These emissions are more or less degraded for short wavelengths as the emission spectrum of the ( B?! X ) line shows in figure 13.
32.
Due to its high sensitivity to the mobility and presence of solvent dipoles, changes in the emission spectrum can be calculated from the generalized polarization.
33.
By analyzing the width of each spectral line in an emission spectrum, both the elements present in a star and their relative abundances can be determined.
34.
The inner filter effects change the spectrum and intensity of the emitted light and they must therefore be considered when analysing the emission spectrum of fluorescent light.
35.
Various models propose that the quantization predicted by Karlsson's formula is related to the emission spectrum signature of hydrogen, described by the Lyman series.
36.
The peak of the emission spectrum occurs at 1.29 eV for Yb 2 O 3 and 0.827 eV for Er 2 O 3.
37.
AE And has prominent allowed and forbidden Fe II and hydrogen lines in its emission spectrum, as well as weaker He I and N II lines.
38.
Paschen notation is somewhat weird notation; it is an old notation made to attempt to fit an emission spectrum of Ne to a hydrogen-like theory.
39.
The emission spectrum of atomic hydrogen is divided into a number of "'spectral series "', with wavelengths given by the Rydberg formula.
40.
The light from a source can consist of a continuous spectrum, an emission spectrum ( bright lines ), or an absorption spectrum ( dark lines ).
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