Theoretical Line Intensities. III. Solar UV Lines and Continua of h, he i, and he II and the Chromospheric Model

1965 ◽  
Vol 142 ◽  
pp. 755 ◽  
Author(s):  
R. Grant Athay
Keyword(s):  
Line Intensities ◽  
Theoretical Line ◽  
Solar Uv

Symmetry effects in rotationally resolved spectra of bi-deuterated ethylene: Theoretical line intensities of cis, trans, and as-C2H2D2 isotopomers

2019 ◽  
Vol 150 (19) ◽  
pp. 194303 ◽  
Author(s):  
Dominika Viglaska ◽  
Michael Rey ◽  
Andrei V. Nikitin ◽  
Vladimir G. Tyuterev
Keyword(s):  
Line Intensities ◽  
Theoretical Line

scholarly journals Theoretical line intensities and spectrum of τ: Scorpii.

1956 ◽  
Vol 61 ◽  
pp. 1
Author(s):  
L. H. Aller ◽  
G. Elste ◽  
J. Jugaku
Keyword(s):  
Line Intensities ◽  
Theoretical Line

EXCITATION CONDITIONS IN THE UPPER ATMOSPHERE AS DETERMINED FROM A STUDY OF ATOMIC EMISSION LINES IN THE AURORAL SPECTRUM

1947 ◽  
Vol 25a (5) ◽  
pp. 293-301 ◽  
Author(s):  
William Petrie
Keyword(s):  
Oxygen Atom ◽  
Atomic Emission ◽  
Upper Atmosphere ◽  
Emission Lines ◽  
Excitation Temperature ◽  
Auroral Region ◽  
Line Intensities ◽  
Theoretical Line ◽  
Measured Line ◽  
Excitation Conditions

Vegard's identifications of a number of lines appearing in the auroral spectrum are discussed. The conclusion is reached that a good many of these lines may be attributed to the oxygen atom in several stages of ionization. It is shown how measured line intensities and theoretical line strengths are combined to give the excitation temperature of the auroral region. Preliminary results indicate that this temperature is in the range 3000° to 6000° K. The meaning of this result is discussed briefly.

Theoretical Line Intensities and the Spectrum of Tau Scorpii

1956 ◽  
Vol 68 ◽  
pp. 23 ◽  
Author(s):  
Günther Elste ◽  
Jun Jugaku ◽  
L. H. Aller
Keyword(s):  
Line Intensities ◽  
Theoretical Line
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