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Inverse wavelength

Fig. 3.20. Idealized continuum and actual fluxes measured in 50-A-wide bands of A7 stars in the Hyades open cluster with Teff = 8000 K, plotted against inverse wavelength in turn-1. Horizontal lines above the spectrum show the locations of the Johnson U, B, V pass bands and the vertical boxes show schematically the corresponding properties of the Stromgren system with central wavelengths in A. (In that system, there are actually two H/3 pass bands, one narrow and one broad, so that comparison of the two gives a measure of the strength of the line.) Some prominent spectral features are marked. Fig. 3.20. Idealized continuum and actual fluxes measured in 50-A-wide bands of A7 stars in the Hyades open cluster with Teff = 8000 K, plotted against inverse wavelength in turn-1. Horizontal lines above the spectrum show the locations of the Johnson U, B, V pass bands and the vertical boxes show schematically the corresponding properties of the Stromgren system with central wavelengths in A. (In that system, there are actually two H/3 pass bands, one narrow and one broad, so that comparison of the two gives a measure of the strength of the line.) Some prominent spectral features are marked.
Fig. 24. Inverse wavelength of reflected circularly polarized light kj1 vs. the reduced temperature T for copolymers No. 4 of Table 8 at different mole fractions xch of the chiral comonomer... Fig. 24. Inverse wavelength of reflected circularly polarized light kj1 vs. the reduced temperature T for copolymers No. 4 of Table 8 at different mole fractions xch of the chiral comonomer...
Fig. 25. Inverse wavelength of reflection LR1 vs. pressure at different temperatures for copolymer No. 4 of Table 8 (xch = 0.17)... Fig. 25. Inverse wavelength of reflection LR1 vs. pressure at different temperatures for copolymer No. 4 of Table 8 (xch = 0.17)...
Fig. 28. Inverse wavelength ,R 1 versus concentration in mole % of the chiral comonomer for induced cholesteric phases No. 4 of Table 8 at T = 0.95. Fig. 28. Inverse wavelength ,R 1 versus concentration in mole % of the chiral comonomer for induced cholesteric phases No. 4 of Table 8 at T = 0.95.
Fig. 29. Inverse wavelength of reflection LR 1 vs. concentration in mole % of the chiral component for induced cholesteric phases = copolymer No. 5, Table 8 O = monomer-polymer mixture... Fig. 29. Inverse wavelength of reflection LR 1 vs. concentration in mole % of the chiral component for induced cholesteric phases = copolymer No. 5, Table 8 O = monomer-polymer mixture...
First, we will examine some of the basic features of an infrared spectrum. Early infrared instruments recorded percentage transmittance over a linear wavelength range. It is now unusual to use wavelength for routine samples and inverse wavelength units are used. This is the wavenumber scale, and the units used are cm"i. The output from the instrument is referred to as a spectrum. Most commercial instruments present the spectrum with the wavenumber decreasing from left to right... [Pg.19]

Taking the easy case of line broadening first, one way for the lines to be so wide is if the excited state lifetimes are very short, on the order of femtoseconds. Fourier analysis indicates that the spectral line width Ap of a transition of lifetime t (ignoring factors of it) is approximately 1/t, and so the fractional line width of the line Ap/pq 1/tpo- It is more convenient to use energy units of inverse wavelength (1/A., or cm" ). Let the energy of the center frequency be given as (in cm" ) with lifetime r. The fractional line width then is... [Pg.144]

We discuss here the use of neutron reflectivity at a polymer solution-air interface, for the experimental determination of the polymer concentration profile. The method consists of analyzing the neutron reflectivity near total reflection, as a function of the incident inverse wavelength k. This method was developed at the LLB in... [Pg.255]

The method used to derive polymer concentration profiles from neutron reflectivity experiments is based on the sensitivity of the reflectivity to the isotopic composition, when one approaches total reflection. It requires a very accurate knowledge of the critical inverse wavelength, ka associated with each isotopic bulk composition. [Pg.266]

Frequency is inversely proportional to wavelength the greater the frequency the shorter the wavelength... [Pg.520]

The Wien displacement law states that the wavelength of maximum emission, A , of a blackbody varies inversely with absolute temperature the product A T remains constant. When A is expressed in micrometers, the law becomes... [Pg.727]

The first polyatomic molecule was detected in 1968 with use of a telescope having a dish 6.3 m in diameter at Hat Creek, California, USA, designed to operate in the millimetre wave region. Emission lines were found in the 1.25 cm wavelength region due to NH3. The transitions are not rotational but are between the very closely spaced 2 = 0 and 2 = 1 levels of the inversion vibration V2 (see Section 6.2.5.4). [Pg.120]

The wavelength of maximum intensity is seen to be inversely proportional to the absolute temperature. The relation is known as Wien s displacement law = (2.898)(10 ) m K. This can be... [Pg.570]

As energy is added and photons collide with other atoms, more and more electrons gain energy and jump orbits. The excited atoms all emit photons at the exact same wavelength. At some point there are more atoms with electrons in excited states than at ground level. This is population inversion. [Pg.703]


See other pages where Inverse wavelength is mentioned: [Pg.1242]    [Pg.104]    [Pg.435]    [Pg.142]    [Pg.1242]    [Pg.142]    [Pg.89]    [Pg.309]    [Pg.265]    [Pg.257]    [Pg.257]    [Pg.266]    [Pg.477]    [Pg.1242]    [Pg.104]    [Pg.435]    [Pg.142]    [Pg.1242]    [Pg.142]    [Pg.89]    [Pg.309]    [Pg.265]    [Pg.257]    [Pg.257]    [Pg.266]    [Pg.477]    [Pg.1296]    [Pg.117]    [Pg.117]    [Pg.462]    [Pg.348]    [Pg.513]    [Pg.7]    [Pg.8]    [Pg.11]    [Pg.377]    [Pg.322]    [Pg.243]    [Pg.338]    [Pg.14]    [Pg.93]    [Pg.256]    [Pg.257]    [Pg.665]    [Pg.217]    [Pg.197]    [Pg.423]   
See also in sourсe #XX -- [ Pg.256 , Pg.266 ]




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Critical inverse wavelength

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