Matches in SemOpenAlex for { <https://semopenalex.org/work/W2116200490> ?p ?o ?g. }
- W2116200490 endingPage "1629" @default.
- W2116200490 startingPage "1623" @default.
- W2116200490 abstract "We have measured the polarization of fluorescence emitted by the noble gases He, Ne, Ar, Kr, and Xe following impact excitation by polarized electrons. In He, the ${3}^{3}$Pensuremath{rightarrow}${2}^{3}$S transition was studied; in the heavy noble gases the ${mathit{np}}^{5}$(n+1)p${mathrm{}}^{3}$${mathit{D}}_{3}$ensuremath{rightarrow}${mathit{np}}^{5}$(n+1)s${mathrm{}}^{3}$${mathit{P}}_{2}$ transitions were analyzed. We investigated these transitions as candidates for efficient optical electron polarimetry and found that, because of their larger excitation cross sections and analyzing power, the heavy noble gases are superior to He, which had been used previously as a polarimetric target. Several issues with regard to the implementation and accuracy of optical electron polarimetric techniques are discussed. textcopyright{} 1996 The American Physical Society." @default.
- W2116200490 created "2016-06-24" @default.
- W2116200490 creator A5025058927 @default.
- W2116200490 creator A5042924143 @default.
- W2116200490 creator A5045592732 @default.
- W2116200490 date "1996-03-01" @default.
- W2116200490 modified "2023-09-27" @default.
- W2116200490 title "Optical electron polarimetry with heavy noble gases" @default.
- W2116200490 cites W131863402 @default.
- W2116200490 cites W1481001196 @default.
- W2116200490 cites W1618278002 @default.
- W2116200490 cites W1978422142 @default.
- W2116200490 cites W1980025732 @default.
- W2116200490 cites W1986733261 @default.
- W2116200490 cites W2003685285 @default.
- W2116200490 cites W2006551790 @default.
- W2116200490 cites W2006605327 @default.
- W2116200490 cites W2011258336 @default.
- W2116200490 cites W2020501388 @default.
- W2116200490 cites W2021114988 @default.
- W2116200490 cites W2022722196 @default.
- W2116200490 cites W2023656415 @default.
- W2116200490 cites W2051282131 @default.
- W2116200490 cites W2056668781 @default.
- W2116200490 cites W2057337412 @default.
- W2116200490 cites W2059695578 @default.
- W2116200490 cites W2062311846 @default.
- W2116200490 cites W2072398603 @default.
- W2116200490 cites W2074166216 @default.
- W2116200490 cites W2077249211 @default.
- W2116200490 cites W2081827569 @default.
- W2116200490 cites W2082818018 @default.
- W2116200490 cites W2089479195 @default.
- W2116200490 cites W2091300414 @default.
- W2116200490 cites W2092319114 @default.
- W2116200490 cites W2137633940 @default.
- W2116200490 cites W4243699606 @default.
- W2116200490 cites W1971059362 @default.
- W2116200490 doi "https://doi.org/10.1103/physreva.53.1623" @default.
- W2116200490 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/9913054" @default.
- W2116200490 hasPublicationYear "1996" @default.
- W2116200490 type Work @default.
- W2116200490 sameAs 2116200490 @default.
- W2116200490 citedByCount "31" @default.
- W2116200490 countsByYear W21162004902013 @default.
- W2116200490 countsByYear W21162004902014 @default.
- W2116200490 countsByYear W21162004902015 @default.
- W2116200490 countsByYear W21162004902016 @default.
- W2116200490 countsByYear W21162004902017 @default.
- W2116200490 countsByYear W21162004902018 @default.
- W2116200490 countsByYear W21162004902020 @default.
- W2116200490 countsByYear W21162004902021 @default.
- W2116200490 crossrefType "journal-article" @default.
- W2116200490 hasAuthorship W2116200490A5025058927 @default.
- W2116200490 hasAuthorship W2116200490A5042924143 @default.
- W2116200490 hasAuthorship W2116200490A5045592732 @default.
- W2116200490 hasBestOaLocation W21162004902 @default.
- W2116200490 hasConcept C120665830 @default.
- W2116200490 hasConcept C121332964 @default.
- W2116200490 hasConcept C121530826 @default.
- W2116200490 hasConcept C147120987 @default.
- W2116200490 hasConcept C147789679 @default.
- W2116200490 hasConcept C184779094 @default.
- W2116200490 hasConcept C185544564 @default.
- W2116200490 hasConcept C185592680 @default.
- W2116200490 hasConcept C191486275 @default.
- W2116200490 hasConcept C205049153 @default.
- W2116200490 hasConcept C2778005398 @default.
- W2116200490 hasConcept C28493345 @default.
- W2116200490 hasConcept C62520636 @default.
- W2116200490 hasConcept C83581075 @default.
- W2116200490 hasConceptScore W2116200490C120665830 @default.
- W2116200490 hasConceptScore W2116200490C121332964 @default.
- W2116200490 hasConceptScore W2116200490C121530826 @default.
- W2116200490 hasConceptScore W2116200490C147120987 @default.
- W2116200490 hasConceptScore W2116200490C147789679 @default.
- W2116200490 hasConceptScore W2116200490C184779094 @default.
- W2116200490 hasConceptScore W2116200490C185544564 @default.
- W2116200490 hasConceptScore W2116200490C185592680 @default.
- W2116200490 hasConceptScore W2116200490C191486275 @default.
- W2116200490 hasConceptScore W2116200490C205049153 @default.
- W2116200490 hasConceptScore W2116200490C2778005398 @default.
- W2116200490 hasConceptScore W2116200490C28493345 @default.
- W2116200490 hasConceptScore W2116200490C62520636 @default.
- W2116200490 hasConceptScore W2116200490C83581075 @default.
- W2116200490 hasIssue "3" @default.
- W2116200490 hasLocation W21162004901 @default.
- W2116200490 hasLocation W21162004902 @default.
- W2116200490 hasLocation W21162004903 @default.
- W2116200490 hasLocation W21162004904 @default.
- W2116200490 hasOpenAccess W2116200490 @default.
- W2116200490 hasPrimaryLocation W21162004901 @default.
- W2116200490 hasRelatedWork W139106637 @default.
- W2116200490 hasRelatedWork W1615347258 @default.
- W2116200490 hasRelatedWork W2003335970 @default.
- W2116200490 hasRelatedWork W2031573763 @default.
- W2116200490 hasRelatedWork W2037544642 @default.
- W2116200490 hasRelatedWork W2090729690 @default.