Stark Broadening of Se IV, Sn IV, Sb IV and Te IV Spectral Lines
Autor
Dimitrijević, Milan S.
Simić, Zoran
Stamm, Roland
Rosato, Joël
Milovanović, Nenad
Yubero, Cristina
Editor
MDPIFecha
2018Materia
Stark broadeningLine profiles
Atomic data
METS:
Mostrar el registro METSPREMIS:
Mostrar el registro PREMISMetadatos
Mostrar el registro completo del ítemResumen
Stark broadening parameters, line width and shift, are needed for investigations, análisis 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 telescopes, data on trace elements, which were previously insignificant, now have increasing importance. Using the modified semiempirical method of Dimitrijević and Konjević, here, Stark widths have been calculated for 2 Se IV, 6 Sn IV, 2 Sb IV and 1 Te IV transitions. Results have been compared with existing theoretical data for Sn IV. Obtained results will be implemented in the STARK-B database, which is also a part of Virtual atomic and molecular data center (VAMDC).