spectral line intensity
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2017 ◽  
Vol 362 (7) ◽  
Author(s):  
N. A. Silant’ev ◽  
G. A. Alekseeva ◽  
V. V. Novikov

2015 ◽  
Vol 30 (10) ◽  
pp. 2107-2119 ◽  
Author(s):  
Jung-Hwan In ◽  
Chan-Kyu Kim ◽  
Sungho Jeong

The precision of laser induced breakdown spectroscopy (LIBS) measurement is analyzed in consideration of both the shot noise of the detector and the shot-to-shot fluctuation noise of the laser plasma.


2014 ◽  
Vol 10 (S305) ◽  
pp. 401-406
Author(s):  
A. Tichý ◽  
J. Štěpán ◽  
J. Trujillo Bueno ◽  
J. Kubát

AbstractWe study the problem of the generation and transfer of spectral line intensity and polarization in models of stellar atmospheres with horizontal plasma inhomogeneities. We solve the non-LTE radiative transfer problem in full 3D geometry taking into account resonant scattering polarization and its modification by magnetic fields via the Hanle effect. We show that horizontal fluctuations of the thermodynamical conditions of stellar atmospheres can have a significant impact on the linear polarization of the emergent spectral line radiation and its center-to-limb variation.


1999 ◽  
Vol 70 (2) ◽  
pp. 1425-1429 ◽  
Author(s):  
A. Lorenz ◽  
N. J. Peacock ◽  
M. G. O’Mullane ◽  
David Neely

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