共查询到20条相似文献，搜索用时 93 毫秒
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光纤是LAMOST子系统焦面仪器的四个主要组成部分之一。它是LAMOST望远镜收焦的星光从焦面到光谱仪的传输介质。尽可能高的传输效率是我们追求的目标。LAMOST的光纤采用芯径320μm的STU光纤。我们在实验室对其性能作了初步测试。结果令人满意。 相似文献
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光纤时间传输及相位补偿 总被引：2，自引：0，他引：2
介绍了国外几种利用光纤进行时间频率传递的方法和经验.对无补偿光纤时间频率传递方法、双向时间频率传递方法、光学机械温度补偿方法及电子共轭相位补偿方法作了较详细的描述.光纤时延主要随温度而变化,在200 km以内,时延的日变化为几纳秒,月变化为十几纳秒.在50 km内利用光纤传输100 MHz频率信号时,在不补偿情况下频率稳定度为: 3×10-14/s,1×10-15/d;光学补偿后的频率稳定度可达到1.5×10-14/s,1×10-17/d.电子共轭相位补偿后,温度变化20℃引起的相位变化降低了45倍.光纤传输对短期频率稳定度影响较小,对日及更长期的频率稳定度影响较大. 相似文献
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光纤光谱的效率损失主要来源之一是光纤的焦比退化,并且往往还在光谱成像时因焦比退化产生环形出射斑,从而使得光纤传输效率降低,并影响色散之后的谱线轮廓。实验获取郭守敬望远镜调试阶段的大芯径光纤因焦比退化产生的出射环型斑貌,结合CCD光谱图像特点实施轮廓拟合抽谱方法,把二维CCD光谱图像转换成一维光谱,选取望远镜红端数据进行模拟,采样点在500~600 nm波段范围,在该波段中有铁的发射线。通过与获得的环形斑轮廓卷积研究焦比变化对铁发射线峰的影响。最后,正确阐明在正式巡天观测时主镜前悬挂平场漫反射屏消除环形斑引发的偏差的效果。 相似文献
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设计了一款1.5 GHz的稳相频标传输装置,具有实时和事后补偿能力,并且兼容了同轴电缆和光纤两种传输介质.对装置的稳相原理和性能进行了分析和评估,然后对同轴电缆稳相系统的性能进行了测试.结果表明,基于目前的测试环境,与未稳相时相比,实时补偿模式可以改善相位变化112倍以上,积分时间长于7 s时,频率稳定度明显提升,长于60s的频率稳定度有1个数量级的改善;事后补偿模式可以改善40倍相位波动,积分时间长于2.5 s频率稳定度明显提升,长于40 s的频率稳定度有1个数量级的改善.对于更长时间积分的频率稳定度,实时和事后补偿模式均可以改善1.5个数量级以上,装置能有效抑制因传输介质的温度系数等因素导致的缓慢伸缩效应. 相似文献
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A. M. Mickaelian 《Astrophysics》2004,47(3):361-377
Results of spectral observations of 66 objects from the BIG (Byurakan IRAS Galaxies) sample made with the 1.93 m telescope at the Observatoire de Haute Provence (OHP, France) are presented. Emission lines are observed from 64 of the galaxies. The red shifts are determined, the radial velocities, distances, and absolute stellar magnitudes are calculated, the spectrum line parameters are determined, diagnostic diagrams are constructed, the objects are classified according to activity type, and their IR and far-IR luminosities are calculated. Of the 66 objects (corresponding to 61 IRAS sources), 6 are Sy2, 2 are LINERs, 8 are AGN (Sy2 or LINER), 10 are composite, 34 are HII, and 4 are Em of undetermined type. It is calculated that IRAS 07479+7832= BIG d141a is a ultraluminous IR galaxy (ULIG), and 21 are LIG. Spectra of several of the galaxies being studied are presented. 相似文献
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Beata Mazur Janusz Kaluzny Wojciech Krzemi&#;ski 《Monthly notices of the Royal Astronomical Society》1999,306(3):727-735
We report the results of a CCD search for short-period variables in the field of a southern globular cluster NGC 6362. We identified 19 new candidate variables, five of which are cluster RR Lyraes, four are probable SX Phe-type stars and eight are eclipsing binaries. Of the discovered binaries, three are EA-type systems, two of which are located on the cluster CMD in the turn-off region and the third 1 mag above the turn-off point, in the yellow straggler region. Five other systems are of W UMa type, three of which are foreground objects and two are likely cluster members. The remaining two candidates exhibit a modulation of the brightness level with an amplitude of 0.1–0.2 mag; further observations are needed to reveal the nature of their variability. Phased VI light curves for 20 variables (18 RR Lyrae stars and two blue stragglers) located in the central region of the cluster are presented. 相似文献
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Results of spectral observations of 45 objects from the BIG sample (corresponding to 35 IRAS sources) obtained on the 2.6-m
telescope at the BAO are reported. Emission lines are observed for 42 galaxies, 1 object is an absorption galaxy, and 2 turned
out to be stars. The red shifts are determined, the radial velocities, distances, sizes, and absolute stellar magnitudes are
calculated, the parameters of the spectral lines are determined, the objects are classified according to their activity type,
and the IR and far IR luminosities are calculated. Of the 42 emission galaxies, 1 was type Sy2, 2 were LINERs, 1 was an AGN
(Sy2 or LINER), 4 were composite, 25 were HII (including 6 with nuclear star-formation activity), and 9 were Em of undetermined
type (3 of which may be AGN). Calculations show that 23 of the objects are LIG. A physical coupling is discovered for 9 multiple
systems. Spectra of some of the galaxies are shown.
