FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2254326466> ?p ?o ?g. }

• W2254326466 endingPage "095602" @default.
• W2254326466 startingPage "095602" @default.
• W2254326466 abstract "The hydrocarbon impurities formation is inevitable due to wall erosion in a long pulse high performance scenario with carbon-based plasma facing materials in fusion devices. The standard procedure to determine the chemical erosion yield in situ is by means of inverse photon efficiency D/XB. In this work, the conversion factor between CH4 flux and photon flux of CH A → X transition (effective inverse photon efficiency PE−1) was measured directly using a cascaded arc plasma simulator with argon/methane. This study shows that the measured PE−1 is different from the calculated D/XB. We compared the photon flux measured by optical emission spectroscopy (OES) and calculated by electron impact excitation of CH(X) which was diagnosed by cavity ring-down spectroscopy (CRDS). It seems that charge exchange and dissociative recombination processes are the main channels of CH(A) production and removal which lead to the inconsistency of PE −1 and D/XB at lower temperature. Meanwhile, the fraction of excited CH(A) produced by dissociative recombination processes was investigated, and we found it increased with Te in the range from 4% to 13% at Te < 1 eV. Our work suggests that the CH spectroscopy should be reinterpreted and the conversion factor should have a new definition instead of D/XB since the electron impact excitation is not the only channel of CH(A) production. These results have an effect on evaluating the yield of chemical erosion in divertor of fusion device." @default.
• W2254326466 created "2016-06-24" @default.
• W2254326466 creator A5021259386 @default.
• W2254326466 creator A5039913940 @default.
• W2254326466 creator A5044784619 @default.
• W2254326466 creator A5047251766 @default.
• W2254326466 creator A5047504020 @default.
• W2254326466 creator A5082599988 @default.
• W2254326466 date "2015-08-11" @default.
• W2254326466 modified "2023-10-16" @default.
• W2254326466 title "Study of the effective inverse photon efficiency using optical emission spectroscopy combined with cavity ring-down spectroscopy approach" @default.
• W2254326466 cites W1487722713 @default.
• W2254326466 cites W1965450018 @default.
• W2254326466 cites W1965928841 @default.
• W2254326466 cites W1973810814 @default.
• W2254326466 cites W1983308909 @default.
• W2254326466 cites W1999412225 @default.
• W2254326466 cites W1999877148 @default.
• W2254326466 cites W2010366863 @default.
• W2254326466 cites W2016962528 @default.
• W2254326466 cites W2031726982 @default.
• W2254326466 cites W2040353785 @default.
• W2254326466 cites W2045942281 @default.
• W2254326466 cites W2046691477 @default.
• W2254326466 cites W2050008357 @default.
• W2254326466 cites W2060784459 @default.
• W2254326466 cites W2063247984 @default.
• W2254326466 cites W2065144024 @default.
• W2254326466 cites W2074806323 @default.
• W2254326466 cites W2075817808 @default.
• W2254326466 cites W2081926331 @default.
• W2254326466 cites W2086407781 @default.
• W2254326466 cites W2091254779 @default.
• W2254326466 cites W2093563833 @default.
• W2254326466 cites W2104131430 @default.
• W2254326466 cites W2138817695 @default.
• W2254326466 cites W2141193438 @default.
• W2254326466 cites W2146965210 @default.
• W2254326466 cites W2154502383 @default.
• W2254326466 cites W2156624310 @default.
• W2254326466 cites W2198991575 @default.
• W2254326466 cites W2237602898 @default.
• W2254326466 cites W594458546 @default.
• W2254326466 doi "https://doi.org/10.1088/0031-8949/90/9/095602" @default.
• W2254326466 hasPublicationYear "2015" @default.
• W2254326466 type Work @default.
• W2254326466 sameAs 2254326466 @default.
• W2254326466 citedByCount "1" @default.
• W2254326466 countsByYear W22543264662019 @default.
• W2254326466 crossrefType "journal-article" @default.
• W2254326466 hasAuthorship W2254326466A5021259386 @default.
• W2254326466 hasAuthorship W2254326466A5039913940 @default.
• W2254326466 hasAuthorship W2254326466A5044784619 @default.
• W2254326466 hasAuthorship W2254326466A5047251766 @default.
• W2254326466 hasAuthorship W2254326466A5047504020 @default.
• W2254326466 hasAuthorship W2254326466A5082599988 @default.
• W2254326466 hasConcept C120665830 @default.
• W2254326466 hasConcept C121332964 @default.
• W2254326466 hasConcept C155552310 @default.
• W2254326466 hasConcept C159317903 @default.
• W2254326466 hasConcept C178790620 @default.
• W2254326466 hasConcept C184779094 @default.
• W2254326466 hasConcept C185592680 @default.
• W2254326466 hasConcept C192562407 @default.
• W2254326466 hasConcept C207467116 @default.
• W2254326466 hasConcept C2524010 @default.
• W2254326466 hasConcept C2780378348 @default.
• W2254326466 hasConcept C32891209 @default.
• W2254326466 hasConcept C33923547 @default.
• W2254326466 hasConcept C41999313 @default.
• W2254326466 hasConcept C62520636 @default.
• W2254326466 hasConceptScore W2254326466C120665830 @default.
• W2254326466 hasConceptScore W2254326466C121332964 @default.
• W2254326466 hasConceptScore W2254326466C155552310 @default.
• W2254326466 hasConceptScore W2254326466C159317903 @default.
• W2254326466 hasConceptScore W2254326466C178790620 @default.
• W2254326466 hasConceptScore W2254326466C184779094 @default.
• W2254326466 hasConceptScore W2254326466C185592680 @default.
• W2254326466 hasConceptScore W2254326466C192562407 @default.
• W2254326466 hasConceptScore W2254326466C207467116 @default.
• W2254326466 hasConceptScore W2254326466C2524010 @default.
• W2254326466 hasConceptScore W2254326466C2780378348 @default.
• W2254326466 hasConceptScore W2254326466C32891209 @default.
• W2254326466 hasConceptScore W2254326466C33923547 @default.
• W2254326466 hasConceptScore W2254326466C41999313 @default.
• W2254326466 hasConceptScore W2254326466C62520636 @default.
• W2254326466 hasFunder F4320321001 @default.
• W2254326466 hasIssue "9" @default.
• W2254326466 hasLocation W22543264661 @default.
• W2254326466 hasOpenAccess W2254326466 @default.
• W2254326466 hasPrimaryLocation W22543264661 @default.
• W2254326466 hasRelatedWork W1472647907 @default.
• W2254326466 hasRelatedWork W1971159631 @default.
• W2254326466 hasRelatedWork W2038902679 @default.
• W2254326466 hasRelatedWork W2051866706 @default.
• W2254326466 hasRelatedWork W2064349215 @default.
• W2254326466 hasRelatedWork W2082356131 @default.
• W2254326466 hasRelatedWork W2090740766 @default.

• next