青年中文spectral lines的意思
spectral lines中文翻譯：
光譜線
spectral───adj.[光]光譜的；幽靈的；鬼怪的
lines───v.排成一行；畫線于（line的三單形式）；n.線；臺詞；航線（line的復數）；n.(Lines)人名；(英)萊恩斯
spectral efficiency───頻譜效率
spectral resolutions───[遙感][光]光譜分辨率，[光]譜分解
spectral radius───[數]譜半徑
fault lines───斷層線；故障線路；n.裂紋線( fault line的名詞復數 )
cheesy lines───俗套的對白
agonic lines───[地物]無偏線；無磁差線
chat lines───n.聊天熱線
I want you to notice that this spectrum is interrupted by dark lines called spectral lines.───我想讓你們注意到的是，這一光譜是被叫做光譜線的暗線所打斷的。
Spectroscopy is basically the study of spectra and spectral lines of light, and specifically for us, the light from stars.───光譜學基本上是一種研究光譜和光譜線的學科，特別對我們來說，是研究恒星發出的光。
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.───一位英國天文學家在分析一臺太陽光攝譜儀時，注意到一種特殊的光譜線模式，它與圖書館里的任何一種都不匹配。
I want you to notice that this spectrum make it interrupted by dark line called spectral lines.───我想讓你們注意到這個打斷了光譜的黑線，這就是光譜線。
Kind of like a chemical finger print of spectral lines for that element appears.───一個化學元素的樣式就被光譜線顯現出來了。
I want you to notice that this spectrum is interrupted by dark lines, called spectral lines.───我希望你們注意到這個光譜被叫做光譜線的黑線打斷。
Working conditions of the instrument and selection of suitable analytical spectral lines for the elements were studied and optimized.───對儀器的工作條件和各元素分析譜線的選擇進行了試驗和優化。
Spectroscopy is basically study of spectra and spectral lines of light.───光譜學是研究光線的光譜和光譜線的。
Secondly, the selective elimination of the spectral lines is obtained by varying the amplitudes and phases of the trichromatic components.───其次，通過改變三色場的振幅和相位可實現譜線的選擇性消除。
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.