S - spectra 中文

spectra n.spectrum 的復數。

n. spectrum 的復數。 “absorption spectra“ 中文翻譯：吸收波譜“age spectra“ 中文翻譯：年齡譜“aliasing spectra“ 中文翻譯：混淆頻譜“atomic spectra“ 中文翻譯：原子光譜“auroral spectra“ 中文翻譯：極光光譜“bodywave spectra“ 中文翻譯：體波譜“brocken spectra“ 中文翻譯：峨嵋光“bubble spectra“ 中文翻譯：氣泡分布“characteristic spectra“ 中文翻譯：特征光譜“detectable spectra“ 中文翻譯：可檢測譜線“dielectric spectra“ 中文翻譯：介電譜“difference spectra“ 中文翻譯：示差光譜“differential spectra“ 中文翻譯：差不譜; 差光譜; 差示光譜“electronic spectra“ 中文翻譯：電子能譜“emanation spectra“ 中文翻譯：輻射光譜“emission spectra“ 中文翻譯：發射光譜“epr spectra“ 中文翻譯：電子順磁共振譜“euro spectra“ 中文翻譯：歐洲鳥瞰“excitation of spectra“ 中文翻譯：光譜激發“excitation spectra“ 中文翻譯：激發光譜“flame spectra“ 中文翻譯：火焰光譜“force spectra“ 中文翻譯：載荷譜計算法“fortification spectra“ 中文翻譯：閃光暗點“wave spectra“ 中文翻譯：波譜“spectra at high and low temperatures“ 中文翻譯：高低溫光譜“spectorgraph“ 中文翻譯：攝譜儀

spectral
Good spectra of the spiral nebulas are difficult to obtain because of their extreme faintness . 旋渦星云因為非常暗，難以得到它們的清晰的光譜。
Experimental configurations for measuring and displaying these spectra are sketched in figure 13.7 . 測量和顯示這幾種頻譜的實驗裝置見圖13.7。
It includes the stipulation that the phase spectrum over that range should be a straight line . 它包括了在該范圍上相位譜應為直線的規定。
We begin to see, from this material, how to visualize a waveform from its spectrum . 從這些分析中初步看到，如何從它的譜構思出該波形來。
Motion of a star across the line of sight causes no change in its spectrum . 恒星橫越視線方向的運動，在它的光譜中不會引起什么變化。
It is possible to describe the excitation spectra in terms of elementary modes of excitation . 可以借助于基本激發模式來描述激發譜。
Trade integration is part of the larger spectrum of types of economic integration . 貿易一體化是范圍較大的各種經濟一體化的一部分。
Several different names have emerged to characterize different parts of the spectrum . 幾個不同的名稱用來表示電磁波譜的不同部分。
A star that has this kind of spectrum reveals at once something of its structure . 具有這種光譜的恒星，馬上就展示出它的一些結構。
This relation between the frequency and the field spectra was noted experimentally . 實驗上已經發現頻率和場頻譜之間的這種關系。
It was surprising when the alkali spectra showed unmistakable doublets . 當堿金屬光譜顯示出不容懷疑的雙線結構時，是令人驚奇的。
The range of the spectrum in which heat is radiated mostly lies within the infrared portion . 輻射熱的光譜段大部分落在紅外區。
These clouds show spectra remarkably similar to those of the illuminating star . 這些云的光譜與照射它的亮星的光譜極其相似。
In practice the identification of lines in a star's spectrum is not so easy . 實際上，要辨認恒星光譜中的譜線并不那么容易。
At the same time broaden the spectrum as result of energy loss fluctuations . 與此同時，電子譜由于能量損失的漲落而展寬。
White light can be split by a prism into a whole spectrum of wavelengths . 白光可以用棱鏡分解成具有各種波長的整個光譜。
The electromagnetic spectrum covers an enormous range of frequencies and energies . 電磁波譜包括極大的頻率和能量范圍。
If the stellar spectrum is known, the albedo of the dust can be obtained . 如果恒星的光譜已知，就可得出塵埃的反照率。
A particular spectrum line corresponds to a certain definite light wavelength . 某特定的譜線就代表一個確定光的波長。

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spectra

spectra n.spectrum 的復數。

spectral

Good spectra of the spiral nebulas are difficult to obtain because of their extreme faintness . 旋渦星云因為非常暗，難以得到它們的清晰的光譜。

Experimental configurations for measuring and displaying these spectra are sketched in figure 13.7 . 測量和顯示這幾種頻譜的實驗裝置見圖13.7。

It includes the stipulation that the phase spectrum over that range should be a straight line . 它包括了在該范圍上相位譜應為直線的規定。

We begin to see, from this material, how to visualize a waveform from its spectrum . 從這些分析中初步看到，如何從它的譜構思出該波形來。

Motion of a star across the line of sight causes no change in its spectrum . 恒星橫越視線方向的運動，在它的光譜中不會引起什么變化。

It is possible to describe the excitation spectra in terms of elementary modes of excitation . 可以借助于基本激發模式來描述激發譜。

Trade integration is part of the larger spectrum of types of economic integration . 貿易一體化是范圍較大的各種經濟一體化的一部分。

Several different names have emerged to characterize different parts of the spectrum . 幾個不同的名稱用來表示電磁波譜的不同部分。

A star that has this kind of spectrum reveals at once something of its structure . 具有這種光譜的恒星，馬上就展示出它的一些結構。

This relation between the frequency and the field spectra was noted experimentally . 實驗上已經發現頻率和場頻譜之間的這種關系。

It was surprising when the alkali spectra showed unmistakable doublets . 當堿金屬光譜顯示出不容懷疑的雙線結構時，是令人驚奇的。

The range of the spectrum in which heat is radiated mostly lies within the infrared portion . 輻射熱的光譜段大部分落在紅外區。

These clouds show spectra remarkably similar to those of the illuminating star . 這些云的光譜與照射它的亮星的光譜極其相似。

In practice the identification of lines in a star's spectrum is not so easy . 實際上，要辨認恒星光譜中的譜線并不那么容易。

At the same time broaden the spectrum as result of energy loss fluctuations . 與此同時，電子譜由于能量損失的漲落而展寬。

White light can be split by a prism into a whole spectrum of wavelengths . 白光可以用棱鏡分解成具有各種波長的整個光譜。

The electromagnetic spectrum covers an enormous range of frequencies and energies . 電磁波譜包括極大的頻率和能量范圍。

If the stellar spectrum is known, the albedo of the dust can be obtained . 如果恒星的光譜已知，就可得出塵埃的反照率。

A particular spectrum line corresponds to a certain definite light wavelength . 某特定的譜線就代表一個確定光的波長。