FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1979377890> ?p ?o ?g. }

• W1979377890 endingPage "435" @default.
• W1979377890 startingPage "427" @default.
• W1979377890 abstract "Analytical and fundamental characteristics of helium inductively coupled plasma mass spectrometry (He ICPMS) were explored for atmospheric-pressure plasmas generated in a 13-mm He ICP torch with the use of a prototype ICPMS equipped with an analogue detector. Four sets of operating conditions were identified for the detection of four categories of elements at levels lower than or similar to those of the Ar ICPMS. In general, detection limits of He ICPMS were improved by two to four orders of magnitude for metals, compared to results from our previous study with the same torch. For the easy-to-atomize elements (Li, Na, K, Ga, Rb, In, Cs, Tl, Pb, and Bi), the detection limits ranged from 0.1 to 7 pg/mL at 500–600 W forward power. Detection limits of the fourth-period transition metals (Cr, Mn, Fe, Co, Ni, and Cu), i.e., elements subject to the spectral interferences in Ar ICPMS, were 4 to 100 pg/mL at a power level of 560–700 W. The detection limits of hard-to-atomize elements (Ti, V, Sr, Y, Rh, Pr, Tm, Th) ranged from 4 to 90 pg/mL at 800 W. For hard-to-ionize elements (As, Se, Br, Sn Sb, I), detection limits of 0.05 to 1 ng/mL were obtained at 820 W. Ion kinetic energies were measured under two diverse sets of operating conditions. At 600 W, the ion kinetic energies were very low (2.6–6.6 eV for mass range 39–209 amu), indicating the absence of a secondary discharge at the sampler tip of the MS interface. The gas-kinetic temperature estimated in this measurement was 600 K for the 600-W He ICP. In contrast, very high ion kinetic energies (31–66 eV for mass range 51–232 amu) were obtained at 800 W. The estimated plasma potential and gas kinetic temperature were 22 V and 3500 K, respectively. Ion kinetic energies of polyatomic ions were slightly lower than those of atomic ions at the same mass, suggesting that polyatomic ions were formed in the low-temperature zones of the He ICP." @default.
• W1979377890 created "2016-06-24" @default.
• W1979377890 creator A5009889404 @default.
• W1979377890 creator A5049341927 @default.
• W1979377890 creator A5059880056 @default.
• W1979377890 creator A5073956556 @default.
• W1979377890 date "1996-04-01" @default.
• W1979377890 modified "2023-10-05" @default.
• W1979377890 title "Atmospheric-Pressure Helium Inductively Coupled Plasmas for Elemental Mass Spectrometry" @default.
• W1979377890 cites W1654191379 @default.
• W1979377890 cites W1966553037 @default.
• W1979377890 cites W1974300681 @default.
• W1979377890 cites W1980656182 @default.
• W1979377890 cites W1980834546 @default.
• W1979377890 cites W1981067890 @default.
• W1979377890 cites W1982924569 @default.
• W1979377890 cites W1985743606 @default.
• W1979377890 cites W1988940826 @default.
• W1979377890 cites W1992056652 @default.
• W1979377890 cites W1997933879 @default.
• W1979377890 cites W1998688722 @default.
• W1979377890 cites W2003200845 @default.
• W1979377890 cites W2004010074 @default.
• W1979377890 cites W2004217919 @default.
• W1979377890 cites W2006370450 @default.
• W1979377890 cites W2008123511 @default.
• W1979377890 cites W2010291336 @default.
• W1979377890 cites W2014122781 @default.
• W1979377890 cites W2015044678 @default.
• W1979377890 cites W2023673781 @default.
• W1979377890 cites W2024125096 @default.
• W1979377890 cites W2042334593 @default.
• W1979377890 cites W2042943049 @default.
• W1979377890 cites W2044961540 @default.
• W1979377890 cites W2052330051 @default.
• W1979377890 cites W2053564511 @default.
• W1979377890 cites W2054869078 @default.
• W1979377890 cites W2057370662 @default.
• W1979377890 cites W2065241992 @default.
• W1979377890 cites W2065786072 @default.
• W1979377890 cites W2072447967 @default.
• W1979377890 cites W2072510398 @default.
• W1979377890 cites W2074674909 @default.
• W1979377890 cites W2083745434 @default.
• W1979377890 cites W2085850515 @default.
• W1979377890 cites W2086050505 @default.
• W1979377890 cites W2089403163 @default.
• W1979377890 cites W2149469665 @default.
• W1979377890 cites W2154136499 @default.
• W1979377890 cites W2170377618 @default.
• W1979377890 cites W2482607623 @default.
• W1979377890 doi "https://doi.org/10.1366/0003702963906140" @default.
• W1979377890 hasPublicationYear "1996" @default.
• W1979377890 type Work @default.
• W1979377890 sameAs 1979377890 @default.
• W1979377890 citedByCount "29" @default.
• W1979377890 countsByYear W19793778902020 @default.
• W1979377890 crossrefType "journal-article" @default.
• W1979377890 hasAuthorship W1979377890A5009889404 @default.
• W1979377890 hasAuthorship W1979377890A5049341927 @default.
• W1979377890 hasAuthorship W1979377890A5059880056 @default.
• W1979377890 hasAuthorship W1979377890A5073956556 @default.
• W1979377890 hasConcept C113196181 @default.
• W1979377890 hasConcept C119128265 @default.
• W1979377890 hasConcept C121332964 @default.
• W1979377890 hasConcept C135889238 @default.
• W1979377890 hasConcept C145148216 @default.
• W1979377890 hasConcept C153294291 @default.
• W1979377890 hasConcept C162356407 @default.
• W1979377890 hasConcept C165697059 @default.
• W1979377890 hasConcept C1700975 @default.
• W1979377890 hasConcept C178790620 @default.
• W1979377890 hasConcept C184779094 @default.
• W1979377890 hasConcept C185544564 @default.
• W1979377890 hasConcept C185592680 @default.
• W1979377890 hasConcept C200239111 @default.
• W1979377890 hasConcept C43617362 @default.
• W1979377890 hasConcept C546029482 @default.
• W1979377890 hasConcept C62520636 @default.
• W1979377890 hasConcept C82706917 @default.
• W1979377890 hasConcept C95974651 @default.
• W1979377890 hasConceptScore W1979377890C113196181 @default.
• W1979377890 hasConceptScore W1979377890C119128265 @default.
• W1979377890 hasConceptScore W1979377890C121332964 @default.
• W1979377890 hasConceptScore W1979377890C135889238 @default.
• W1979377890 hasConceptScore W1979377890C145148216 @default.
• W1979377890 hasConceptScore W1979377890C153294291 @default.
• W1979377890 hasConceptScore W1979377890C162356407 @default.
• W1979377890 hasConceptScore W1979377890C165697059 @default.
• W1979377890 hasConceptScore W1979377890C1700975 @default.
• W1979377890 hasConceptScore W1979377890C178790620 @default.
• W1979377890 hasConceptScore W1979377890C184779094 @default.
• W1979377890 hasConceptScore W1979377890C185544564 @default.
• W1979377890 hasConceptScore W1979377890C185592680 @default.
• W1979377890 hasConceptScore W1979377890C200239111 @default.
• W1979377890 hasConceptScore W1979377890C43617362 @default.
• W1979377890 hasConceptScore W1979377890C546029482 @default.
• W1979377890 hasConceptScore W1979377890C62520636 @default.

• next