Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...396..331d&link_type=abstract
Astronomy and Astrophysics, v.396, p.331-336 (2002)
Astronomy and Astrophysics
Astrophysics
7
Lines: Profiles, Atomic Data
Scientific paper
Stark shifts of nine doubly charged (Si III) and six triply charged (Si IV) silicon ion spectral lines have been measured in a linear, low-pressure, pulsed arc operated in O2 and SF6 discharges. Si III Stark shift values have been also calculated using the semiclassical perturbation formalism (SCPF) for electrons, protons and helium ions as perturbers. Transition probabilities of the spontaneous emission (Einstein's A values) of nine Si III transitions have been obtained using the relative line intensity ratio (RLIR) method, not applied before in Si III spectrum, and, also, calculated using the Coulomb approximation method. The measured Si IV shift and some calculated Si III shift values present the first published data in this field.
Bukvic Srdan
Dimitrijevic Milan S.
Djenize Stevan
Sreckovic A.
No associations
LandOfFree
Stark shifts and transition probabilities in Si III and Si IV spectra does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Stark shifts and transition probabilities in Si III and Si IV spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stark shifts and transition probabilities in Si III and Si IV spectra will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1889148