spectral lines信息详情
光谱线
spectral───adj.[光]光谱的；幽灵的；鬼怪的
lines───v.排成一行；画线于（line的三单形式）；n.线；台词；航线（line的复数）；n.(Lines)人名；(英)莱恩斯
spectral efficiency───频谱效率
spectral resolutions───[遥感][光]光谱分辨率，[光]谱分解
spectral radius───[数]谱半径
fault lines───断层线；故障线路；n.裂纹线( fault line的名词复数 )
cheesy lines───俗套的对白
agonic lines───[地物]无偏线；无磁差线
chat lines───n.聊天热线
I want you to notice that this spectrum is interrupted by dark lines called spectral lines.───我想让你们注意到的是，这一光谱是被叫做光谱线的暗线所打断的。
Spectroscopy is basically the study of spectra and spectral lines of light, and specifically for us, the light from stars.───光谱学基本上是一种研究光谱和光谱线的学科，特别对我们来说，是研究恒星发出的光。
A British astronomer was analyzing a spectrograph of sunlight, and he noticed a particular pattern of spectral lines that didn't match anything in the library.───一位英国天文学家在分析一台太阳光摄谱仪时，注意到一种特殊的光谱线模式，它与图书馆里的任何一种都不匹配。
I want you to notice that this spectrum make it interrupted by dark line called spectral lines.───我想让你们注意到这个打断了光谱的黑线，这就是光谱线。
Kind of like a chemical finger print of spectral lines for that element appears.───一个化学元素的样式就被光谱线显现出来了。
I want you to notice that this spectrum is interrupted by dark lines, called spectral lines.───我希望你们注意到这个光谱被叫做光谱线的黑线打断。
Working conditions of the instrument and selection of suitable analytical spectral lines for the elements were studied and optimized.───对仪器的工作条件和各元素分析谱线的选择进行了试验和优化。
Spectroscopy is basically study of spectra and spectral lines of light.───光谱学是研究光线的光谱和光谱线的。
Secondly, the selective elimination of the spectral lines is obtained by varying the amplitudes and phases of the trichromatic components.───其次，通过改变三色场的振幅和相位可实现谱线的选择性消除。
They also studied the spectral lines from hot iron atoms that whirl around in a disk just beyond the neutron stars' surfaces at speeds reaching 40 percent light speed.
The spectral interferences from zirconium to the spectral lines of the elements determined were investigated and corrected by the matrix matching and background correction methods.
Still other spectral lines hint at outflowing jets and winds, generated when magnetic fields threading the disk fling some of the inflowing disk material back out.
Thus, the nonthermal broadening in the stars' spectral lines above has been explained abstractly by the theory of spectral lines broadening in plasmas.
Hot ionised gases, and the impurities they contain, also produce spectral lines that are characteristic of the plasma temperature.
The occurrence of discrete spectral lines can be decided by means of real spectral characteristic of complete symmetrical window.
For Rhodamine 6G two spectral lines of laser output is separated from each other by up to about 250A.
Balmer had been thinking about the spectral lines from hydrogen.
Spectroscopic measurements in 1960 indicated that small-scale motion of the plasma was producing the doppler broadening of the spectral lines.