balmer series造句

例句与造句

1. Designations from the early Balmer Series are in parentheses.
2. The Bohr assumptions recover the observed Balmer series.
3. The solution for the hydrogen atom describes standing waves of energy exactly given by the Balmer series.
4. Rydberg managed to find a formula to match the known Balmer series emission lines, and also predicted those not yet discovered.
5. Urey and grating spectrograph, a sensitive device that had been recently installed at Columbia and was capable of resolving the Balmer series.
6. It's difficult to find balmer series in a sentence. 用balmer series造句挺难的
7. At the limit of the Balmer series a change happens where at shorter wavelengths more bound-bound Balmer series transitions cause more opacity.
8. At the limit of the Balmer series a change happens where at shorter wavelengths more bound-bound Balmer series transitions cause more opacity.
9. Urey and his colleague George Murphy calculated the redshift of heavy hydrogen from the Balmer series and observed very faint lines on a spectrographic study.
10. I'm not entirely sure, but since 365.1nm is in the visible light spectrum that means it's in the Balmer series?
11. Emission lines of hydrogen ( mainly of the Lyman series and Balmer series ), helium, carbon, magnesium, iron and oxygen are the brightest lines.
12. The spectrum of WR 42e shows many characteristics of an OIf * star, such as hydrogen Balmer series absorption lines and emission lines of ionised nitrogen and helium.
13. The visual spectrum of Vega is dominated by absorption lines of hydrogen; specifically by the hydrogen Balmer series with the electron at the n = 2 principal quantum number.
14. The solution of this equation for atoms led to the explanation of the Balmer series for atomic spectra and consequently formed a basis for all of atomic physics and chemistry.
15. Due to the prevalence of hydrogen in interstellar gas, and its relatively low energy of ionization, many emission nebulae appear red due to the strong emissions of the Balmer series.
16. The spectral classification of stars, which is primarily a determination of surface temperature, is based on the relative strength of spectral lines, and the Balmer series in particular is very important.
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