W.F. Meggers, C.H. Corliss and B.F. Scribner, Tables of Spectral-Line Intensities Part I, Arranged by Elements; Part II, Arranged by Wavelength, National Bureau of Standards Monograph 32 (1985), p. 485 Part I.Part II, 284 pp., $3.00.(Available from the Superintendent of Documents, U.S. Government Printing Office, Washington 25, D.C., U.S.A.

1962 ◽  
Vol 18 (4) ◽  
pp. 1476-1476
Author(s):  
E DEKALB
Keyword(s):  
Spectral Line ◽  
Government Printing ◽  
National Bureau ◽  
Line Intensities

On the Inhomogeneity of Chemical Composition over the Surface of 21 Per

1976 ◽  
Vol 32 ◽  
pp. 343-349
Author(s):  
Yu.V. Glagolevsky ◽  
K.I. Kozlova ◽  
V.S. Lebedev ◽  
N.S. Polosukhina
Keyword(s):  
Chemical Composition ◽  
Spectral Line ◽  
Variable Star ◽  
Radial Velocities ◽  
Crimean Astrophysical Observatory ◽  
Line Intensities ◽  
Magnetic Variable

SummaryThe magnetic variable star 21 Per has been studied from 4 and 8 Å/mm spectra obtained with the 2.6 - meter reflector of the Crimean Astrophysical Observatory. Spectral line intensities (Wλ) and radial velocities (Vr) have been measured.

Atomic data and spectral line intensities for Ni XVII

2011 ◽  
Vol 97 (3) ◽  
pp. 189-224 ◽  
Author(s):  
A.K. Bhatia ◽  
E. Landi
Keyword(s):  
Spectral Line ◽  
Atomic Data ◽  
Line Intensities

scholarly journals Excitation and analytical characteristics of an ethanol loaded U-shaped arc

2003 ◽  
Vol 68 (2) ◽  
pp. 109-118 ◽  
Author(s):  
Marija Raskovic ◽  
Ivanka Holclajtner-Antunovic ◽  
Mirjana Tripkovic ◽  
Dragan Markovic
Keyword(s):  
Spectral Line ◽  
Electron Number Density ◽  
Ethanol Solution ◽  
Number Density ◽  
Electron Number ◽  
Plasma Parameters ◽  
Line Intensities ◽  
Ethanol Addition ◽  
Plasma Characteristics ◽  
Dc Arc

The effect of the ethanol load on the discharge and analytical parameters of an argon stabilized U-shaped DC arc has been recorded. Measurements of the radial distribution of the apparent temperatures and the electron number density of the DC plasma showed that ethanol addition causes a decrease in both plasma parameters. The changes in the plasma characteristics, as well as in transport and atomisation processes of the analyte cause a general change in the spectral line intensities, which depends on the physical characteristics of the analyte and the quantity of ethanol loaded into the plasma. Improved detection limits were obtained for V and Mn when a 10%(v/v) water?ethanol solution was nebulized into the plasma.

scholarly journals Tables of spectral-line intensities :

1961 ◽  
Author(s):  
William F Meggers ◽  
Charles H Corliss ◽  
Bourdon F Scribner
Keyword(s):  
Spectral Line ◽  
Line Intensities
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