SELECTIVE REFLECTION FROM MERCURY VAPOR AT HIGH PRESSURES

1957 ◽  
Vol 35 (1) ◽  
pp. 98-113 ◽  
Author(s):  
H. L. Welsh ◽  
J. A. Galt

Selective reflection from mercury vapor in the region of the 2537 Å resonance line was investigated at pressures up to 340 atm. using reflection cells of special design. The results were interpreted on the basis of the classical theory of reflection from an absorbing medium. By fitting calculated curves to the experimental reflection contours, values of the oscillator strength, f, and the damping constant, γ, were determined. The f values so obtained are density-dependent and at high pressures are approximately equal to one half the value for the free atom. As predicted by theory, the damping constant varies directly as the density of the atoms in the vapor. This result contradicts the earlier work of Welsh, Kastner, and Lauriston (1950) in which it was concluded that γ varies as the square root of the density. A subsidiary reflection maximum was observed at 2540 Å; it is attributed to Hg2 molecules which occur in relatively large concentrations at high densities. Some preliminary observations on the selective reflection at the 1850 Å resonance line were made up to 4.4 atm.

1957 ◽  
Vol 35 (1) ◽  
pp. 114-121 ◽  
Author(s):  
H. L. Welsh ◽  
J. A. Galt

The influence of the foreign gases hydrogen, helium, nitrogen, and argon on the selective reflection from mercury vapor at 2537 Å was studied at pressures up to 1500 atm. The results were interpreted on the basis of the classical theory of reflection from an absorbing medium. The damping constant was found to vary linearly with foreign gas density as predicted by collision broadening theory. Frequency shifts and collision diameters determined from selective reflection data agree fairly well with values measured in absorption by other workers.


1950 ◽  
Vol 28a (2) ◽  
pp. 93-112 ◽  
Author(s):  
H. L. Welsh ◽  
J. Kastner ◽  
A. C. Lauriston

Selective reflection from mercury and cadmium vapors in the neighborhood of the resonance lines was investigated quantitatively using incident light of continuous spectral distribution. For a given experimental arrangement the lowest vapor density (atoms per cubic centimeter) at which selective reflection could be detected at Hg 2537 Å, Cd 2288 Å, and Cd 3261 Å was inversely proportional to the oscillator strength (f-value) of the absorption line. Contours of the selective reflection of the Hg 2537 Å and Cd 2288 Å lines were obtained over a large range of vapor densities up to 80 × 1018 atoms per cc. At this density the cadmium reflection extended over several thousand cm.−1 compared to about a hundred cm.−1 for mercury. The general features of the reflection contours can be explained by the theory of reflection from an absorbing medium. Fitting a theoretical curve to the experimental reflection contour yields values of the oscillator strength and the damping constant. For Hg 2537 Å and Cd 2288 Å the f-values are 0.0268 and 1.40 respectively, in good agreement with those found by other methods. The damping constant, γ, varies as the square root of the number of atoms per cubic centimeter, indicating that the mechanism of selective reflection is not the same as that for absorption and emission. An empirical areal law for selective reflection confirms the relationship [Formula: see text]. A shift of the resonance frequency of the order of magnitude of the coupling shift calculated by Weisskopf was observed for Hg 2537 Å. Deviations from theory at both high and low pressures were observed for Cd 2288 Å. The low pressure deviation takes the form of a line of residual intensity at the resonance frequency, which may be due to a different kind of selective reflection.


1980 ◽  
Vol 21 (1) ◽  
pp. 77-81 ◽  
Author(s):  
M. Gröbel ◽  
W. Heering

1970 ◽  
Vol 48 (15) ◽  
pp. 1817-1829 ◽  
Author(s):  
P. R. Timpson ◽  
J. M. Anderson

It has been shown that the afterglow following a discharge in xenon consists of two parts: (1) the resonance line, whose intensity initially decays exponentially in agreement with Holstein's theory; (2) an accompanying distributed radiation, experimentally a continuum, extending to about 1900 a.u. The intensity of this continuum decays exponentially at the same rate as the population of the lower metastable state at all wavelengths and each pressure studied. All departures from an exponential decay seem to be caused by repopulation of states by ionic recombination and are current dependent. Electron disappearance is due to ambipolar diffusion at low pressures and ion recombination at high pressures. The value of the ambipolar diffusion coefficient indicates that the afterglow positive ion is Xe2+ for pressures greater than 0.3 Torr. No phenomena which could be due to interchange of population between metastable states have been found in xenon.


1993 ◽  
Vol 99 (3-4) ◽  
pp. 185-190 ◽  
Author(s):  
V. Vuletić ◽  
V.A. Sautenkov ◽  
C. Zimmermann ◽  
T.W. Hänsch

1971 ◽  
Vol 49 (9) ◽  
pp. 1098-1102 ◽  
Author(s):  
L. O. Dickie ◽  
F. M. Kelly

The lifetime of the second excited singlet P level of barium 6s7p1P1 has been determined from the width of the Hanle resonance of the 6s7p1P1–6s21S0 3071.58 Å resonance line. The lifetime is determined to be 13.2 ± 0.4 × 10−9 s. From this lifetime the oscillator strength of the 3072 Å transition is 0.12 ± 0.05 and that of the 6s7p1P1–6s5d1D2 4726 Å is 0.09 ± 0.04.


2001 ◽  
Vol 325 (2) ◽  
pp. 767-771 ◽  
Author(s):  
P. Bonifacio ◽  
E. Caffau ◽  
M. Centurion ◽  
P. Molaro ◽  
G. Vladilo

Sign in / Sign up

Export Citation Format

Share Document