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Translated from Astrofizika, Vol. 49, No. 1, pp. 23–40 (February 2006). 相似文献
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物态方程一直是恒星模型理论研究中的最重要的物理方程之一，对于日震学等高精度要求的研究领域来讲，只包含理想效应的物态方程并不能满足研究需要，而要更细致、包含非理想效应的物态方程对系统作更精确和完善的描述，在弱耦合及弱电子简并的系统中，为研究各种带电粒子之间的库仑耦合效应，以化学图像为基础，分别用具有硬核改正的Debye—Hueckel扩展理论来处理离子-电子作用、多体作用的经典点粒子相互作用理论描述离子-离子作用和量子统计方法处理电子-电子作用，并把此3种作用对物态方程自由能的贡献用半解析的数学公式给出，为适应日震学研究的要求，特别选取一组类太阳的恒星模型作为研究对象，从实际模型计算出发，对库仑耦合中的各种效应进行了比较分析，讨论并检验了所作的理论改进。 相似文献
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恒星临边昏暗系数的测定 总被引：2，自引：0，他引：2
介绍一种新的一级挖和二级近似描述恒星大气临边昏境现象方法,其临边昏境系数可通过有关物理量的直接测量或测量流量和辅助量恒星表面温度的方法间接给出。与太阳观测比较和数值模型大气方法比较,均显示新方法能够以很精确的方式描述恒星临边昏境关系,或确定其相应系数 方法对太阳观测的１７６个数据比较了统计方差,其中直接法的一级挖和二级挖分别为０．３８％和０．２６％;间接法的方差与此相近而略大;与数值模型大气比较其 相似文献
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Machine-learning algorithms are applied to explore the relation between significant flares and their associated CMEs. The
NGDC flares catalogue and the SOHO/LASCO CME catalogue are processed to associate X and M-class flares with CMEs based on
timing information. Automated systems are created to process and associate years of flare and CME data, which are later arranged
in numerical-training vectors and fed to machine-learning algorithms to extract the embedded knowledge and provide learning
rules that can be used for the automated prediction of CMEs. Properties representing the intensity, flare duration, and duration
of decline and duration of growth are extracted from all the associated (A) and not-associated (NA) flares and converted to
a numerical format that is suitable for machine-learning use. The machine-learning algorithms Cascade Correlation Neural Networks
(CCNN) and Support Vector Machines (SVM) are used and compared in our work. The machine-learning systems predict, from the
input of a flare’s properties, if the flare is likely to initiate a CME. Intensive experiments using Jack-knife techniques
are carried out and the relationships between flare properties and CMEs are investigated using the results. The predictive
performance of SVM and CCNN is analysed and recommendations for enhancing the performance are provided. 相似文献
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It is logically possible that early two-body relaxation in simulations of cosmological clustering influences the final structure of massive clusters. Convergence studies in which mass and spatial resolution are simultaneously increased cannot eliminate this possibility. We test the importance of two-body relaxation in cosmological simulations with simulations in which there are two species of particles. The cases of two mass ratios, √2:1 and 4:1, are investigated. Simulations are run with both a spatially fixed softening length and adaptive softening using the publicly available codes gadget and mlapm , respectively.
The effects of two-body relaxation are detected in both the density profiles of haloes and the mass function of haloes. The effects are more pronounced with a fixed softening length, but even in this case they are not so large as to suggest that results obtained with one mass species are significantly affected by two-body relaxation.
The simulations that use adaptive softening are less affected by two-body relaxation and produce slightly higher central densities in the largest haloes. They run about three times faster than the simulations that use a fixed softening length. 相似文献
The effects of two-body relaxation are detected in both the density profiles of haloes and the mass function of haloes. The effects are more pronounced with a fixed softening length, but even in this case they are not so large as to suggest that results obtained with one mass species are significantly affected by two-body relaxation.
The simulations that use adaptive softening are less affected by two-body relaxation and produce slightly higher central densities in the largest haloes. They run about three times faster than the simulations that use a fixed softening length. 相似文献
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自适应光学技术应用于激光测月中大气波前倾斜量的探测与计算 总被引：2，自引：0，他引：2
针对云南天文台1.2米望远镜在激光测月中回波光子数太少的问题，将大气湍流效应考虑到激光测月中，研究了互相关和绝对差分两种跟踪算法的原理，并编写了算法程序，利用太阳数据验证了程序的正确性,给出了根据所采集的月面感兴趣区域的图像数据，用不同方法在不同条件下处理所得的大气波前整体倾斜信号，比较了算法的优劣。 相似文献