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When flash spectra (spectra of the atmosphere during an eclipse) were first obtained, astronomers found several surprising features.
In order to quantify this effect for varying representative spectra, spectra for cloud optical thicknesses from 0 to 150 were investigated.
We quantified changes in photoreceptor and LMC output in frequency domain by comparing corresponding frequency spectra (spectra) of the photoreceptor and LMC outputs in WT and mutant flies at each second of repetitive stimulation.
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Among the simulated spectra, spectrum iii is most sensitive to dynamic heterogeneities.
Chroma varied in relation to the contrast in relative brightness in segments of the spectrum; spectra with the strongest differences between reflectance in yellow and blue or red and green (e.g., spectrum 1) gave the highest chroma values.
It allows zooming, highlighting of regions within the spectrum, spectrum reversal and display of multiple spectra.
Box-counting method was applied to compute multifractal spectrum, spectrum width Δα and spectrum difference Δf of counter surfaces.
Maximax response spectra (envelope spectra) are plotted.
a Survey spectra, b Pb 4f spectra, c Te 3d spectra, d O 1s spectra.
Their working mechanism was studied by UV vis spectra, fluorescent spectra and/or mass spectra.
Reflectance spectra, derivative spectra and continuum-removed spectra were compared in terms of predictive power.
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CEO of Professional Science Editing for Scientists @ prosciediting.com