Stark Broadening of Se IV, Sn IV, Sb IV and Te IV Spectral Lines

Stark Broadening of Se IV, Sn IV, Sb IV and Te IV Spectral Lines

Stark broadening parameters, line width and shift, are needed for investigations, analysis and modelling of astrophysical, laboratory, laser produced and technological plasmas. Especially in astrophysics, due to constantly increasing resolution of satellite borne spectrographs, and large terrestrial...

Full description

Bibliographic Details
Main Authors: Milan S. Dimitrijević, Zoran Simić, Roland Stamm, Joël Rosato, Nenad Milovanović, Cristina Yubero
Format: Article
Language:English
Published: MDPI AG 2018-03-01
Series:Atoms
Subjects:
Stark broadening
line profiles
atomic data
Online Access:http://www.mdpi.com/2218-2004/6/1/10

Internet

http://www.mdpi.com/2218-2004/6/1/10

Similar Items