对点的检验方法,该方法综合考虑了空间位置、形状、面积等多种因素,并通过符合主观判断的模糊逻辑算法计算相似度,克服了数值预报传统检验方法对于空间位置的过度依赖以及TS评分中的"双重惩罚"等不足。个例研究表明该方法具有明显的优势,有较高的实际应用价值。     

一种基于行人航位推算的改进航迹跟踪算法

针对在未知环境中行人轨迹跟踪问题,提出一种基于行人航位推算的改进航迹跟踪算法,有效实现了在磁场干扰环境下行人轨迹的高精确跟踪.在步数估计中,利用双重阈值二值化算法对加速度数据进行分析,进而获得行人的运动步数;在航向估计中,利用自适应融合算法来获取航向.该融合过程首先根据姿态更新微分方程,将角速度与加速度融合获取一次航向...     

聚乙烯冲击压缩特性实验研究

利用神光Ⅱ装置第九路输出的倍频激光,采用直接驱动方式研究了聚乙烯(CH₂)材料的冲击压缩特性.实验表明聚乙烯冲击波阵面自发辐射较强,冲击波在聚乙烯台阶中的传播比较稳定.采用阻抗匹配方法,以铝作标准材料,测量了聚乙烯的冲击绝热线,聚乙烯冲击压强达0.54 TPa,冲击波速度测量相对扩展不确定度~2%(K=2),实验数据的一致性较好,与已有低压实验数据及状态方程解析模型比较符合.     

光纤传感器在双翻斗雨量传感器超差调整中的应用

双翻斗雨量传感器标校过程中，对于不同雨强超差方向相反的雨量计需要分别调节上翻斗的定位螺钉和计量翻斗的容量调节螺钉，同时也需要记录上翻斗和计量翻斗的翻动次数。雨量计使用的是无源脉冲输出，计量翻斗的每次翻动触发干簧管产生一个脉冲，利用单片机即可采集这个信号自动记录。而上翻斗的翻动次数靠人工观察统计，由于翻斗翻动速度较快人工计数不准确，最终造成标校不准。并且人工每次只能记录1台雨量计，无法批量自动记录数据。本文采用光纤传感器在不干扰雨量计运行情况下自动统计上翻斗翻动次数，为标校提供准确数据。     

浅论富钴结壳柱状构造的成因机制

柱状构造为富钴结壳中多种微观构造类型之一。为探讨富钴结壳柱状构造的形成机制,利用高分辨率电子探针技术分析了位于中太平洋某海山的富钴结壳中柱状构造的微观形态和微区元素化学特征,结果表明,柱状构造是由围绕核心的微层呈弓形外延辐射生长逐渐分枝而成。壳层由亮色、暗色微层交替叠置而成,其中亮色微层富锰、钴、镍和氧,而暗色微层富铁和硅;同一微层各部分的生长速率不同,介于0.27~0.92 mm/Ma。柱状构造壳层亮色、暗色微层交替变化以及相应成分的不同是微观氧化还原环境变化的结果,而柱状构造的分枝和同一微层生长速率的差异则与富钴结壳生长界面有界面双电层有关。     

Measurements of visual double stars with PISCO2 at the Nice 76-cm refractor in 2013–2014 (new data) and in 2015

We present relative astrometric and photometric measurements of visual double stars made in 2013–2015, with PISCO2 installed at the 76-cm refractor of Côte d'Azur Observatory in Nice (France). Our observing list contains orbital couples as well as double stars whose motion is still uncertain. Most of the observations were done in 2015, but some other observations of wide couples were done in 2013–2014 (0.3% of the total of the observations). Three different techniques were used for obtaining measurements: lucky imaging, speckle interferometry and the direct vector autocorrelation method. From our observations of 2837 multiple stars, we obtained 5182 new measurements with angular separations in the range of 0 ${}^{″}$.1–32 ${}^{″}$ and an average accuracy of $0^{″}.018$. The mean error on the position angles is 0°.8. Most of the position angles were determined without the usual 180° ambiguity with the application of the direct vector autocorrelation technique and/or by inspection of the Lucky images or the long integration files. We managed to routinely monitor faint systems ( $m_V\approx 9-11$) with large magnitude difference (up to $\mathrm{\Delta }{m}_V\approx 4.5$). We have thus been able to measure 21 systems containing red dwarf stars that had been poorly monitored since their discovery, from which we estimated the stellar masses thanks to Gaia measurements. We also measured the magnitude difference of the two components of 1079 double stars with an estimated error of 0.2 mag. Except for a few objects that are discussed, our measurements are in good agreement with the ephemerides computed with published orbital elements, even for the double stars whose separation is smaller than the diffraction limit. Thanks to good seeing images and with the use of high-contrast numerical filters, we have also been able to obtain 196 measurements with an angular separation smaller than the diffraction limit of our instrumentation, and consistent with those obtained with larger telescopes. We also report measurements of the 164 new double stars that we found in the files obtained during the observations. Finally, from a study of the DR3 Gaia release, it is shown that all the objects of the Tycho Double Star Catalog that we did not resolve in 2015 are probably false detections by Tycho.     

镉稳定同位素研究进展

Cd具有挥发性和亲硫性,在海洋环境中Cd为微量营养元素,而在生态环境及农业土壤环境中Cd为有毒元素.因此,镉同位素被应用于海洋科学、地球科学、环境科学及农业科学研究,并展现出巨大的应用潜力.本文总结了近年来富含有机质的环境样品、植物样品和生物样品的消解方法,以及Cd分离纯化及双稀释剂校正方法的研究进展.采用微波、高压灰...