Theoretical study of the D̃→C̃ emission spectrum of NO2

2008 ◽  
Vol 129 (12) ◽  
pp. 124303 ◽  
Author(s):  
R. Schinke
Keyword(s):  
Emission Spectrum ◽  
Theoretical Study

Theoretical study of the X-ray Kβ emission spectrum of an argon atom

2007 ◽  
Vol 103 (4) ◽  
pp. 513-520
Author(s):  
A. N. Khoperskiĭ ◽  
A. M. Nadolinskiĭ ◽  
V. A. Yavna ◽  
A. S. Kasprzhitskiĭ
Keyword(s):  
Emission Spectrum ◽  
Theoretical Study ◽  
Argon Atom ◽  
X Ray

Intensities and spin decoupling in the ScO emission spectrum

1977 ◽  
Vol 55 (2) ◽  
pp. 180-188 ◽  
Author(s):  
J.-L. Féménias ◽  
J. P. Goure ◽  
R. Stringat
Keyword(s):  
Emission Spectrum ◽  
Intensity Distribution ◽  
Theoretical Study ◽  
Great Influence ◽  
Spectrometric Data ◽  
Mixing Coefficients

Previous work on the theoretical study of the intensity distribution in the emission spectrum of ScO is now extended and a comparison is made with some experimental spectrometric data, and some physical results such as the temperature of emission and the 'spin allowed' property of the A2Π → X2Σ transition are given and discussed. The great influence of the slight spin decoupling of the A2Π (case (a)) state on the intensity distribution is shown and is explained theoretically using the mixing coefficients obtained in a former rotational study of the spectrum.

Theoretical study of the HPCl emission spectrum: re-assignment of the vibrational progressions and comparison with HNCl

2003 ◽  
Vol 289 (2-3) ◽  
pp. 263-274 ◽  
Author(s):  
I Baraille ◽  
C Larrieu ◽  
A Dargelos ◽  
M Chaillet
Keyword(s):  
Emission Spectrum ◽  
Theoretical Study

Models of Thermodynamic Properties of Prominences

1979 ◽  
Vol 44 ◽  
pp. 349-355
Author(s):  
R.W. Milkey
Keyword(s):  
Thermodynamic Properties ◽  
Mass Transport ◽  
Emission Spectrum ◽  
Thermodynamic Parameters ◽  
Working Group ◽  
Physical Processes ◽  
Theoretical Concepts ◽  
Group 3 ◽  
Observational Techniques

The focus of discussion in Working Group 3 was on the Thermodynamic Properties as determined spectroscopically, including the observational techniques and the theoretical modeling of physical processes responsible for the emission spectrum. Recent advances in observational techniques and theoretical concepts make this discussion particularly timely. It is wise to remember that the determination of thermodynamic parameters is not an end in itself and that these are interesting chiefly for what they can tell us about the energetics and mass transport in prominences.

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