s sa sb sc sd se sf sg sh si sj sk sl sm sn so sp sq sr ss st su sv sw sy

Перевод: spectral

[прилагательное]
призрачный; спектральный

Тезаурус:

1. The Model 1605 is especially suited to the educational laboratory operating over the spectral range 4400-;450 cm -1 .
2. The concept of a dividing line in the H-R diagram was proposed to describe the apparently abrupt disappearance of coronae as stars evolve towards the giant branch at early K spectral type.
3. In spectral terms this means that new frequencies are generated, the main ones being the sum of the strong and weak frequencies are generated, the main ones being the sum of the strong and weak frequencies and their difference.
4. In these conditions spectroscopy of the light emitted from the plasma indicated that the temperature was somewhere between 2 and 5 million K. (The spectroscopists looked at the doppler widths of spectral lines.
5. The time-averaged flux of PSR1706-;44 above 100MeV is (1.0 0.3) x10 -6 photonscm -2 s -1 , where the quoted uncertainty includes both the statistics and an uncertainty from the spectral fitting.
6. Since 1975, William Livingston has been using the world's largest solar telescope, at Kitt Peak in Arizona, to study these temperature-sensitive spectral lines.
7. Especially spectacular was the veil scene where three spectral figures hang suspended above a billowing orange red cloth, held like a tent over the dancers.
8. By the late 1920s Bowen and Fowler had shown that the spectral lines of coronium, nebulium, and so on, came from excited or ionised states of ordinary elements like oxygen and nitrogen.
9. A very famous spectral hound which haunts the ancient castle of Peel on the Isle of Man.
10. The value of this information is inherently dependent upon the quality of the inference process and that in turn depends upon the complexity of the scene, the spatial, temporal and spectral resolution of the sensors and the particular algorithms used.
11. Models 1650/1650(F) are available with a spectral range of 7800-;350 cm -1 and 7800-;200 cm -1 respectively.
12. If the wavelength of a line produced in the observer's laboratory at A is and the wavelength of the same line observed in the spectrum of the collapsing object is then the fractional increase z= ( -) / is called the red shift of the spectral line.
13. Norman Lockyer, in 1868, had announced the existence of helium, on the basis of a spectral line in sunlight which corresponded to no known terrestrial element.