Please use this identifier to cite or link to this item:
https://physrep.ff.bg.ac.rs/handle/123456789/174
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Djeniže, S. | en |
dc.contributor.author | Srećković, A. | en |
dc.contributor.author | Jelisavčić, M. | en |
dc.contributor.author | Bukvić, Srđan | en |
dc.date.accessioned | 2022-07-05T16:23:50Z | - |
dc.date.available | 2022-07-05T16:23:50Z | - |
dc.date.issued | 2002-01-01 | en |
dc.identifier.issn | 0004-6361 | en |
dc.identifier.uri | https://physrep.ff.bg.ac.rs/handle/123456789/174 | - |
dc.description.abstract | Stark widths and shifts of two prominent triply ionized sulfur (S IV) ultraviolet spectral lines (309.727 nm and 311.761 nm) in the 4s2S-4p2P0 transition have been measured in a linear, low-pressure, pulsed arc discharge created in a SF6 plasma at 33600 K electron temperature and at 2.8 × 1023 m-3 electron density. Presented Stark shifts are the first measurement of the line shift in the S IV spectrum. Obtained broadening parameters have been compared to the available experimental and theoretical data. The transition probability ratio of the mentioned S IV spectral lines is also obtained. | en |
dc.relation.ispartof | Astronomy and Astrophysics | en |
dc.subject | Atomic data | en |
dc.subject | Lines: profiles | en |
dc.title | Experimental Stark widths and shifts of triply ionized sulfur spectral lines | en |
dc.type | Article | en |
dc.identifier.doi | 10.1051/0004-6361:20020717 | en |
dc.identifier.scopus | 2-s2.0-0036646033 | en |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/0036646033 | en |
dc.relation.issue | 3 | en |
dc.relation.volume | 389 | en |
dc.relation.firstpage | 1086 | en |
dc.relation.lastpage | 1089 | en |
item.grantfulltext | none | - |
item.fulltext | No Fulltext | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.cerifentitytype | Publications | - |
item.openairetype | Article | - |
Appears in Collections: | Journal Article |
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