光谱线

研究了硼元素光谱线的特性及其光谱干扰，建立了不须分离干扰元素和不充氮条件下，直接测定高温合金中微量硼元素的ICPAES法

Character of spectral line with B element , and its spectral interference were studied In condition without separating interference element and filling N , ICP AES method was adopted to determine trace element B in high temperature alloy

恒星光谱线的跃迁系数和能源函数

The transition coefficients and source function for stellar spectral line

类钴氙离子入射Ni表面激发的红外光谱线和X射线谱

Cobalt-like-Xe-induced infrared light and x-ray emission at Ni surface

同时观察到最高阶为四阶的Stokes光谱线。

Also the fourth order Stokes spectral line is observed . 3 .

激光等离子体镁光谱线Stark展宽的测量与计算

Measurment and calculation of Stark broadening of Mg spectral lines in laser plasma

高电荷态离子入射Ta表面形成的靶原子的特征光谱线

The characteristic spectral lines induced by the impact of highly charged ion on Ta solid surface

~（126）Xe~（q+）轰击Al表面产生的原子和离子光谱线

Atomic and Ion ′ s Light Emission Spectra Induced by the Impact of ~ ( 126 ) Xe ~ ( q + ) on Al Solid Surface

应用离轴的F-P扫描干涉仪对快束光谱线的都普勒展宽进行补偿

Application of an off-axis Fabry-Perot scanning interferometer for compensating Doppler broadening in fast-beam spectroscopy

理论和实验上研究了多频相位调制产生等幅光谱线并将其应用在光纤传输系统中的受激布里渊散射抑制（SBS）。

The method of generating equal-amplitude spectral lines by multi-frequency phase modulation is used in stimulated Brillouin scattering ( SBS ) suppression .

ICP-AES中光谱线及其相互干扰的计算机模拟&Ⅴ模拟程序及谱线数据库

Computer simulation of emission spectra and spectral interferences in inductively coupled plasma atomic emission spectrometry ⅴ . the computer programme and spectral database

SIH4激光等离子体氢光谱线的加宽机制

Study on the broadening mechanism of H spectral lines in SIH_4 laser Plasma

精确测定光谱线峰光强新途径的探索

A new approach of precisely measuring peak intensities of spectral lines

此后又发现了氢原子的其他光谱线系。

Other series spectra for hydrogen have since been discovered .

他发现光谱线在磁场中分裂了。

And he found line splitting in the magnetic field .

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

从而估计出有光谱线出现激光的可能性。

So that we can estimate the possibility that spectrum can produce laser .

较重的原子具有较复杂的光谱线。

The larger atoms have much more complex spectra .

激光烧蚀铜产生原子和离子光谱线的研究

Studies on Atomic and Ion Emission Spectrum Produced by Pulsed laser Ablation of Copper

影响光谱线的积分强度的因素

Factors affecting the integral intensity of spectral lines

太阳光谱线的形成深度

The Depths of Formation of Solar Spectral Lines

我国土壤光谱线之研究

Research of China 's Soil Spectral Line

不同的光谱线分布意味着星体有不同的化学性质。

And so different sets of chemical line mean the star have different chemical compoisition .

原子光谱线增宽的原因

Several Reasons for Atomic Spectral Line Broadening

本文对引起恒星光谱线加宽的物理机制作了回顾。

The historical retrospect of physical mechanisms of spectral lines broadening in stars is presented .

太阳光谱线的快速变化

The Rapid Variations of Solar Spectral Lines

一种光谱线库通过火焰测试累积起来。

Well , a kind of spectroscopic library of elements was compiled using flame tests .

原子光谱线位移机理的研究

Wavelength Shift of Atomic Spectral Lines

我想强调一点，这条光带被暗光带中断，称作光谱线。

I want to notice this spectrum is interrupted by dark lines , called spectrum lines .

但是这些光谱线会在不同的地方断裂，形成不同的模式。

But the spectral lines would break it up at different places , making different patterns .

这样，寻求新的理论解释恒星光谱线的加宽成为必要。

So it is necessary to seek new theories to explain the spectral lines broadening of stars .