Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/960
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dc.contributor.authorVasiljević, Milica M.en
dc.contributor.authorSpasojević, Djordjeen
dc.contributor.authorŠišović, Nikola M.en
dc.contributor.authorKonjević, Nikolaen
dc.date.accessioned2022-07-12T17:56:41Z-
dc.date.available2022-07-12T17:56:41Z-
dc.date.issued2017-09-01en
dc.identifier.issn0295-5075en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/960-
dc.description.abstractWe present a study of argon glow discharge which shows that measured wavenumber DC Stark shifts Δν of two neutral argon lines, Ar I 518.75nm and Ar I 522.127 nm, can be used for reliable determination of the electric field strength F distribution in the cathode sheath region of the discharge. In order to experimentally determine the coefficient c in quadratic correlation Δν = cF2, manifested in a low field range (up to 15 kV/cm), the discharge is seeded with a small admixture of hydrogen, and the values of F are measured via Stark polarization spectroscopy of the hydrogen Balmer beta line. Once known, this can be used for the determination of F by a simple and inexpensive spectroscopic Stark shift measurement in discharges with other argon admixtures or pure argon. Reported shift results are in good agreement with data extrapolated from measurements performed at high electric fields (over 100 kV/cm) by Windholz (Phys. Scr., 21 (1980) 67).en
dc.relation.ispartofEPLen
dc.titleStark effect of Ar i lines for electric field strength diagnostics in the cathode sheath of glow dischargeen
dc.typeArticleen
dc.identifier.doi10.1209/0295-5075/119/55001en
dc.identifier.scopus2-s2.0-85040067722en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85040067722en
dc.relation.issue5en
dc.relation.volume119en
item.openairetypeArticle-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.orcid0000-0003-2177-530X-
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