Absolute intensity measurements of Brillouin spectra of liquid and solid krypton, and determination of the elasto-optic constants

1975 ◽  
Vol 11 (10) ◽  
pp. 3984-3989 ◽  
Author(s):  
Yoshiaki Kato ◽  
B. P. Stoicheff
1973 ◽  
Vol 95 (19) ◽  
pp. 6182-6190 ◽  
Author(s):  
R. F. Curl ◽  
Tatsuya. Ikeda ◽  
R. S. Williams ◽  
Sharron. Leavell ◽  
L. H. Scharpen

1973 ◽  
Vol 4 (47) ◽  
pp. no-no
Author(s):  
R. F. CURL ◽  
TATSUYA IKEDA ◽  
R. S. WILLIAMS ◽  
SHARRON LEAVELL ◽  
L. H. SCHARPEN

1964 ◽  
Vol 17 (2) ◽  
pp. 200
Author(s):  
V Metchnik

The measurements of the absolute intensities of Ou Ka radiation, isolated by means of balanced nickel and iron filters,. necessitated the determination of the quantum counting efficiency of three types of detectors: an end� window argon-filled Geiger counter, a two side-window, xenon-filled proportional counter, and a scintillation counter with NaITI crystal. It is shown that, provided the necessary corrections are made, results of absolute intensity measurements obtained with these three detectors show good agreement.


1997 ◽  
Vol 51 (6) ◽  
pp. 778-784 ◽  
Author(s):  
M. C. Quintero ◽  
A. Rodero ◽  
M. C. García ◽  
A. Sola

This paper analyzes the influence of the departure from thermodynamic equilibrium on three spectroscopic methods for determining the excitation temperature: the classical Boltzmann plot method, the method of absolute intensity measurements, and the method of the ratio of atomic to ionic lines for one element. Use of these methods is illustrated with experiments conducted in a helium microwave plasma in nonthermodynamic equilibrium produced by an axial injection torch at atmospheric pressure. The excitation temperature was determined at a variable microwave power and different positions along the flame. The results are discussed in terms of the atomic-state distribution function (ASDF) calculated for the plasma.


1965 ◽  
Vol 23 ◽  
pp. 29-30
Author(s):  
H. E. Hinteregger

Experimental problems of absolute intensity measurements of solar electromagnetic radiation in the extreme ultra-violet (EUV) and soft X-ray region of the spectrum (designated cumulatively as “XUV” for brevity) are reviewed. From an evaluation of existing rocket and satellite data together with existing projects and goals of future observations from space vehicles, it is suggested that the numerous associated practical problems be devided into two major areas, namely (a) the general experimental art of heterochromatic absolute XUV spectrophotometry in the laboratory and (b) specific problems characteristic of the objectives of solar physics as well as existing restrictions of space technology. Within the first area (a) emphasis is placed on recent progress toward justified reliance on ionization detectors without necessary connection to source standards. For the second area (b), emphasis is placed on the immediate need to have existing exploratory observations followed by a new phase of more systematic experiments of increased accuracy.


2012 ◽  
Vol 43 (9) ◽  
pp. 1293-1298 ◽  
Author(s):  
A. Lucotti ◽  
M. Tommasini ◽  
D. Fazzi ◽  
M. Del Zoppo ◽  
W. A. Chalifoux ◽  
...  

1970 ◽  
Vol 25 (11) ◽  
pp. 1617-1626 ◽  
Author(s):  
H. Frank ◽  
M. Neiger ◽  
H.-P. Popp

Abstract A wall stabilized low-current cylindric arc was used to produce the radiation of the negative Bromine-ions. The radiation consists of an affinity-continuum with a long-wave threshold of 3682 Å, yielding an electron affinity for Bromine of 3.366 eV, and of an intense electron-atom Bremsstrahlung in the visible. Intensity measurements of the continua allow the determination of the photo-detachment-and attachment-cross-sections of Bromine and also the determination of the mean elastic cross-section of electrons against Bromine atoms.


Sign in / Sign up

Export Citation Format

Share Document