太阳光谱

利用该模型计算了FeⅠ1.56μm红外太阳光谱的分光流量，分析了实验观测的可行性及改进方案。

The spectral flux of Fe ⅰ 1.56 μ m infrared solar spectrum is calculated by using the model . The feasibility of the infrared observation on the current experiment platform and the reform methods are analyzed .

这些光电转换体系通常采用TiO2、ZnO等宽带隙半导体作为其基本构成材料，但是这些宽带隙材料本身并不具有对占太阳光谱主要区域的可见光的吸收能力。

In general , these photoelectric conversion systems usually use TiO2 , ZnO and other wide bandgap semiconductors as the basic components . However , these wide bandgap semiconductors do not absorb visible light which occupy a large proportion of the solar spectrum .

O3，CO2浓度及太阳光谱变化对作物光合作用影响的数值模拟研究

Numerical simulation of the influence of o_3 , co_2 and spectrum variation on the photosynthesis of crop canopy

通过数值模拟，考察了大气气溶胶对AVHRR通道1,2和整个太阳光谱区的行星反照率和地面反照率的影响，并研究了气溶胶对行星反照率和地面反照率之间关系的影响。

Through numerical simulations the effects of atmospheric aerosols on the planetary and surface albedos and the relationship between them in the AVHRR channels 1 and 2 and the whole solar spectral region from 0.2 to 3.58 μ m are investigated .

这些窄带隙共轭聚合物展现了宽的吸收光谱（350nm-850nm），能有效地与太阳光谱匹配，提高太阳光采集率。

These narrow-band-gap conjugated polymers show a wide absorption spectrum ( 350nm-850nm ), can effectively cover the solar spectrum to improve the collection rate of the sun .

测试结果表明，加各种膜卤钨灯的色温变化不大，均为3000K左右，故利用加膜卤钨灯来模拟太阳光谱是不可行的。

As a result , we conclude that it is improper that the spectrum of the Halogen-lamp of covered films is used by simulating the spectrum of the solar radiation because it is about 3000K that the color-temperature of the Halogen-lamp have vary films .

探讨高稳定性、高性能、低成本的太阳光谱选择吸收光热转换涂层制备方法和机理。本论文首先研究了射频反应磁控溅射工艺参数对Ti-O系薄膜的结构和紫外光-可见光吸收性质的影响。

The preparation method and mechanism of solar selective absorbing films with high stability , high performance , low cost have been discussed . Firstly , the influence of RF reactive magnetron sputtering technology process parameters on the structure and absorption UV and visible spectrum of Ti-O films were discussed .

空气中NO2浓度的太阳光谱法测量研究

Measurement of NO_2 Concentration in the Atmosphere by Sun Spectroscopy Method

太阳光谱方法测量成都地区大气二氧化氮浓度

Measurement of NO_2 Concentration in Atmosphere in Chengdu by Solar Spectra

太阳光谱绝对测量中的数据采集系统设计

Design of Data Collecting System of the Solar Spectral Intensity Monitor

太阳光谱方法和多云模型应用研究总结

Summary on solar spectral methods and application studies of multi-cloud model

关于太阳光谱的构成，我们已了解不少。

We have known much of the constitution of the solar spectrum .

太阳光谱选择性吸收表面光学性能计算

Optical property calculations of multilayer stack models for solar selective absorbing surfaces

太阳光谱线轮廓在日面上的变化和宁静太阳大气模型

Center-to-limb variation of spectral lines and quiet sun atmospheric model

新型太阳光谱选择性吸收涂层的热稳定性

Study on thermal stability of solar selective absorbing surfaces with new material

绿色太阳光谱反射涂层的性能研究

Research on the Property of Green Solar Spectral Reflective Coat

太阳光谱望远镜仪器轮廓的测定

Determination of the Instrument Profile of the Solar Spectrum Telescope

实验结果给出了模拟光谱与太阳光谱曲线的对比图，并利用评价函数对模拟结果进行评价。

The comparison charts and evaluation function are given in the experimental results .

氮化钛太阳光谱选择性吸收薄膜研究进展

Research Progresses on TiN Solar Spectroscopic Selective Absorbing Film

二维太阳光谱观测方法和技术

The Methods and Techniques of Solar 2D Spectral Observations

太阳光谱中的磁场敏感谱线

Magneto - sensitive lines in the solar spectrum

太阳光谱中布喇开γ线的斯塔克效应

Stark effect in Brackett γ of solar spectrum

中高温太阳光谱选择性吸收涂层的研制

Preparation and Characterization of Solar Selective Absorbing Coatings for Medium & High Temperature Application

太阳光谱线的形成深度

The Depths of Formation of Solar Spectral Lines

太阳光谱吸收率的测量

Research in measurement of solar spectral absorptance

太阳光谱望远镜鬼线强度测量方法及初步结果

Measuring Method and Preliminary Results of the Ghost Line Intensity for the Solar Spectral Telescope

从反射太阳光谱反演大气气溶胶体积谱分布的理论研究

The theoretic study on the retrieval of aerosols ' volume distribution from solar spectral reflectance

荒漠地区直接太阳光谱的测量

Direct solar spectral measurements in desert range

太阳光谱线的快速变化

The Rapid Variations of Solar Spectral Lines

云台凤凰山太阳光谱最佳观测时间讨论

Discussion on the Optimal Duration of Solar Spectral Observation at the Phoenix Mountain of Yunnan Observatory